Instruction Manual
ETX-90AT Astro TelescopeETX-105AT Astro TelescopeETX-125AT Astro Telescope

CONTENTSWARNING!
Never use a Meade ETX Astro Telescope
to look at the Sun! Looking at or near the
Sun will cause instant and irreversible
damage to your eye. Eye damage is often
painless, so there is no warning to theobserver that damage has occurred until it is
too late. Do not point the telescope or its
viewfinder at or near the Sun. Do not lookthrough the telescope or its viewfinder as it ismoving. Children should always have adultsupervision while observing.
®

®

Caution: Use care to install batteries in theorientation indicated by illustration in thebattery slots of the battery compartment.
Follow battery manufacturer's precautions.
Do not install batteries backwards or mix
new and used batteries. Do not mix battery
types. If these precautions are not followed,
batteries may explode, catch fire or leak.
Improperly installed batteries void your
Meade warranty.

If you are anxious to use your telescope
for the first time, read the QUICK-STARTGUIDE on pages 4 and 5.

® The name "Meade," “ETX,” “Autostar” and the Meade logo
are trademarks registered with the U.S. Patent Office and inprincipal countries throughout the world.
Patents:
US 6,304,376
US 6,392,799
US 6,563,636
D 422,610
Patent Pending© 2004 Meade Instruments Corporation.

Quick-Start Guide .......................................................... 4
Telescope Features ...................................................... 6
Autostar Features .......................................................... 9
Getting Started ..............................................................12Parts Listing ..............................................................12
How to Assemble Your Telescope & Tripod ..............12
Attaching and Using the Viewfinder ..........................13
Focusing and Aligning the Viewfinder ......................14
Choosing an Eyepiece ..............................................15
Observing ......................................................................16
Observing by Moving the Telescope Manually ........16
Terrestrial Observing ................................................16
Observing Using Autostar's Arrow Keys ..................16
Slew Speeds ............................................................17
Astronomical Observing, Observe the Moon ............17
To Track an Object Automatically..............................17
Moving Through Autostar’s Menus......................17
Initializing Autostar ..............................................18
Easy (Two-Star) Align ..........................................18
Observe a Star Using Automatic Tracking ..........20
Go To Saturn ............................................................20
Using the Guided Tour ..............................................21
Basic Autostar Operation................................................22
Autostar Navigation Exercise ....................................22
Entering Data, Navigating Autostar ..........................23
Autostar Menus ............................................................24
Menu Tree ................................................................24
Objects Menu ............................................................25
Event Menu, Glossary Menu ....................................26
Utilities Menu ............................................................27
Setup Menu ..............................................................28
Advanced Autostar Features ..........................................31
Adding Observing Sites ............................................31
Finding Objects Not in the Database ........................32
Observing Satellites ..................................................32
Create Your Own Guided Tour..................................33
Landmarks ................................................................36
Identify ......................................................................37
Advanced Alt/Az Alignment Methods ........................38
Browse ......................................................................39
Photography ..................................................................40
Photography with Autostar Suite ..............................42
Optional Accessories ......................................................43
Maintenance ..................................................................45
Troubleshooting ......................................................46
Specifications ................................................................48
Appendix A: Equatorial (Polar) Alignment ......................51
Equatorial Alignment, Celestial Coordinates ............51
Polar Mounting with #884 Deluxe Field Tripod ........51
Equatorial Mounting Procedure ................................52
To Track a Star When Polar Mounted ......................52
Autostar Polar Alignment Modes ..............................53
Locating the Celestial Pole ......................................53
Setting Circles ..........................................................54
Appendix B: Latitude Chart ............................................55
Appendix C: Training the Drive ......................................56
Appendix D: Basic Astronomy ........................................57

QUICK-START GUIDEThis Quick Start Guide demonstrates how to install the batteries and eyepiece, and how to observe using the Autostar Arrow keys.
If you wish to try out Autostar’s “Go To” capabilities, check out the list of page references at the bottom of the following page.

2

B

B
H

A
®

Remove the ETX telescope from its packaging and place
it on a sturdy surface. Place the ETX on its side andremove the battery compartment cover (A) from the underside of the drive base. Insert eight (user-supplied) AA-size
batteries into the battery compartment (B) oriented asshown in the battery compartment. Replace the cover andreturn the telescope to an upright position (if you wish toattach the telescope to the deluxe field tripod, see page
12).

C...and the other end of the coiled cord into the coiled cord
port at the bottom of Autostar handbox (H), as shown above.

C
D
E
I

J

Tighten (to a "firm feel" only, do not overtighten) the vertical lock(I) and the horizontal lock (J). See page 7 and 8 for more information.

Place the 26mm eyepiece (C) into the eyepiece holder on
the telescope and tighten the attachment thumbscrew (D) toa "firm feel" only. See page 7, for more information.
Remove the dust cover (E) from the end of the telescope
tube.

D
F

F

G

Make sure that the computer control panel power switch(F) is in the OFF position. Remove the Autostar handbox
and the coiled cord from the packing materials. Plug one
end of the cord into the HBX port (G).
®

4

Flip the Power Switch (F) on the computer control panel to
the ON position. A copyright message lights on Autostar’s
LCD display, followed by a warning not to look at the Sun.
Press the Autostar key prompted by the message when you
are done reading.
A “Getting Started” message displays. Press ENTER to skip
this message.
See pages 9 to 11 for more information about Autostar’s
keys.

Enter
Key

L

K

Scroll Up
Key

ScrollDown
Key

Keep pressing the ENTER key until "Country/State" appearson the display. (Ignore the prompts requesting "Date" and"Time" for now – these functions will be explained later).

Make sure that the flip mirror control (K) is in the “Up” position,
as shown the diagram above.

When “Country/States” displays, press either one of the
SCROLL KEYS to cycle through the choices on the list. When
your state or country appears on the list, press ENTER.
“Cities” displays. Using the SCROLL KEYS, cycle through thelist of cities and press ENTER when the city closest to you
displays.
Finally “Telescope Models” displays. Using the SCROLL KEYS,
cycle through the list of telescope models and press ENTER
when your model displays.
The display now displays "Setup: Align." See page 19 for more
information.
If Autostar does not requests the Country/State, City andTelescope Model information, use the "Telescope Model"
and "Site" options in the Setup menu to change thisinformation. See pages 28, 29 and 31 for more information.

Arrow
Keys

Arrow
Keys

L

Sight along the side of the telescope’s main tube to locate an
object. If you wish to learn how to attach and align thetelescope’s viewfinder, see pages 13 to 14.
Use the telescope’s focus knob (L) to bring the object into
focus.

NumberKeys

You can now use the ARROW KEYS to slew (move) thetelescope up, down, right or left. Practice using the ARROW
KEYS to center objects in the eyepiece.
To change the speed at which the telescope moves (known
as the “slew” speed) press a NUMBER KEY from 1 through 9.
1 is the slowest speed and 9 is the fastest.

If you wish to observe using Autostar’s databases,
see:
Page 19 to learn how to perform an Easy Alignment
Page 20 to “Go To” Saturn”
Page 21 to learn about Guided Tours
Pages 22 to 39 to learn more about Autostar’s menus

5

TELESCOPE FEATURES
18

1

2

4

3

5

Features of the ETX-90AT, ETX-105AT,
and ETX-125AT are identical, with the
exception of the size of optical tube
and the type of viewfinder.

17

19

16

6

(on leftfork arm)

15

7

14

8

13
11

9
10
12

Fig. 1: The ETX-90AT Telescope.
1
2
3
4
5
6
7
8
9
10

6

Eyepiece
Viewfinder
Holder Thumbscrew
90° Eyepiece Holder
Optical Tube
Vertical Lock
Fork Arms
Focus Knob
Horizontal Lock
Computer Control Panel
A. ON/OFF Switch
B. Auxiliary Ports (2)C. Handbox PortD. 12v
E. LED

11
12
13
14
15
16
17
18
19

Base Housing
Battery Compartment(bottom of base)
Right Ascension (R.A.)/
Horizontal Setting Circle
Flip-Mirror Control Knobs
Photo Port
Declination (Dec.)/Vertical
Setting Circle
Viewfinder Alignment Screws
Viewfinder Alignment Bracket
Dust Cap

E

B

C

D

A

B

Fig. 2 (Inset): Computer Control Panel. (A) On/Off switch; (B)Auxiliary ports; (C) Handbox port; (D) 12v connector; (E)Power indicator light.

MEADE ETX: YOUR PERSONALWINDOW TO THE UNIVERSE
Caution:Using products other thanstandard Meade accessories
may cause damage to thetelescope’s internal
electronics and may void the
Meade warranty.

B Want to learn more

The Meade ETX-90AT, ETX-105AT and the ETX-125AT are extremely versatile, highresolution telescopes. With pushbutton controls, automatic tracking of celestial
objects and diffraction-limited imaging, an ETX telescope may be all the telescope
ever required by many terrestrial and astronomical observers.
Your ETX telescope reveals nature in an ever-expanding level of detail. Observe thefeather structure of an eagle from 50 yards or study the rings of the planet Saturn froma distance of 800 million miles. Focus beyond the Solar System and observe
majestic nebulae, ancient star clusters, remote galaxies and even stars recently
discovered to have planets orbiting about them. Meade ETX telescopes are
instruments fully capable of growing with your interest and are ideal for both thecasual observer and serious astronomer alike.

about the eyepieces
available for your ETX
telescope?

Telescope Controls
Become acquainted with all of these controls before attempting observations throughthe telescope.

See OPTIONALACCESSORIES, pages

B

Eyepiece: Place the supplied 26mm eyepiece into the 90° Eyepiece Holder (4,Fig. 1) and tighten in place with thumbscrew (3, Fig.1).

C

Viewfinder
ETX-90AT: 8 x 21mm Viewfinder: Slide the eyepiece end of the viewfinder
through the front of the viewfinder bracket (Fig. 18).
ETX-105AT, ETX-125AT: 8 x 25mm Right-Angle Viewfinder: Slide the front cellend of the viewfinder through the rear of the viewfinder bracket (Fig. 19).

D

Eyepiece Holder Thumbscrew: Tightens the eyepiece in place. Tighten to a firm
feel only.

eF

90° Eyepiece Holder: Holds the eyepiece upright for easy viewing.

43 to 44.

c Want to learn how to
attach the viewfinder toyour ETX telescope?
See VIEWFINDER,
pages 13 and 14.

G Want to learn more
about the Right
Ascension and
Declination setting
circles? See page 54.

Optical Tube: The main optical component that gathers the light from distantobjects and brings this light to a focus for examination with the eyepiece.

G

Vertical Lock: Controls the manual vertical movement of the telescope. Turning
the vertical lock counterclockwise unlocks the telescope enabling it to be freely
rotated by hand about the vertical axis. Turning the vertical lock clockwise (to afirm feel only) prevents the telescope from being moved manually, but engages
the vertical motor drive clutch for Autostar operation. When polar aligned, thevertical lock serves as the Declination or Dec. lock.
Note: The vertical lock knob is a knurled knob located on the fork arm to
the right of the focus knob (8, Fig. 1). Mounted beneath the knob is a circular scale without numbers. Do not confuse this scale with the Dec.
setting circle (16, Fig. 1) on the opposite fork arm which has a numberedscale used to locate astronomical objects.

H

Fork Arms: Hold the optical tube in place.
Note: The telescope base and fork mount are designed with internal“rotational limit stops.” The horizontal limit stop prevents the telescopefrom rotating more than 630° to avoid damage to the internal wiring. The
vertical limit stop prevents the viewfinder from striking the fork mountwhen the telescope is pointed upward just past 90° and prevents the
optical tube from striking the base if pointed downward more than 30°. Do
not force the telescope to move beyond these stops or damage to thetelescope will result.

i

Focus Knob: Moves the telescope’s primary mirror in a finely-controlled motion
to achieve precise image focus. The ETX telescopes can be focused on objects
from a distance of about 11.5 ft (ETX-90AT) or 15 ft (ETX-105AT or
ETX-125AT) to infinity. Rotate the focus knob clockwise to focus on distantobjects and counterclockwise to focus on nearby objects.

Caution:When loosening the Dec.
lock, be sure to support
the optical tube (5 Fig. 1).
The weight of the tube
could cause the tube toswing through the forkarms suddenly.

7

Definitions
Throughout this manual,
you will notice the terms"Alt/Az," "Right
Ascension," and"Declination." Alt/Az or
more properly, altazimuth,
is frequently used to refer toaltitude or Declination (theup-and-down verticalmovement of the telescope)and azimuth or Right
Ascension (the side-to-sidehorizontal movement of thetelescope). Right Ascension
is abbreviated as "R.A."
and Declination as "Dec."j

Horizontal Lock: Controls the manual horizontal rotation of the telescope. Loosen
the horizontal lock counterclockwise to unlock the telescope, enabling it to be freely
rotated by hand about the horizontal axis. Tightening the horizontal lock clockwise
prevents the telescope from being rotated manually, but engages the horizontal
motor drive clutch for Autostar operation. When polar aligned, the horizontal lockserves as the Right Ascension or R.A. lock.

1)

Computer Control Panel (see Fig. 2)
A. ON/OFF Switch: Turns the Computer Control Panel and Autostar
handbox ON or OFF.
Note: Always remove the batteries if they are not to be used for a long
period of time.
B. Auxiliary (AUX) Ports (2): Provide connection for current and future
Meade accessories. See OPTIONAL ACCESSORIES, page 43.
C. Handbox (HBX) Port: Plug the Autostar handbox into this port.
D. 12v: The 12v connector is designed to accept an external power
supply such as the optional #541 AC Adapter or the #607 Power Cord(see OPTIONAL ACCESSORIES, page 43). When one of the external
power supply options is used, the internal batteries are disconnectedfrom the power circuit.
E. LED: The red power indicator light illuminates when power is supplied
to the connected handbox and to the telescope’s motor drive.

1!

Base Housing: Supports the telescope for placement on a flat, level surface,such as a tabletop or tripod.

1@

Battery Compartment (not shown, underneath base): Install eightuser-supplied AA batteries in this compartment. See page 12 for more
information.

1#
1$

Right Ascension (R.A.) Setting Circle: See page 54 for detailed information.

Fig. 3a: Flip mirror control inthe “up” position.

Fig. 3b: Flip mirror control inthe “down” position.

1* Want to learn more about
attaching and aligning
the viewfinder?
See pages 13 and 14.

1( Note: The dust cap
should be replaced
after each observing
session and thepower turned off to
the telescope. Verify
that any dew thatmight have collectedduring the observing
session has
evaporated prior to
replacing the dust
cap. Do not
overtighten.

8Flip-Mirror and Flip-Mirror Control Knobs: ETX telescopes include an internal
mirror. With the flip-mirror control in the “up” position, as shown in Fig. 3a, light isdiverted to the eyepiece. With the flip-mirror control in the “down” position, as
shown in Fig. 3b, light proceeds straight out the photo port for photography. See
PHOTOGRAPHY, page 40.
Note: The flip-mirror control is in the “up” position when the control isvertical (perpendicular to the telescope tube). To place the flip-mirror in the“down” position, turn the control until it is horizontal.

1%

Photo Port: Attach any 35mm camera with a removable lens to this port using an
optional #64ST T-Adapter or attach the #932 Erecting Prism for correctly
oriented images through the eyepiece. See OPTIONAL ACCESSORIES, page 43.

1^

Declination (Dec.) Setting Circle (on left fork arm): See page 54 for detailed
information.

1&

Viewfinder Alignment Screws: Adjust these screws to align the viewfinder. See
pages 13 and 14 for more information.

1*

Viewfinder Alignment Bracket: Attach the viewfinder to this bracket. See pages
13 and 14 for more information.

1(

Dust Cap: Unthread the dust cap counterclockwise from the front lens of thetelescope.

AUTOSTAR FEATURES
1
2

L
4

3
5

1 LCD Display
2 ENTER Key

67

3 MODE Key
4 GO TO Key

K
8

9

J

5 Arrow Keys
6 Number Keys
7 Scroll Keys
8 Speed/? Key
9 Coil Cord
10 RS232 Port
11 Light key
12 Utility Light

Fig. 4: The Autostar Handbox.
Want to learn more about
downloading the latest
updates of Autostar
software from the
Meade website? Seepages 29 and 43.

Tour the Cosmos with Just the Push of a Button
Control of ETX Telescopes is through the operation of the standard-equipment #497
Autostar. Nearly all functions of the telescope are accomplished with just a few
pushes of Autostar’s buttons. Some of the major features of Autostar are:•Automatically move the telescope to any of the 30,000 objects stored in the
database or manually enter the astronomical coordinates of any celestial object.

•

Take a guided tour of the best celestial objects to view on any given night of the
year.

•

Download the latest satellite data, guided tours and software revisions directlyfrom the Meade website (www.meade.com) and share software with other
Autostar enthusiasts. (Requires optional #505 AstroFinder™ Cable Connector
Kit. See OPTIONAL ACCESSORIES, page 43.)•

Access a glossary of astronomical terms.

•

Calculate which eyepiece to use for optimum viewing of a celestial object.

Autostar provides control of virtually every telescope function. The Autostar handbox
has soft-touch keys designed to have a positive feel. The LCD (Liquid Crystal Display)is backlit with red LEDs (Light Emitting Diodes) for easy viewing in the dark. The backlit display, key arrangement and sequential menu structure make Autostar extremelyuser friendly.

9B 2-Line LCD Display: This screen displays Autostar's menus and informationcabout the telescope.
• Top line: Lists the primary menu.
• Bottom line: Displays other menus that may be chosen, menu
options, telescope status or information about a function that is being
performed.
ENTER Key: Press to go to the next menu level or to choose an option in amenu. The ENTER key is similar to the RETURN or ENTER key on a computer.
See MOVING THROUGH AUTOSTAR’S MENUS, page 17 and AUTOSTAR MENUS,
page 24.

d MODE Key: Press to return to the previous menu or data level. The top menu

e Want to learn more
about using the GO TO
function? See page 20.
Want to learn how to
perform a spiralsearch? See page 20.

elevel is “Select Item." The MODE key is similar to the ESCAPE key on a computer.
Note: Pressing MODE repeatedly while in the “Select Item” level moves
Autostar to the topmost screen: “Select Item: Object.”
Note: If MODE is pressed and held for two seconds or more, information
about the telescope's status displays. When the status displays, press
one of the Scroll keys (7, Fig. 2) to display the following information:• Right Ascension and Declination (astronomical) coordinates• Altitude (vertical) and Azimuth (horizontal) coordinates• Local Time and Local Sidereal Time (LST)• Timer and Alarm Status• Date• Site coordinates• Battery status
Press MODE again to return to the previous menu.
GO TO Key: After the telescope is aligned, press to slew (move) the telescope tothe coordinates of the currently selected object. While the telescope isslewing, the operation may be aborted at any time by pressing any key except
GO TO. Pressing GO TO again resumes the slew to the object. Also, press
during the alignment or GO TO procedures to activate a "spiral search."f Arrow Keys: The Arrow keys have several functions. Press an Arrow key to slew
the telescope in a specific direction (up, down, left and right), at any one of nine different speeds. See SLEW SPEEDS, page 17. Use the Up and Down Arrow keys tomove the telescope vertically up and down. The Left Arrow key rotates thetelescope horizontally counterclockwise, while the Right Arrow key rotates it clockwise.
Also, use the Arrow keys to scroll through numbers 0 through 9 and the alphabet. The Down Arrow key begins with the letter "A;" the Up Arrow key begins withdigit "9."Additionally, use the Arrow keys to to move the cursor across the display: Use theRight or Left Arrow key to move the cursor from one number to the next in thedisplay.

g Want to learn more
about changing slew
speeds? See page 17.

g Number Keys: Press to input digits 0 to 9. To change the speed at which thetelescope moves (known as the “slew” speed) press a NUMBER KEY from 1
through 9. 1 is the slowest speed and 9 is the fastest.

h Scroll Keys: Press to access options within a selected menu. The menu isdisplayed on the first line of the screen. Options in the menu are displayed, one
at a time, on the second line. Press the Scroll keys to move through the options.
Press and hold a Scroll key to move quickly through the options.
The Scroll keys also control the speed of text scrolling on the Autostar display.
When text is scrolling, press and hold the Up Scroll key for a faster display speed
and the Down Scroll key for a slower display speed.

10

i ? Key: Press to access the "Help" file. "Help" provides on-screen information on
how to accomplish whatever task is currently active.
Press the ? key and then follow the prompts on the display to access details ofAutostar functions in the Help feature. The Help system is essentially an
on-screen instruction manual.
If you have a question about an Autostar operation, e.g., INITIALIZATION, ALIGNMENT, etc., press the ? key and follow the directions that scroll on thesecond line. When satisfied with the Help provided, press MODE to return to theoriginal screen and continue with the chosen procedure.

j RS232 Port: Plug in optional cable to download the latest satellite data andsoftware revisions directly from the Meade website (www.meade.com). You canalso share software with other Autostar enthusiasts or control your telescope
remotely from your PC. (Requires optional #505 AstroFinder™ Software andCable Connector Kit. See OPTIONAL ACCESSORIES, page 43.)

1) Coil Cord Port/Coil Cord: Plug one end of the supplied Autostar coil cord into
this port located at the bottom of the handbox and the other end into the HBX portof the Computer Control Panel.

1! Light/0 Key: Press to turn on Utility light (12, Fig. 4).
1@ Utility Light: Use this built-in red light to illuminate star charts and accessories
without disturbing your eye's adaptation to darkness. Press "0" to turn the light on
and off.

ETX TIPS
Join an Astronomy Club, Attend a Star Party
One of the best ways to increase your knowledge of astronomy is to join an astronomy
club. Check your local newspaper, school, library or telescope dealer/store to find out if
there’s a club in your area.
At club meetings, you will meet other astronomy enthusiasts with whom you will be able
to share your discoveries. Clubs are an excellent way to learn more about observing thesky, to find out where the best observing sites are and to compare notes about
telescopes, eyepieces, filters, tripods and so forth.
Often, club members are excellent astrophotographers. Not only will you be able to see
examples of their art, but you may even be able to pick up some “tricks of the trade” totry out with your ETX telescope. See page 40 for more information about photography
with the ETX.
Many groups also hold regularly scheduled Star Parties at which you can check out andobserve with many different telescopes and other pieces of astronomical equipment.
Magazines such as Sky & Telescope and Astronomy print schedules for many popularStar Parties around the United States and Canada.

11

GETTING STARTED
Parts Listing
Getting the telescope ready for first observations requires only a few minutes. When
first opening the packing box, note carefully the following parts:
•
•
•
•

Cover

•
Batteries

The ETX Astro Telescope with fork mount system.
#497 Autostar handbox with coil cord.
One or more eyepieces, packed in plastic storage containers.
Hex-wrench, packed with the instruction manual. See MAINTENANCE,
page 45.
#884 Deluxe Field Tripod; two attachment knobs; spreader tray with separate spring, washers (2) and tension knob; leg extension lock knobs.

How to Assemble Your Telescope and Tripod

Fig. 5: Battery installation.

2

Assembly of the ETX telescope requires eight AA-size (user-supplied) batteries.
1.

1

Remove the ETX telescope from its packaging and place it on a sturdy surface.
Place the ETX on its side and remove the battery compartment cover from theunderside of the drive base. Insert eight (user-supplied) AA-size batteries into thebattery compartment oriented as shown in the battery compartment. Replace thecover and return the telescope to an upright position.
Caution: Use care to install batteries as indicated by the diagrams in thebattery compartment. Follow battery manufacturer's precautions. Do notinstall batteries backwards or mix new and used batteries. Do not mix
battery types. If these precautions are not followed, batteries may
explode, catch fire or leak. Improperly installed batteries void your Meade
warranty. Always remove the batteries if they are not to be used for a long
period of time.

Fig. 6: Spread tripod legs.

2

Note: Autostar does not require batteries; the telescope’s batteries
supply power to Autostar.
2.

Fig. 7: Slide spreader on rod.

3

Fig. 8: Tension knob assembly.

4
Fig. 9: Adjust tripod height.

3.

Assemble the #884 Deluxe Field Tripod:
Step a: Spread the tripod (1, Fig. 6) legs apart to a fully open position.
Step b: Slide the spreader tray (2, Fig. 7) onto the central threaded rod.
Step c: Slide a washer, followed by the spring, another washer and thetension knob (3, Fig. 8) onto the threaded rod. Tighten the tension knob
to a firm feel.
Step d: Adjust the height of the tripod by loosening the leg lock knobs (4, Fig. 9)
and adjusting the height of the inner leg extensions. Then retighten the lockknobs.
Mount your telescope in the altazimuth (alt/az) mode. If you wish to mount yourtelescope in the equatorial mode, see EQUATORIAL ALIGNMENT, page 51.
Note: Throughout this manual, you will notice the term "Alt/Az," or more
properly, altazimuth. This term is frequently used to refer to altitude or the
up-and-down vertical movement of the telescope). Azimuth refers to theside-to-side horizontal movement of the telescope.
Step e: Loosen the latitude control latch (6, Fig. 10) and lift up the tilt-plate (5, Fig.
10) so that you can easily access the underside of the plate. Relock thelatitude control latch, so the assembly doesn't slip while you are attaching
the telescope.
Step f: Line up the mounting hole (7, Fig. 11) on the base of the telescopemarked "High Latitude Leg" with the attachment knob (8, Fig. 11) that isclosest to the latitude control bar (9, Fig. 11). Line up the othermounting hole with the attachment knob at the bottom of the tilt-plate.
Thread both attachment knobs into the base of the telescope. Tighten toa firm feel only. (See Fig. 12.)
Step g: Unlock the latitude control latch (10, Fig. 13) and lower the tilt-plate until
it is level (push the tilt-plate down until it stops; this is the level
position). Lock the latitude control latch.

12

L
M
6

5

N
O

Fig. 10: Loosen control latch .

7
8

Fig. 15: Insert eyepiece.

4.

5.

9
Fig. 11: High latitude leg
mounting hole andcorresponding attachment
knob.

6.

Fig. 16: Tighten verticallock.

Fig. 17: Tighten horizontal
lock.

Place the 26mm eyepiece (12, Fig. 15) into the eyepiece holder on thetelescope and tighten the attachment thumbscrew (13, Fig. 15) to a "firm feel" only.
Make sure that the flip-mirror control (14, Fig. 15) is in the “up” position, as shownin the above photo. See page 8, for more information. Remove the dust cover (15,Fig. 15) from the end of the telescope tube.
Make sure that the computer control panel power switch (A, Fig. 2) is in the OFF
position. Remove the Autostar handbox and the coiled cord from the packing
materials. Plug one end of the cord into the HBX port (C, Fig. 2)and the other endof the coiled cord into the coiled cord port at the bottom of Autostar handbox, as
shown above.
Tighten (to a "firm feel" only, do not overtighten) the vertical lock (Fig. 6) and the horizontal lock (Fig. 9).

Attaching the Viewfinder
ETX-90AT: 8 x 21mm Viewfinder: Slide the eyepiece end of the viewfinder
through the front of the viewfinder bracket (16, Fig. 18).
ETX-105AT or ETX-125AT: 8 x 25mm Right-Angle Viewfinder: Slide the front
cell end of the right-angle viewfinder through the rear of the viewfinder bracket(17, Fig. 19).

8

Unthread the six alignment screws slightly to fit the viewfinder through thebracket. With the viewfinder in place, tighten the six alignment screws to a firm feel
only against the viewfinder tube.

Using The Viewfinder

Fig. 12: Attach telescope totripod.

J

As with most astronomical telescopes, the ETX model telescopes present a fairly
narrow field of view to the observer. As a result it is sometimes difficult to locate andcenter objects in the telescope’s field of view. The viewfinder, by contrast, is a lowpower, wide-field sighting scope with crosshairs that let you easily center objects inthe eyepiece of the main telescope’s field of view. The telescope viewfinder is a great
help in locating faint astronomical objects before you begin observing through thetelescope eyepiece.
ETX-90AT 8 x 21mm Erect-Image Viewfinder:Standard equipment with the ETX-90AT, the 8 x 21mm Erect-Image Viewfinder has
8-power magnification and an aperture of 21mm. This viewfinder presents acorrectly oriented image both up-and-down and left-to-right.
ETX-105AT or ETX-125AT 8 x 25mm Right-Angle Viewfinder:Standard equipment with the ETX-105AT and ETX-125AT, the 8 x 25mm Right-Angle
Viewfinder has 8-power magnification and an aperture of 25mm. This viewfinderpresents a correctly oriented image up-and-down, but is reversed left-for-right.

Fig. 13: Level tilt-plate.

L

P

Fig. 14: Handbox HBX port.
Fig. 18: ETX-90 Viewfinder Installation.

Q
Fig. 19: ETX-105/-125 Viewfinder

13

Focusing the Viewfinder

1

2

The ETX model viewfinders are pre-focused at the factory. Individual eye variations
may require that the viewfinder be re-focused. To check the focus, point the
viewfinder at a distant terrestrial (land) object such as a telephone pole or light poleand look through the viewfinder. If the viewfinder image is not in sharp focus, follow
the procedure below that applies to your telescope model.

4

5

3

Fig. 20a: ETX-90 Viewfinder:(1) Front lens cell;(2) Knurled lock-ring;(3) Viewfinder eyepiece;(4) Alignment screws;(5) Viewfinder bracket;

76

ETX-90AT
1. Remove the viewfinder by slightly unthreading the six alignment screws (4, Fig.
20a) and slipping it out of the bracket.
2. Loosen the knurled lock-ring (2, Fig. 20a) located near the viewfinder’s front lens
cell (1, Fig. 20). Unthread this ring (counterclockwise, as seen from the eyepieceend of the viewfinder) by several turns.
3. Look through the viewfinder and focus on a distant object. Slowly rotate the front
lens cell in one direction or the other, until the object appears sharp. One or two
rotations of the lens may have a significant effect on image focus.
4. Lock the focus in place by threading the knurled lock-ring clockwise up against the
viewfinder’s lens cell.
5. Replace the viewfinder into the viewfinder bracket. Gently tighten the six alignment
screws. Proceed with Aligning the Viewfinder.
ETX-105AT or ETX-125AT
Turn the focus ring (6, Fig. 20b) at the base of the viewfinder eyepiece (7, Fig. 20b)in either direction until a sharp focus is reached.

Aligning the Viewfinder
Fig. 20b: ETX-105/-125
Viewfinder:(6) Focus ring;(7) Viewfinder eyepiece

In order for the viewfinder to be useful, it must first be aligned with the main telescope,so that both the viewfinder and the main telescope are pointing at precisely the same
location. To align the viewfinder:
1. Turn the three rear alignment screws of the viewfinder bracket (4, Fig. 20a) so thatthe viewfinder tube is roughly centered within the viewfinder bracket.
Tip: Do not overtighten the alignment screws. When tightening one screw it may
be necessary to loosen one or both of the two other alignment screws.
2. Point the main telescope at some tall, well-defined land object, such as the top ofa telephone pole. Center the object, as precisely as possible, in the SP 26mm
eyepiece's field of view. Tighten the vertical and horizontal locks (6 and 9, Fig. 1)
so that the tube cannot move and the object remains centered (1, Fig. 21).
3. While looking through the viewfinder, turn one or more of the three front
viewfinder alignment screws (4, Fig. 20a), until the crosshairs of the view-finder
point at precisely thesame position as theviewthroughthe(beforeeyepiece of the mainalignment)
telescope (2, Fig. 21).
Check that the viewfinder’scrosshairs and the main
telescope are now pointing
at precisely the same
object. The viewfinder is
now aligned to the main
telescope. Unless thealignment
screwsare
disturbed or the viewfinder
jarred,theviewfinder
should remain aligned
indefinitely.

1

View through the
viewfinder

View through thetelescope eyepiece(afteralignment)

2

Fig. 21: Aligning the Viewfinder.

14

Choosing an Eyepiece
The magnification or power, at which a telescope is operating is determined by two
factors: the focal length of the telescope and the focal length of the eyepiece.
Telescope Focal Length is the distance that light travels inside the telescope before
reaching a focus. In the mirror-lens design of the ETX models, the focal length iscompressed by the telescope’s secondary mirror, so that a long focal length is housedin the short ETX optical tube. For example, the ETX-90AT’s focal length is 1250mm
or about 49”. This means that if the ETX–90AT were a classical refracting-type oftelescope, the optical tube would be more than four feet long instead of theETX–90AT's compact 11” tube length.

Fig. 22: Meade Super
Plössl eyepieces.

Tip: If you plan on
viewing using higher
magnification eyepieces,
first locate, center andfocus the object using a
low-power eyepiece(e.g., 26mm eyepiece).
Then remove the lowpower eyepiece andreplace it with a higherpower eyepiece; theobject should still becentered in the field ofview. Objects are mucheasier to locate andcenter at lower powers;
higher powers are
employed simply bychanging eyepieces.

Eyepiece Focal Length is the distance light travels inside the eyepiece before
reaching focus. Focal length is usually printed on the side of the eyepiece, for example,
26mm. Low-power eyepieces are typically available in 26mm, 32mm and 40mm sizes(see OPTIONAL ACCESSORIES, page 43). The low-power eyepiece provided with yourETX is designed to provide a wide, comfortable field of view with high image resolution.
Calculating Magnification: On a telescope, such as the ETX, different eyepiece
focal lengths are used to achieve different magnifications, from low to high. A 26mm
eyepiece yields 48X (“48-power”) on the ETX-90AT, 57X on the ETX-105AT and 73X
on the ETX-125AT. A variety of powers may be obtained with the addition of optional
eyepieces as well as the #126 2X Barlow Lens which doubles the power of an eyepiece (see OPTIONAL ACCESSORIES, page 43). To calculate magnification, divide thefocal length of the telescope’s optical tube by the focal length of the eyepiece. For
example:Telescope Focal Length divided by Eyepiece Focal Length
1250mm divided by 26mm
With Barlow: 73 x 2= Power= 73X= 146XThe eyepiece power or magnification is therefore 73X and 146X with the Barlow.
Most observers should have 3 or 4 eyepieces plus the #126 2X Barlow to achieve thefull range of reasonable magnifications possible with ETX models.

ETX TIPS
Too Much Power?
Can you ever have too much power? If the type of power you’re referring to is
eyepiece magnification, yes, you can! The most common mistake of the
beginning observer is to “overpower” a telescope by using high magnifications
which the telescope and atmospheric conditions cannot reasonably support.
Keep in mind that a smaller, but bright and well-resolved image is far superior to
one that is larger, but dim and poorly resolved (see Figs. 23a and 23b). Powers
above 300X should be employed only under the steadiest atmosphericconditions.
Fig. 23a & 23b: Jupiter: Examplesof the right amount ofmagnification and too muchmagnification.

Autostar can calculate the best eyepiece for you to use. Try out the “EyepieceCalc” feature in the Utilities menu.
Most observers should have three or four additional eyepieces to achieve the fullrange of reasonable magnifications possible with the ETX telescopes. See
OPTIONAL ACCESSORIES, page 43.

15

OBSERVING
Observing by Moving the Telescope ManuallyNote:
Viewing conditions vary
widely from night-to-nightand site-to-site. Turbulencein the air, even on anapparently clear night, candistort images. Low-power
eyepieces, such as the
26mm supplied with yourtelescope, are better suited
to resolving images in poor
viewing conditions.

If you wish to observe a distant land object, such as a mountain top or a bird, you canobserve by merely pointing the telescope and looking through the eyepiece.
1. Loosen the telescope’s horizontal lock (9, Fig. 1) and vertical lock (6, Fig. 1).
2. Move your telescope to observe distant street signs, mountains, trees and otherstructures. Use your viewfinder to help sight-in on an object.
3. Center the object in the viewfinder’s crosshairs and then in the telescope
eyepiece. When the object is centered in your eyepiece, remember to re-tighten
the horizontal and vertical locks.
4. Practice focusing objects using the focus knob (8, Fig. 1).
5. Once you get a feel for how your telescope moves and focuses, try to view
something more challenging, like a bird or a distant moving train.
You can also observe stars and objects in the night sky using this method, but notethat objects begin to slowly drift across the eyepiece field. This motion is caused by
the rotation of the Earth. As you become familiar with the Autostar handbox operation,
you can counteract the drift using the automatic tracking feature (see TO TRACK ANOBJECT AUTOMATICALLY, page 17) or by using Autostar's GO TO capabilities (seeGO TO SATURN, page 20).

Terrestrial Observing

NEVER point
the telescope
directly at ornear the Sun at
any time! Observing theSun, even for the smallest
fraction of a second, will
result in instant andirreversible eye damage,as well as physicaldamage to the telescope
itself.
Do not look through thetelescope's eyepiece orviewfinder while it is rapidly moving. Children
should always have adultsupervision whileobserving.

Important Note:
Autostar requests theCountry/State, City andTelescope Model
information only the firsttime Autostar is activated.
Subsequently, Autostar
uses the location andmodel number you havechosen.
If you wish to change thisinformation, use the"Telescope Model" and"Site" options in the Setup
menu. See pages 28, 29
and 31 for more
information.

16

ETX telescopes are excellent high-resolution terrestrial (land) telescopes. Viewing
terrestrial objects requires looking along the Earth's surface through heat waves.
These heat waves often cause degradation of image quality. Lower power eyepieces,like the 26mm, magnify these heat waves less than higher power eyepieces (such asa 9mm eyepiece). Therefore, lower power eyepieces provide a steadier, higher quality image. If the image is fuzzy or ill-defined, reduce to a lower power eyepiece, where
the heat waves do not have such an effect on image quality. Observing in early morning hours, before the ground has built up internal heat, produces better viewing
conditions than during late afternoon hours.

Observing Using Autostar Arrow Keys
You may observe land and astronomical objects using Autostar's Arrow keys to movethe telescope.
1.
2.
3.

4.
5.

6.

7.
8.
9.

Tighten the horizontal and vertical locks (9 and 6, Fig. 1).
Make sure that Autostar’s coiled cord is connected to the computer control
panel’s HBX port (C, Fig. 2).
Flip the Power Switch (A, Fig. 2) on the computer control panel to the ON
position. A copyright message lights on Autostar’s LCD display, followed by awarning not to look at the Sun. Press the Autostar key prompted by the message
when you are done reading. See page 9 to 11 for more information about
Autostar’s keys.
A “Getting Started” message displays. Press ENTER to skip this message.
Keep pressing the ENTER key until "Country/State" displays. (Ignore theprompts requesting "Date" and "Time" for now—these functions will be explainedlater).
When “Country/States” displays, press either one of the SCROLL KEYS to cycle
through the choices on the list. When your state or country appears on the list, press
ENTER.
“Cities” displays. Using the SCROLL KEYS, cycle through the list of cities and press
ENTER when your city or the city closest to your observing site displays.
Finally “Telescope Models” displays. Using the SCROLL KEYS, cycle through thelist of telescope models and press ENTER when your model displays.
The display now displays "Setup: Align." .

You can now use the ARROW KEYS to slew (move) the telescope up, down, right orleft. Practice using the ARROW KEYS to center objects in the eyepiece.
To change the speed at which the telescope moves (known as the “slew” speed),press a NUMBER KEY from 1 through 9. 1 is the slowest speed and 9 is the fastest.
See SLEW SPEEDS on the following page.

Slew Speeds
Autostar has nine slew speeds that move the optical tube at rates that are directly
proportional to the sidereal rate and have been calculated to accomplish specificfunctions. Press the Number key to change the slew speed.
The nine available speeds are:Number Key 1 =1x =1 x sidereal (0.25 arc-min/sec or 0.004°/sec)
Number Key 2 =2x =2 x sidereal (0.5 arc-min/sec or 0.008°/sec)
Number Key 3 =8x =8 x sidereal (2 arc-min/sec or 0.033°/sec)
Number Key 4 =16x =16 x sidereal (4 arc-min/sec or 0.067°/sec)
Number Key 5 =64x =64 x sidereal (16 arc-min/sec or 0.27°/sec)
Number Key 6 = 128x =30 arc-min/sec or 0.5°/sec
Number Key 7 = 1.0° =60 arc-min/sec or 1.0°/sec
Number Key 8 = 1.5° =90 arc-min/sec or 1.5°/sec
Number Key 9 = Max =approx. 4.5°/sec
Speeds 1, 2 or 3: Best used for fine centering of an object in the field of view of ahigher power eyepiece, such as a 9mm eyepiece.
Speeds 4, 5 or 6: Enable centering of an object in the field of a low-to-moderate
power eyepiece, such as a 26mm.
Speeds 7 or 8: Best used for rough centering of an object in the viewfinder.
Speed 9: Moves the telescope quickly from one point in the sky to another.

Astronomical Observing
Used as an astronomical instrument, your telescope has many optical and electromechanical capabilities. It is in astronomical applications where the high level of
optical performance is readily visible. The range of observable astronomical objects
is limited only by the observer’s motivation.

Observe the Moon
Point your telescope at the Moon (note that the Moon is not visible every night) andpractice using the Arrow keys and the slew speeds to view different features. The
Moon contains many interesting features, including craters, mountain ranges and fault
lines. The best time to view the Moon is during its crescent or half phase. Sunlight
strikes the Moon at an angle during these periods and adds a depth to the view. No
shadows are seen during a full Moon, making the overly bright surface appear flat andrather uninteresting. Try using a neutral density Moon filter when observing the Moon(see OPTIONAL ACCESSORIES, page 43). Not only does it cut down the Moon's brightglare, but it also enhances contrast, providing a more dramatic image.

To Track an Object AutomaticallyAs the Earth rotates beneath the night sky, the stars appear to move from East toWest. The speed at which the stars move is called the sidereal rate. You can setup
your telescope to move at the sidereal rate so that it automatically tracks (follows) thestars and other objects in the night sky. If the telescope is not tracking anastronomical object, the object will drift out of the eyepiece field of view. The tracking
function automatically keeps an object centered in the telescope’s eyepiece.
To automatically track objects, you need to learn how the Autostar keypad operates
in order to move through its menus. You'll need to initialize and align your telescope.

Moving Through Autostar’s Menus
The Autostar database is organized in levels for quick and easy navigation.
••••

Press ENTER to go deeper into Autostar's menu levels.
Press MODE to move back toward the top menu level.
Press the Scroll keys to move up and down through the options
available for each level.
Press the Arrow keys to enter characters and digits. The Arrow keys
are also used to move the telescope.

17

Initializing Autostar
Definition:
Initialization is aprocedure that makes surethat Autostar operates
correctly. When you firstuse Autostar, it doesn't yet
know where the observation location site is or thetime or date of theobservation session.
During the alignment
procedure, you will enter
time, date and observing
location
Autostar Uses thisinformation to precisely
calculate the location ofcelestial objects (such asstars and planets) and tomove your telescopecorrectly for various
operations.

Tip:
When multiple choices areavailable within an Autostar
Menu option, the current
option is usually displayed
first and highlighted by aright pointing arrow (>).

Important Note:
Autostar requests theCountry/State, City andTelescope Model
information only the firsttime Autostar is activated.
Subsequently, Autostar
uses the location andmodel number you havechosen.
If you wish to change thisinformation, use the"Telescope Model" and"Site" options in the Setup
menu. See pages 28, 29
and 31 for more information.

This section describes how to initialize Autostar. Perform this procedure the first time
you use Autostar or after performing a Reset (see RESET, page 30). Autostar will ask
you to enter the current time and date and to choose your observing location and yourtelescope’s model number from the list it displays.
1.

Tighten the vertical and horizontal locks (6 and 9, Fig. 1) if necessary.

2.

Make sure that Autostar is connected to the HBX port (C, Fig. 2) of thetelescope’s computer control panel.

3.

Flip the telescope power switch (A, Fig. 2) to the ON position.
The Autostar screen displays a copyright message, followed by a short beep.
Then Autostar takes a few moments to start up the system.

4.

A message displays that warns not to look at the Sun. At the end of this message,press the key prompted by Autostar to signify that the message has been readand understood.

5.

The Getting Started menu displays a scrolling message. Press ENTER (2, Fig.
4) to bypass the Help tutorial and continue with initialization.

6.

Autostar then requests the current date. Use the Number keys (6, Fig. 4) to enter
the digits for the date. Use the Arrow keys (5, Fig. 4) to move back and forth from
one number to the next in the day display. Next, use the Right Arrow key to moveto the month position. Use the Scroll keys (7, Fig. 4) to cycle through the list ofmonths.
When the current month is displayed, use the Right Arrow to move to the year
position. Use the Number keys to enter all four digits of the current year. Press
ENTER when the entire date has been entered.

7.

Autostar then requests the current time. Use the Number keys to enter the time.
(Use a "0" for the first digit if it is less than 10.) Use the Arrow keys to move from
one number to the next. Press one of the Arrow keys to scroll to "AM" or "PM." If
you select the "blank" choice that follows "AM" and "PM," the clock displays timein a 24-hour (military time) format. Press ENTER to start the clock.

8.

Autostar then requests the status of Daylight Savings Time. Press a Scroll key totoggle between the YES/NO settings. Select the desired setting by pressing
ENTER when the correct setting displays.
Note: Daylight Savings Time may be referred to by a different name invarious areas of the world.
9.

Autostar then requests the country or state (listed alphabetically) of theobserving site. Use the Scroll keys to cycle through the database of countries,
states and provinces. Press ENTER when the correct location displays.

10. Autostar then requests the city (listed alphabetically) closest to the observingsite. Use the Scroll keys to cycle through the database of cities. Press ENTER
when the closest city displays.
11. Autostar then requests the telescope model number. Use the Scroll keys to cycle
through the database of models. Press ENTER when your model number displays.
12. System initialization is complete and the screen reads "Setup: Align."

Easy (Two-Star) Align
The fastest and easiest way to locate celestial objects is to use the alt/az Easy Align.
Autostar is in the alt/az mode when you first power it on, so you do not need to selectthis mode, unless you have changed this setting in the Telescope/Mount menu. If you
wish to align your telescope in the equatorial (polar) mode, see EQUATORIAL
ALIGNMENT, page 51.
Autostar automatically picks two stars from its database for the Easy Align procedure.
During this procedure, Autostar moves the telescope to a first alignment star and theuser is asked to center the star in the eyepiece. The process is then repeated with asecond star to complete the alignment.

18

Important Note: Before aligning the telescope, you MUST first initialize
Autostar, as described in INITIALIZING AUTOSTAR, page 18. See MOVINGTHROUGH AUTOSTAR’S MENUS, page 17, for a description of how
Autostar’s keys operate.
How to perform the Easy Align Procedure
If you have just performed the initialization procedure, go to step 6.
1.

Sun Warning: Press the key prompted by Autostar to accept.

2.

Getting Started: Press ENTER to continue.

3.

Enter Date: Enter the current date, then press ENTER.

4.

Enter Time: Enter the current time. Select "AM," "PM," or 24-hour clock (blank).
Then press ENTER.

5.

Daylight Savings: Select “Yes” or “No,” then press ENTER.

6.

Alignment Option Screen: “Setup: Align” displays. Press ENTER.

7.

Select Alignment: “Align: Easy” displays. Press ENTER.

8.

Set Home Position: Autostar then prompts you to set the telescope in the Alt/Az
Alignment home position (if necessary). To set your telescope in the "Alt/Az"
home position:

Loosen the telescope’s vertical lock (6, Fig. 1).
Level the tripod head. See Step #3g, page 12. Level the optical tube bylining up 0° on the Dec setting circle (16, Fig. 1) with the Dec pointer(the small molded triangle under the setting circle).
•
Retighten the vertical lock (6, Fig. 1) to a firm feel only.
•
Unlock the horizontal lock (9, Fig. 1).
•
Grasp the telescope by a fork arm and rotate the telescope counterclockwise
until it stops.
•
Turn the telescope clockwise until a fork arm is directly over the computer
control panel.
•
Re-lock the R.A. lock (9, Fig. 1).
•
Lift and rotate the telescope and tripod until they point North. Press ENTER.
See LOCATING THE CELESTIAL POLE, page 53 for more information.
9 . Star Alignment: Autostar chooses two stars to align upon. When the telescope
slews to the first star for alignment, it may not appear in the field of view in theeyepiece. Try to locate the star using the viewfinder (2, Fig. 1). The alignment starshould be easily recognized and be the brightest star in the area of the sky where
the telescope is pointing. Look through the viewfinder and use the Arrow keys tomove the telescope until the star is visible. Then center the star in the eyepiece.
Press ENTER. Repeat the procedure for the second alignment star.
•
•

Tip:
The GO TO key also
allows you to perform a"spiral search." A spiralsearch is useful when thetelescope slews to an
object, but that object is
not visible in the eyepieceafter the telescopefinishes its search. (Thissometimes occurs during
an alignment procedure.)
Press GO TO when thetelescope stops slewing.
The telescope begins tomove in a spiral pattern ata very slow speed aroundthe search area. Lookthrough theeyepiece and when theobject does become
visible, press MODE tostop the spiral search.
Then use the Arrow keys
to center the object.

Important Note:

The first time you use
your telescope or if you
are experiencing any
problems with pointing
accuracy, follow theprocedure described in
APPENDIX C: TRAINING
THE DRIVE, page 56, toinsure accurate pointing
and tracking.

ETX TIPS
Which One’s the Alignment Star?
If you’re not familiar with objects in the night sky, how can you be sure if the starin your eyepiece is really the alignment star?
The rule of thumb is that an alignment star is usually the brightest star in thatarea of the sky. If you perform a GO TO to an alignment star and you're not sure
if you have located the alignment star or it isn't in the eyepiece, look through yourviewfinder. When you view an alignment star in the viewfinder, it stands out
dramatically from the rest of the stars in that portion of the sky. The viewfinder
will help you locate a star more quickly than the eyepiece, because it has a muchwider field of view than the eyepiece. Using Autostar, set the slew speed to 6
(push Number key 6) or higher and use the Arrow keys to center the alignment
star in the viewfinder. If your viewfinder has been aligned with the telescope, thealignment star should now be in the eyepiece. Set the slew speed to 4 or lessand center the star in the eyepiece. Also see the SPIRAL SEARCH tip, page 20.

19

Important Note:
While performing theautomatic tracking
procedure, only use theArrow keys to move thetelescope. Once thetelescope has beenaligned, do not loosen
the telescope’s vertical or
horizontal locks (6 and 9,
Fig. 1) or move the basemanually or alignment
will be lost.

When the procedure is performed correctly, "Alignment Successful" displays. If
Autostar does not display this message, perform this procedure again.
NOTE: Autostar locates alignment stars based on the date, time and location entered. The alignment stars may change from night to night. All thatis required is for the observer to center the selected stars in the eyepiece
when prompted.

Observe a Star using the Automatic Tracking Feature
In this example, the Autostar Arrow keys are used to find a star and then Autostar's
tracking feature automatically keeps the star centered in yourtelescope's eyepiece. Make sure you have initialized and aligned your telescope
before you try out this feature (see pages 18 and 19).
1.

Once you’re telescope has been aligned, “Align Successful” and then “Select Item:
Object” display. Push the Scroll Up key once and “Select Item: Setup” displays

2.

Press ENTER. “Setup: Align” displays.

3.

Press the Scroll Down key repeatedly until "Setup: Targets" displays. Press
ENTER.

4.

"Targets: Terrestrial" displays. Press one of the Scroll keys once. "Targets:
Astronomical" now displays.

5.

Use the Arrow keys (5, Fig. 2) to locate a bright star in the night sky. Use theviewfinder (2, Fig. 1) to help line up on the star. You may choose any unobstructed, bright star for the purposes of this example. Use Autostar's Arrow keys
to center the star in the eyepiece. Once the star is centered, press ENTER toselect "Astronomical." The telescope's tracking motors then engage. It may takethe tracking motors several seconds to begin tracking. When they do, it may benecessary to once again center the star in the eyepiece. The tracking motors willthen keep the star you have chosen in the center of the eyepiece.

6.

Press and hold the ENTER key for a few seconds and then release to stop tracking. You may repeat the procedure to locate another star or object using theArrow keys. Then press ENTER to re-engage the tracking motors.

Go To Saturn
After performing the Easy Align procedure, the motor drive begins operating and thetelescope is aligned for a night of viewing. Objects in the eyepiece will maintain theirposition even though the Earth is rotating beneath the stars.
This exercise demonstrates how to select a celestial object, the planet Saturn, forviewing from Autostar’s database.
NOTE: Saturn is not visible the entire year and you may need to choose
another object from Autostar's database; however, the procedure, as
described below, remains the same. If Saturn (or any other object) is not
currently visible in the sky, Autostar displays “Below Horizon.”

20

1.

After the telescope is aligned, “Select Item: Object” displays. If “Select Item:
Object” is not displayed on your handbox, keep pressing MODE until it does display. Press ENTER.

2.

“Object: Solar System” displays. Press ENTER.

3.

“Solar System: Mercury” displays. Keep pressing the Scroll Down key until “Solar
System: Saturn” displays (or you may choose another object from the Solar
System list if Saturn is not visible).

4.

Press ENTER. “Calculating” displays. Then “Saturn” and a set of coordinates
displays. Note that Saturn’s (and other planets’) coordinates change throughout
the year.

5.

Press GO TO. “Saturn: Slewing...” displays and the telescope slews until it finds
Saturn. You may need to use the Arrow keys to center Saturn precisely in theeyepiece. Autostar then automatically moves the telescope so that it "tracks"
Saturn (or whatever other object you may have chosen); i.e., Saturn remains
centered in the eyepiece.

Using the Guided TourThis example demonstrates using “Tonight’s Best” Guided Tour.
Tip: Try out the Guided
Tour feature; the “Tonight’s
Best” Guided Tour will point
your telescope at the best
objects visible in the sky forevery given night of theyear. The objects in thistour may change from night
to night and month tomonth.

1.

After observing Saturn, press MODE twice so that “Select Item: Object” displays
again.

2.

Press the Scroll Down key twice. “Select Item: Guided Tour” displays.

3.

Press ENTER. “Guided Tour: Tonight’s Best” displays. Press ENTER.
NOTE: If you wish to try out other Guided Tours, press the Scroll Down
key to scroll through other tour choices. When the tour you wish to selectdisplays, press ENTER.

4.

Other preprogrammed
Guided Tours are alsoavailable.
You can easily create yourown Guided Tour using theoptional Meade’s Autostar
Suite software. See
PHOTOGRAPHY WITH
MEADE’S AUTOSTARSUITE, page 42 for more

“Tonight’s Best: Searching...” displays. After calculating, “Tonight’s Best: Jupiter”
displays.
NOTE: Different objects may be displayed on a tour list on any given night.
Tour objects are selected based on location’s time and date.
Press ENTER to display information about the object. Press GO TO to move thetelescope to the object.

5.

Press MODE to return to the Tour list. Press the Scroll keys to scroll through thelist. Press ENTER when you find the next object you wish to observe.

6.

Press and hold down MODE for two seconds to leave the Guided Tour menu.

information.

ETX TIPSStar Charts
Even with the Autostar's large 30,000 object library, star charts andplanispheres are still useful for a variety of reasons. In particular, they are agreat aid in planning a night of celestial viewing.
A wide variety of star charts are available in books, in magazines, on the internet and on CD Roms. Meade offers Autostar Suite™ and other star locator
software. Contact your Meade dealer or Meade's Customer Service
department for more information.
Astronomy and Sky and Telescope magazines print star charts each monthfor up-to-the-minute maps of the heavens.

21

AUTOSTAR OPERATIONSETUP MENU
Automatic alignment
permits all telescope
operations with only
minimal setup.

Select Item:
ObjectSelect Item:
Setup
UTILITIES MENU
Calculate eyepiecemagnifications;
set timer alerts;
create your own
landmark survey.

The Universe of

AutostarA
utostaruto
star

Select Item:
Utilities
GLOSSARY
What is an elliptical galaxy?
How far away is the Sun?
Expand your knowledge ofastronomy by displaying terms
and definitions, and other information.

OBJECT MENU
Want to see Mars? The Orion nebula?
The Andromeda galaxy? Select fromover 30,000 objects and press
GO TO to move the telescope
automatically to an object.
Select Item:
Event
EVENT MENU
Display the time ofpast, present and future
astronomical events,
such as Moon phases
or meteor showers.
Select Item:
Guided Tour

Select Item:
Glossary

GUIDED TOUR
Autostar escorts you
on a tour of tonight's
best celestial objects
at your viewing location.

Fig. 24: The Autostar Universe: The six primary categories listed in the Select menu.

ObjectEvent
Guided Tours
Glossary
Utilities
Setup

Fig. 25: Menus set in a loop.

Setup
Align
Date
Time
Daylight Saving
Telescope
Targetsetc.

Fig. 26: Menu options display on thesecond line. Use the Scroll keys tomove up or down through the list of
options. Press ENTER to select thedesired option.

It is important to understand that menu selections are set in a loop (Fig. 25). This meansthat pressing the Scroll Down key cycles down through all the available options withina given category, then returns to the first option. The Scroll Up key cycles up throughthe options in the opposite order. Note that this capability is a quick way to get to an
option that is near the bottom of the list. The following example demonstrates thiscapability.
Example:To navigate to the “Select Item: Setup” menu option when the “Select Item: Object” menu isdisplayed:
1.

Press the Scroll Down key four times or the Scroll Up key once.

The screen in Fig. 26 shows two lines of information in the Autostar display. The top
line shows the current menu level. The second line displays an option which may be
selected. Some options are submenus that offer more choices. The Scroll keys moveup and down within the list of available options, showing one option at a time.
When an option is displayed on the second line, press the ENTER key to choose that
option.
Press the MODE key to return back to the last menu. This can be useful to exit a menu
or if the wrong menu option is chosen.
IMPORTANT NOTE: No matter how many levels into Autostar are traveled, each press of the MODE key moves up a level, until the top level,"Select Item," is reached. Once Select Item displays, press MODE toreturn to the topmost level, "Select Item: Object."

Autostar Navigation Exercise
To demonstrate how the Autostar menu structure works, the following exercise
calculates Sunset time so an evening observing session can be planned.
NOTE: To perform an accurate calculation, Autostar MUST be properly
initialized with the current date, time and location of the observing site. To
enter the current date, time and location information, see INITIALIZINGAUTOSTAR, page 18, before proceeding with this exercise.
To Calculate Sunset time:
1. Press the MODE key several times, until “Select Item: Object” is displayed.
2.

22

Press the Scroll Down key once to display the “Event” option in the “Select Item”
menu.

3.

Press the ENTER key to choose the "Event" option and move down a level.
"Event: Sunrise" is displayed.

4.

Press the Scroll Down key once to display the "Sunset" option in the Event menu.

5.

Press the ENTER key to choose the "Sunset" option and move down anotherlevel.

6.

Autostar calculates the Sunset time based on the current date, time and location.
Autostar then displays the results of the calculation.

7.

Press MODE once to start moving back up through the Autostar levels. The firstlevel up is the Event menu.

8.

Press MODE again to move up another level. This is the top level, "Select Item."

9.

Press MODE again to return to the starting point of "Select Item: Object."Entering data into Autostar■

To enter numbers and text:a) Use the Number keys, orb) Use the Arrow keys to scroll through numbers 0 - 9 and the alphabet. The
Down Arrow key begins with the letter "A;" the Up Arrow key begins with digit "9."Tip:

When multiple choices
are available within amenu option, the current
option is usuallydisplayed first andhighlighted by a rightpointing arrow (>).

■

To move the cursor across the display:
Use the Right or Left Arrow key (5, Fig. 4) to move the cursor from one number
to the next in the display.

■Press ENTER when the desired information has been entered.

Navigating Autostar
Autostar's menus are organized for quick and easy navigation:■

Press ENTER to go deeper into Autostar's menu levels.

■

Press MODE (3, Fig. 4) to move back toward the top menu level.

■

Press the Scroll keys to move up and down through the options or lists.

■

Press the Arrow keys to move the cursor across the display.

■Press the Help (?) key to access on-line help.

ETX TIPS
Look into the Future
The Date option in the Setup menu is much more than just an entry of today's
date; with it you can look far into the future or learn about past events. Autostar
can calculate the date and times of future events and, except for eclipses, past
events as well (based on the current calendar system). E.g., a Sunrise on
March 6, 2043 A.D. or the Vernal Equinox in 1776 A.D. To use this feature,enter the desired date in the Setup menu or select an option in the Event menu.
Autostar, using the Event menu, can calculate dates and times for Sunrises,
Sunsets, Moonrises, Moonsets, Moonphases, Solar and Lunar Eclipses (forthe next 100 years), meteor showers, equinoxes and solstices and the minimums of Algol.
One very practical use of the Event menu is to check the Sunset option todetermine when you can begin your astronomical observing session.

23

24
SunriseSunsetMoonriseMoonsetMoon Phases
Next Full Moon
Next New Moon
Next 1st Qtr
Next 3rd Qtr
Meteor Showers
Quadrantids
LyridsEta Aquarids
Delta Aquarids
Perseids
Orionids
Taurids
Leonids
Geminids
UrsidsSolar Eclipses
Lunar Eclipses
Min. of Algol
Autumn Equinox
Vernal Equinox
Winter SolsticeSummer Solstice

Select Item:
Event

Figure 27: The Complete Autostar Menu Tree Structure.

Solar System
Mercury
Etc.
Moon
Asteroids
CometsConstellations
Andromeda
Etc.
Deep Sky
Named Object
Galaxies
Nebulae
Messier
Etc.
Star
Named
SAO Catalog
DoubleVariable
Etc.
Satellite
SelectAdd
Delete
Edit
User Objects
SelectAdd
DeleteEdit
Landmarks
SelectAdd
DeleteIdentify
BrowseStart Search
Edit Parameters

Select Item:
ObjectTonight's BestHow Far is Far
A Star's Life
Downloaded Tours
User-created Tours

Tour Objects

Select Item:
Guided Tour
Accretion Disk
Etc.
B...
C...
D...
E...
F...
G...
H...
I...
J...
K...
L...
M...
N...
O...
P...
Q...
R...
S...
T...
U...
V...
W...
X...
Y...
Z...

A...

Select Item:
Glossary
Timer
Set
Start & Stop
Alarm
Set
On & OffEyepiece Calc.
Field of View
Magnification
Suggest
Display Options
Sun Warning
Getting Started
Brightness Adj.
Contrast Adj.
Beep
Battery Alarm
Landmark Survey
Sleep Scope
Park Scope
Cord Wrap

Select Item:
Utilities
Align
Easy
One Star
Two Star
Date
Time
Daylight Saving
Telescope
Telescope Model
Focal Length
Az/RA Ratio
Alt/Dec Ratio
Mount
Az/RA Percent
Alt/Dec Percent
Train Drive
Tracking Rate
Reverse L/R
Reverse Up/Dn
Quiet Slew
Max Elevation
Min AOSCalibrate Motor
High Precision
Targets
Astronomical
Terrestrial
Site
SelectAdd
DeleteEdit
Owner Info
Clone
Download
Statistics
Reset

Select Item:
Setup

AUTOSTAR's MENUS

Use the OBJECT menu
to select an object from thedatabase.
When your telescope isaligned and you select anobject from any of theselists, you just need to press
the GO TO key to move thetelescope so that it ispointed at the selected
object.

Object Menu
Almost all observing with Autostar is performed using the Object menu category. (Thetwo exceptions are the Guided Tours and Landmark Survey.) See GO TO SATURN, page20, for an example of observing using the Object menu. Also see USING THE GUIDED
TOUR, page 21.
Many Autostar menu categories contain databases. The Autostar object database isa list of viewable objects, such as stars, planets, comets, nebulae and so forth. Whenone of these objects is selected from the object database and is above the horizon,
Autostar moves your telescope (if properly aligned) and points it at the selected
object.
Note: Most celestial objects are visible in the sky for only part of the night
and also only visible part of the year. If an object is not visible on the night
you are observing, Autostar displays a message that the object is below
the horizon.

Over 30,000 objects areavailable for ETX-90AT,
ETX-105AT and ETX125AT models.
The available objects
include planets,
constellations, individual
stars, double stars, starclusters, galaxies, quasars,
satellites, asteroids andcomets.
Also, try out the Guided
Tour feature; the “Tonight’s
Best” Guided Tour will point
your telescope at the best
objects visible in the sky forevery given night of theyear.

The Object Menu options include:
Solar System is a database of the eight planets (Earth is not included) in order out
from the Sun, followed by the Moon, asteroids and comets.
Constellation is a database of all 88 Northern and Southern Hemisphereconstellations. To use this menu:
1.
2.

3.
4.

When this menu option is chosen and “Andromeda” displays, use the Scroll keys
to scroll through the constellation list.
Press ENTER to select a constellation and to display the coordinates of the constellation. Press one of the Scroll keys and information about the constellation willscroll across the display screen.
Press GO TO to display the list of stars in the constellation. Use the Scroll keys
to scroll through the list of stars in the constellation, from the brightest to dimmest.
Press ENTER to select a star and use the Scroll keys to display information about
the star. Press GO TO again to slew the telescope to that star.
Note: Use MODE to abort any of these operations.

Deep Sky is a database of objects outside our Solar System such as nebulas, starclusters, galaxies and quasars.
Star is a database of stars listed in different categories such as named, double,
variable or nearby.
Want to learn more about
Observing Satellites? Seepage 32.

Satellite is a database of Earth-orbiting objects such as the International Space
Station, the Hubble Space Telescope, Global Positioning System (GPS) satellites andgeosynchronous orbit satellites.
User Objects allows the user to define and store in memory deep-sky objects ofspecific interest that are not currently in the Autostar database. See page 32 for more
information.
Landmarks stores the location of terrestrial points of interest in the permanent
Autostar database.
IMPORTANT NOTE: To use the Landmark function, the telescope must be
located and aligned exactly as when the landmark was added to the
database.

Want to learn more about
Landmarks? See page 36.

■

Select: To select a Landmark already in the database (see ADD below), choosethe "Select" option and scroll through the list. Press ENTER to select a Landmark,then press GO TO and the telescope slews to the object.

■

Add: To add a Landmark, choose the "Add" option. Enter a name for theLandmark. Locate and center the Landmark in the eyepiece, then press ENTER.

Identify is an exciting feature for an observer who wants to scan the night sky andstart exploring. After the telescope has been properly aligned, use the Autostar Arrowkeys to move about in the sky. Then follow this procedure:

25

1.

Want to learn more about
using the Browse menu?
See page 39.

Use the Event menu
to look up dates of various
astronomical events, suchas sunrises and sunsets,
eclipses, moon phases,
meteor showers, equinoxes
and solstices...
...and not just for thecurrent date. Set any date,
past or future, when
initializing Autostar and you
can check the time forother events.
WARNING!
Never use
your ETX
Telescope tolook at the Sun! Looking
at or near the Sun willcause instant andirreversible damage toyour eye. Eye damage isoften painless, so there is
no warning to theobserver that damage has
occurred until it is toolate. Do not point thetelescope or its viewfinderat or near the Sun. Do notlook through the telescopeor its viewfinder as it ismoving. Children should
always have adultsupervision whileobserving.
Use the Glossary menu
to look up definitions ofastronomical terms and get
a description of Autostar
features.

26

IMPORTANT NOTE FOR ALL ALIGNMENT-BASED OPERATIONS:
Only use the Arrow keys to move the telescope during the Identify
procedure. Do not loosen the telescope locks or move the base or thealignment will be lost.
When a desired object is visible in the eyepiece, keep pressing MODE until the“Select Item: Object” menu is displayed. Press ENTER to select this menu.

2.

Scroll through the Object menu options until the “Object: Identify” screen appears.

3.

Press ENTER. Autostar searches the database for the identity of the object being
observed.

4.

If the telescope is not directly on an Autostar database object, the nearest
database object is located and displayed on the screen. Press GO TO and thetelescope slews to that object.

Browse allows you to search the database for objects with certain parameters, much
like a search engine. "Edit Parameters" lets you set various parameters for the search,such as: Object Type, Minimum Elevation, Largest, etc. Once you have set theparameters of the search, select "Start Search" and press ENTER. Autostar will
display the results of the search. See page 39 for more information.

Event Menu
The Event menu provides access to dates and times of astronomical events. The
Event database includes:
Sunrise and Sunset calculates the time that the Sun rises or sets on the current date.
Find rise and set times for other dates by entering a new date into the “Setup: Date”
menu. See DATE, page 28 and also see ETX TIPS, page 23.
Moonrise and Moonset calculates the time that the Moon rises or sets on the current
date. Find rise and set times for other dates by entering a new date into the “Setup:Date” menu. See DATE, page 28 and also see ETX TIPS, page 23.
Moon Phases displays the date and time of the next Full, New, 1st Quarter and 3rd
Quarter Moon.
Meteor Showers provides information on upcoming meteor showers, such as the
Perseids, the Leonids, etc. Also lists the dates of the showers and when they reachmaximum.
NOTE: Meteors are fast moving objects that cover large areas of the sky
and are usually best observed with the naked eye.
Solar Eclipse lists upcoming Solar Eclipses, including the date and type (total,
annular or partial) of eclipse and the location and time of the first and last contacts of
the Moon's shadow. Use the Scroll Up and Down keys to display the available data.
Remember, never use a telescope to look at the Sun! See WARNING! to the left.
Lunar Eclipse lists upcoming Lunar Eclipses, including the date and type (total,
partial, penumbral) of eclipse. Use the Scroll Up and Down keys to display theavailable data.
Min. (Minimum) of Algol is the minimum brightness of the dramatic eclipsing binary
star system, Algol. It is relatively close at a distance of 100 light years. Every 2.8 days
during a 10-hour period, Algol undergoes a major change in apparent magnitude as
one of the two stars passes behind the other. The combined magnitude of the twostars thus dips from +2.1 to a minimum of +3.4 halfway through the eclipse as thesecond star is hidden. Autostar calculates minimum magnitude time at mid-eclipse.
Autumn and Vernal Equinox calculates the time and date of the fall or springequinox of the current year.
Winter and Summer Solstice calculates the time and date of the winter or summer
solstice of the current year.

Glossary Menu
The Glossary menu provides an alphabetical listing of definitions and descriptions forcommon astronomical terms and Autostar functions. Access directly through theGlossary menu or through hypertext words embedded in Autostar. A hypertext word is
any word in [brackets], usually found when using the Autostar Help function or whenreading a scrolling message such as a description of a planet or star. Press ENTER
whenever a hypertext word is on screen and Autostar goes to the glossary entry forthat word.
To access directly from the Glossary menu, use the Scroll keys to scroll through thealphabet. Press ENTER on the desired letter. Scroll to the desired entry and thenpress ENTER to read the description.

Utilities Menu
Use the Utilities menu
to perform many ofAutostar’s useful features,such as setting an alarm,adjust the display contrast,
calculate the best eyepiecefor viewing an object, set
up your own landmark
survey, and so forth.

The Utilities menu provides access to several extra features within Autostar, including
a countdown timer and an alarm. The Utilities functions include:
Timer selects a countdown timer. This feature is useful for functions such as
astrophotography and tracking satellites. See OBSERVING SATELLITES, page 32. To
use the Timer, press ENTER, then choose “Set” or “Start/Stop."■

Set: Enter the time to be counted down, in hours, minutes and seconds, then press
ENTER.

■Start/Stop: Activates the timer set previously. Use the Scroll keys to toggle
between ON and OFF. When ON is displayed, press ENTER to activate the timer.
When the timer runs out, four beeps sound and the timer is deactivated.

Alarm selects a time for an alarm signal as a reminder. To use the Alarm, press
ENTER, then choose "Set" or "Start/Stop."Tip:
The Contrast Adjustment
feature is usually only
required in very cold
weather.
If you adjust the contrast
so that you can no longer
read the display, turn off
the power and turn it on
again. When Version
appears on the display (theinitial display screens are
not affected by theContrast control), press
MODE.

Tips:
To use the Landmark
function, the telescopemust be located andaligned exactly as when
the landmark(s) was added
to the database.
To add objects to theLandmark database, thetelescope must be locatedand aligned exactly as
when the original objects
were added to the
database.

■

Set: Enter the time of day for the alarm to sound, in hours, minutes and seconds,
then press ENTER.

■

Start/Stop: Activates the alarm set previously. Use the Scroll keys to toggle
between ON and OFF. When ON is displayed, press ENTER to activate thealarm. When the alarm time arrives, Autostar beeps. Press ENTER to deactivate
the alarm.

Eyepiece Calc calculates information about an eyepiece for the specific telescope towhich Autostar is connected.
■

Field of View: Scroll through a list of available eyepieces. When an eyepiece isselected, the field of view is calculated.

■

Magnification: Scroll through a list of available eyepieces. When an eyepiece isselected, the magnification is calculated.

■

Suggest: Autostar calculates and suggests the best eyepiece for viewing, basedon the telescope and the object being viewed.

Display Options enables or disables Autostar’s two initial displays. If both displays
are disabled, Autostar begins with the Date display.
■

Sun Warning: Turns the SUN WARNING message on or off.

■

Getting Started: Turns the GETTING STARTED message on or off.

Brightness Adj: Adjusts the brightness of the display using the Scroll keys. Whencomplete, press ENTER.
Contrast Adj: Adjusts the contrast of the display using the Scroll keys. When complete,press ENTER.
NOTE: This feature is usually only required in very cold weather.
Beep: Turns the beep on or off.
Landmark Survey automatically slews the telescope to all user-defined landmarks
with a short pause at each location. Press ENTER to start the survey. While a slew isin progress, press any key to skip that object and go to the next landmark on the list.
To observe a landmark for a longer period, press MODE when paused on the object
to stop the survey. Press ENTER to restart the survey at the first object on the list. See
LANDMARKS, page 36, for information about creating a Landmark survey.

27

Sleep Scope is a power saving option that shuts down Autostar and the telescope
without forgetting its alignment. With "Sleep Scope" selected, press ENTER to
activate the Sleep function. Autostar goes dark, but the internal clock keeps running.
Press any key, except ENTER, to re-activate Autostar and the telescope.
Park Scope is designed for a telescope that is not moved between observing sessions. Align the telescope one time, then use this function to park the telescope. Next
time it is powered up, enter the correct date and time – no alignment is required.
Pressing ENTER causes the telescope to move to its pre-determined Park position.
Once parked, the screen prompts to turn off power.
IMPORTANT NOTE: When the "Park Scope" option is chosen and thedisplay prompts you to turn off the telescope's power, Autostar is unable
to be returned to operation without turning the power off and then backon.
Cord Wrap, when set to "On," moves the telescope in such a way as to prevent thecords and cables attached to your telescope assembly from getting wound around theassembly and tangled as the telescope slews to objects. "Off" is the default setting.

Setup Menu
Use the Setup menu
to perform many of thefeatures that apply to theset up of your telescope,such as training the drive,
selecting terrestrial or
astronomical modes,changing observing site
information.

The Setup menu’s primary function is to align the telescope (see EASY ALIGN, page19). However, there are numerous other features available within the Setup menu,
including:
Date changes the date used by Autostar. This function is useful to check events in thepast or future. For example, set the Date menu for a day three months in the future.
Then check the "Select Item: Event" menu for the Sunset time on that date. See
EVENT MENU, page 26.
Time changes the time entered into Autostar. Setting the correct time is critical for
Autostar to properly calculate locations and events. Time may be set to 24-hour mode
(military time) by selecting the "blank" option which follows the "AM" and "PM"options.
Daylight Saving is used to enable or disable Daylight Savings time.
NOTE: Daylight Savings Time may be referred to by different names invarious areas of the world. Check local time to verify.
Telescope accesses the several options, including:■Model: Allows you to select the telescope model connected to Autostar.
■

Focal Length: Displays the focal length of the selected telescope.

■Az/RA Ratio and Alt/Dec Ratio: The ratios refers to the gears of the telescope's
motors. Do not alter these numbers.

■

Az/RA Percent: The Az (Azimuth)/RA (Right Ascension) Percent allows you toadjust the amount of azimuth backlash taken out by Autostar. Azimuth backlash
is the way the Arrow keys move the telescope along the azimuth (horizontal) axis.
If you enter a value near 100, the telescope tube responds more quickly (itresponds immediately at 100%) as you hold down an Arrow key and also slews(moves) the tube more quickly. If you enter a value near 0, it takes longer for the
tube to respond as you hold down an Arrow key and also slews the tube more
slowly. Experiment with this option. Try changing the percent value until you geta "feel" for the Arrow keys that is comfortable for you.

■

Alt/Dec Percent: The Alt (Altitude)/Dec (Declination) Percent operates identicalto the Az/RA Percent option (see above), but allows you to adjust the altitude
backlash, i.e., the way the Arrow keys move the telescope when moving along
the altitude (vertical) axis.

■

Train Drive: Trains the Altitude and Azimuth motors to locate objects with more
precision.
The first time you use your telescope or if you are experiencing any problems
with pointing accuracy, follow the procedure described in APPENDIX C: TRAINING
THE DRIVE, page 56, to insure accurate pointing and tracking.

28

■Tracking Rate: Changes the speed at which the telescope tracks targets in the
sky.
a.

■

■

Reverse UP/DOWN: Reverses the functions of the Up and Down Arrow keys
(i.e., the Up key moves the telescope down).

■

Quiet Slew: Sets the maximum slew rate to 1.5° for quieter operation.

■

Max Elevation: Allows you to enter a value in degrees that sets a limit as to how
far the optical tube can swing upward during a programmed slew. (Note that it
does not prevent you from performing a manual slew past this limit.) This is useful when you have a camera or other peripheral attached to the telescope—you
can prevent it from striking the telescope base.

■

Min AOS (Acquisition of Signal): Allows you enter a value in degrees. Thisvalue represents the altitude at which your telescope begins to slew when
acquiring a satellite track. This is useful when you are observing satellites, but atall tree or building is obstructing the telescope. For example, you might begin to
track the satellite at 15° altitude, instead of 5°. See OBSERVING SATELLITES,
page 32, for more information about satellites.
Calibrate Motor: If the telescope motors appear to have a problem, use thisoption to retest the motors before performing a Reset. This option is also used if
an Autostar unit is moved between telescopes, to match Autostar to the new telescope. To calibrate the motors, select this option and press ENTER.

■

Tip:
If the "ENTER to Sync"
feature is accessed by
mistake (holding the
ENTER key for more than
2 seconds), press MODE
to return to the previous
screen.

Want to learn more about
adding and editing sites?
See page 31.

Time Zone
Atlantic
Eastern
CentralMountainPacific
AlaskaHawaiiShift-4 Hours-5 Hours-6 Hours-7 Hours-8 Hours-9 Hours-10 Hours

Sidereal: The default setting for Autostar; sidereal rate is the standard rate
at which stars move from East to West across the sky due to the rotation of
the Earth.
b. Lunar: Choose this option to properly track the Moon over long observing
sessions.
c. Custom: Allows entry of user-defined tracking rates.
Reverse L/R: Reverses the functions of the Left and Right Arrow keys (i.e., theRight key moves the telescope to the left).

■

High Precision: If High Precision is turned on, when looking for a faint celestial
object (i.e., a nebula or galaxy), Autostar first slews to a nearby bright star anddisplays "ENTER to Sync." Center the star in the eyepiece, then press ENTER.
At that point the telescope has a high precision alignment to that part of the sky
and it then slews to the object that was originally requested.

Targets switches between Astronomical targets and Terrestrial targets. If"Astronomical" is selected, the telescope tracking motor is activated and any object
you observe will remain centered in the eyepiece. If "Terrestrial" is selected and thetelescope is aligned, the tracking motor is turned off. To learn how to track an object
automatically, see page 20.
Site provides access to several options including:■Select: Displays the currently selected observing site. Use the Scroll keys tocycle through all available sites (see "Add" below). Press ENTER when the site
you wish to select displays. Use this option when you move to a different
geographic location.
■

Add: Allows you to add new observing sites to the database (up to six sites may be
stored). Scroll through the list of Countries/States. Press ENTER when the site you
wish to add displays. Then choose the desired city in the same manner.

■

Delete: Deletes a stored site from the database.

■Edit: Edits a selected site, including: the name, latitude, longitude and time zone.
Time Zone refers to the Greenwich Mean Time (GMT) time zone shift. Users
West of Greenwich, England use “-” hours, East of Greenwich use “+” hours. For
the United States, look up the time zone shift in table above.
NOTE: Autostar compensates for daylight savings time, if selected. See“Setup Menu: Daylight Saving,” page 28.

Table 1: Time Zone Shift.
Calculations are for standard
time.

29

Owner Info accesses the owner information menu, including:■Name: Users may enter both their first and last names using the Up and Down
Arrow keys to cycle through the alphabet. Use the Right and Left Arrow keys tomove through the text. Press ENTER when the entry is complete.
■

Note:
The Download function
requires the optional #505
Astrofinder Software andCable Connector Kit. See
the instruction sheet
included with the kit for
more information on how to
download. Also see
OPTIONAL ACCESSORIES,
page 43.

Address: Use the Up and Down Arrow keys to enter your street address, city,
state and zip code. Press ENTER when the entry is complete.

Download transfers information from another Autostar. During the operation, thewarning “Downloading Do Not Turn Off” appears.
Clone uploads information from one Autostar handbox to another. Three options areavailable:■
Catalogs: Sends only user-defined object information, such as new satellite
orbits or comet data to another Autostar handbox.
■

Software: Sends only the basic Autostar software. This is useful if one user has
downloaded a new version of Autostar software from the Meade website(www.meade.com) and wants to pass this software along to friends.

■

All: Everything – user-defined information and Autostar software – is sent toanother Autostar.

Statistics provides basic statistical data about Autostar, including:■Characters Free: Shows how much room is available in user-defined object
memory.
■Version: Shows the current version of the Autostar software.

Reset completely resets Autostar. Most values entered into the menus revert tofactory defaults. Autostar requires initialization again after a Reset before proceedingwith observations. See INITIALIZING AUTOSTAR, page 18.

ETX TIPS
Surf the Web
One of the most exciting resources for astronomy is the internet. The internet is fullof websites with new images, discoveries and the latest astronomical information.
For example: When Mars made its closest approach in 60,000 years to our Sun in2003, astronomers around the world posted new photos daily.
On the internet, you can find websites for almost any topic relating to astronomy. Try
the following key word searches: NASA, Hubble, HST, astronomy, Messier, satellite,
nebula, black hole, variable stars, etc.
Check Meade’s website for the latest product and technical information. You candownload the latest software revisions, links to other astronomical sites, coordinatesof celestial objects and the latest satellite tracking information for your Autostar
handbox. See page 32 for more information. You’ll find our website at:www.meade.com/
Here are some other sites you might find interesting:• Sky & Telescope:
http://www.SkyandTelescope.com• Astronomy:
http://www.astronomy.com• The Starfield:
http://users.nac.net/gburke/• Astronomy Picture of the Day:
http://antwrp.gsfc.nasa.goc/apod• Heavens Above (satellite observing information):
http://www.heavens-above.com• Photographic Atlas of the Moon:
http://www.lpi.ursa.edu/research/lunar_orbiter• Hubble Space Telescope Public Pictures
http://oposite.stsci.edu/pubinfo/pictures.html

30

ADVANCED AUTOSTAROPERATION
Before trying out the examples in this section, familiarize yourself with the basic
operations of Autostar described earlier in this manual. The following examples
assume that you have a basic knowledge of Autostar and understand how to scroll toa desired menu or menu option and how to enter numbers and text. It also assumes
that you have initialized Autostar and have placed the telescope in the "Home"
position (when appropriate).

Adding Observing Sites
If you plan to observe using Autostar at different geographic locations, you can store
up to six observation sites in Autostar's memory to help simplify your telescope setup.
Perform these procedures using the Site options (Add, Select, Delete, Edit) of the
Setup menu.
To Add a Site to the user-defined site list:
In this example, you will choose a city and add it to the database list. You will thenselect the site to enable it.
1.
2.
3.
4.

5.

Navigate to the "Setup: Site" menu. Press ENTER,
Scroll through the options until "Site: Add" displays. Press ENTER.
Scroll through the list of countries/states. Press ENTER when the country/state
you wish to add displays.
Scroll through the list of cities. Press ENTER when the city you wish to add
displays. The Site is now added to the database. You may add 5 sites using thismethod (the sixth site is the site you entered during the Initialization process)To choose a site, navigate to "Site: Select." Press ENTER. Scroll through the listof sites. When the desired site displays, press ENTER.

To Edit a Site:
In this procedure, you will enter a location that is not available in the Autostar database by editing data of a nearby site. You will edit the location's name, latitude,
longitude and the time zone shift. You will then select the site to enable it.
You will need to know the latitude and longitude of your location to perform thisprocedure. This information is available on most maps.
1.

Time Zone
Atlantic
Eastern
CentralMountainPacific
AlaskaHawaiiShift-4 Hours-5 Hours-6 Hours-7 Hours-8 Hours-9 Hours-10 Hours

Table 1: Time Zone Shift.
Calculations are for standard
time.

Using the Add option, choose a site on the list that is closest to your observingsite and press ENTER so that the site is added to your observing sites list.
Choosing a site already on the list (as opposed to using the "Custom" feature)makes it easier to edit, as the "Time Zone" value may not need to be changed.
2. Scroll to "Site: Edit" and press ENTER. "Edit: Name" displays. Press ENTER.
3. The name of the site you have just entered to your list displays; if it does not,scroll to the site.
4. Using the Arrow keys, change the name of the site so that it now reads the nameof your observing location. Press ENTER. "Edit: Name" displays again.
5. Press the Scroll Down key and "Edit: Latitude" displays. Press ENTER.
6. Using the Number Keys, enter the latitude of your observing site and then press
ENTER. "Edit: Latitude" displays again.
7. Press the Scroll Down key and "Edit: Longitude" displays. Press ENTER.
8. Using the Number Keys, enter the longitude of your observing site and then press
ENTER. "Edit: Longitude" displays again.
9. Press the Scroll Down key and "Edit: Time Zone" displays. Press ENTER. (If thesite you chose from the list in step 1 has the same Time Zone as the site you are
editing, just press ENTER again to go on to the next step.) "Time Zone" refers to
the Greenwich Time Zone shift. Users West of Greenwich, use "-" hours (onehour per time zone) and users East of Greenwich use "+" hours. For the UnitedStates, look up the shift in Table 1, at the left.
10. After entering the shift, press ENTER. "Edit Time Zone" displays.
11. Press MODE. "Site: Edit" displays.
12. Using the Arrow keys, scroll to "Site: Select." The site you have just edited
displays. Press ENTER to select the site or press MODE to exit.

31

Using Autostar to Find Objects Not in the DatabaseIn this procedure, you will enter coordinates of celestial objects that do not appear inany of the Autostar database lists. You will enter the object's name and R.A. and Dec.
coordinates (required information). You may also enter the object's magnitude andsize (optional information).
Although Autostar contains an extensive database of celestial objects (stars, nebulae,
planets, etc.) that you can observe, you may eventually want to view objects that are
not part of the database. Autostar provides a feature that allows you to enter an
object's R.A and Dec coordinates in the "User: Objects" option of the Object menu andallows automatic slewing of the telescope to the user-entered coordinates.
In order to use this menu option, you first need to look up the R.A and Dec.
coordinates of the object or objects you wish to observe. Check out your local library,computer store or bookstore for astronomy books, CD Roms or magazines (such as
Sky & Telescope or Astronomy), to find coordinates of celestial objects. The
objects/coordinates you enter become part of your own permanent database, called"User Objects."
To enter coordinates of an object into the "User: Objects" option of the Object
menu:
1. Make sure Autostar has been initialized and the telescope has been aligned.
2. After the telescope is aligned, "Select Item: Object" displays. (If necessary, use
the Scroll keys to scroll through the menus, as previously described, to find thisoption.) Press ENTER.
3. "Object: Solar System" displays. Keep pressing the Scroll Up key until "Object:
User Object" displays and press ENTER.
4. "User Object: Select" displays. Press the Scroll Down key once. "User Object:
Add" displays. Press ENTER.
5. "Name" displays on the top line and a blinking cursor on the second line. Use theArrow keys, as previously described, to enter the name of the object you wish to
add to the database. When you are finished, press ENTER.
6. "Right Asc.: 00.00.0" displays. Use the Number keys to enter the digits for the
Right Ascension coordinate of your object. When you are finished, press ENTER.
7. "Declination: +00°.00'" displays. Use the Number keys to enter the digits for the
Declination coordinate of your object. If necessary, use the Scroll Keys to change"+" to "-." When you are finished, press ENTER.
8. Autostar then prompts you to enter the size of the object. This step is optional.
Use the Number keys to enter the size (in arc-minutes), if so desired and press
ENTER to go to the next display. If you do not wish to enter this information,
simply press ENTER.
9. Autostar then prompts you to enter the magnitude of the object. This step is also
optional. Use the Number keys to enter this information, if so desired and press
ENTER to go to the next display. "User Object: Add" displays again.
To GO TO a user-entered object:
In this procedure, you will choose an object from the User Object list and GO TO theobject.
1.

With "User Object: Add" displayed, press the Scroll Up key once. "User Object:
Select" displays. Press ENTER.

2.

Use the Scroll keys (if necessary) to scroll to the desired object. Press ENTER.

3.

The name of the object and the Right Ascension and Declination coordinates
display.

4.

Press GO TO and the telescope slews to the object.

Observing Satellites
In this procedure, you will prepare your telescope to observe a satellite pass.
1.
2.

32

Navigate to the "Object: Satellite" menu option and press ENTER.
Use the Scroll keys to scroll through the list of satellites.

3.
4.
5.

6.

7.
8.

Select a satellite from list and press ENTER.
"Calculating...." and then "Tracking..." displays. If the satellite is going to make apass, "Located" displays.
Use the Scroll keys to display data about the pass: aos – acquisition of signal andlos – loss of signal. If you subtract the aos from the los, you can calculate howlong the satellite will be visible. Location information also displays.
"Alarm" displays after the location information. Press ENTER and Autostar
automatically sets the alarm to sound a minute before the satellite's scheduledappearance. You may return to regular observations until the alarm goes off.
When the alarm goes off, return to the Satellite menu and press a Scroll key until
the desired satellite is on the top line of the display.
Press GO TO. Autostar slews the telescope to where the satellite should appear.
The motor drive stops and a countdown is displayed.
NOTE: If the scheduled appearance position of the satellite is obstructed(i.e., by a building, tree or hill), press ENTER and Autostar starts to movethe telescope along the expected satellite track. When the track clears theobstruction, press ENTER again to pause the telescope, then continue
with this procedure.

9.

With about 20 seconds left on the countdown timer, start watching through thetelescope viewfinder for the satellite to enter the field of view.
10. When the satellite enters the viewfinder field of view, press ENTER. The
telescope starts to track with the satellite.
11. Use the Autostar Arrow keys to center the object in the viewfinder, then lookthrough the eyepiece to view the object.
Satellite orbits change and new satellites (including the Space Shuttle) are launched.
Visit the Meade web site (www.meade.com) approximately once a month to get
updated information and instructions on how to download this data to Autostar. If
orbital parameters are more than one month old, the satellite pass may not happen at
the time predicted by Autostar. Downloading requires the optional #505 AstroFinder™
Software and Cable Connector Kit. See OPTIONAL ACCESSORIES, page 43.
Note: Satellite observing is an exciting challenge. Most satellites are in low
orbit, travelling at approximately 17,500 mph. When visible, they movequickly across the sky and are only in the field of view for a few minutes,
requiring Autostar to slew the telescope rapidly. Best viewing is near Sunrise
or Sunset when the sky is still dark. Viewing in the middle of the night can beproblematic because the satellite may pass overhead, but not be visible as it
is in the Earth's shadow.

How to Create Your Own Guided Tour
Note:
Meade’s Autostar Suiteprovides an easy way foran observer to create theirown Guided Tour. See
PHOTOGRAPHY WITH
MEADE’S AUTOSTAR SUITE,

page 42, and also
OPTIONAL ACCESSORIES,

page 43, for more
information.

When a Guided Tour is selected, Autostar slews your telescope to a predetermined listof objects and displays information about each object, such as type of object,
constellation location, R.A. and Dec coordinates and so forth. Autostar contains a few
Guided Tours which are programmed at the factory. But it is also possible for an
observer to create a custom Guided Tour.
A tour is basically an ASCII text file that contains a list of directions and descriptions.
Each line of a tour is either a comment line, a command line or a description.
What you will need:•
A PC with text editor or word processing software installed (the tour must be
saved as a "text only" or as a "MS-DOS text" file).
•
The Meade #505 Cable Connector Kit to download tour information to the Autostar
handbox.
Tour Modes
The objects chosen for a tour list are selected from Autostar's database or byentering the object's RA and Dec coordinates. The tour is presented in one of twomodes:
Automatic Mode: The title of an object appears on the first line and descriptive text
scrolls on line 2.

33

Interactive Mode: Tour name appears on the first line of the Autostar display and thename of the object displays on line 2. To display descriptive text in this mode, the user
must press ENTER.
Comment Line
Information in the Tour program that is not displayed, such as authorship, revisionhistory, copyrights, etc. All comments begin with a "/" character in column 1 of the line.
For example:/ Extreme Objects/ (c) 2000 Meade Instruments Corporation
Command Line
This line contains programming commands, including: R.A. and DEC. coordinates, atitle string, a description string and a keyword.
RA: Enter the Right Ascension of an object in the following format: HH:MM:SS.
Eg., 18:51:05
Dec: Enter the Declination of an object in the following format: DDdMMmSSs.
Eg., – 06d16m00s
Title String: Text within a title string is displayed as the title of the object. A title string
can contain up to 16 characters and must be surrounded by quotation marks. For
example. "M64" or "My Favorite Star."
In Interactive Mode, the title string appears on line 2 until it is selected with the ENTER
key.
In Automatic Mode or after Interactive Mode selection, the title string appears on line
1 while the description scrolls across line 2.
Keywords: Action to be performed during a tour. Autostar recognizes the following
keywords:
TITLE
IC
PLANETCOMETCONSTELLATIONPICK ONE/PICK END

TEXT
SAO
MOON
LUNAR ECLIPSESTAR
AUTO SLEW ON/OFFUSER
MESSIERSATELLITE
METEOR SHOWER
LANDMARK#ENDNGCCALDWELLASTEROIDDEEP SKY
DEFINE

Description String: Description of an object. Must be surrounded by quotation
marks. If the description is longer than one line, each line must end with a quotation
mark and a hard return. Begin the next description line with a quotation mark.
If quotation marks are to be displayed in the on-screen description, use two quote
marks at the beginning and end of the desired phrase. For example: "The Orion
Nebula is considered ""awesome"" by many who view it."
Writing a Tour
Using the list of commands listed above, a custom tour can be created. Placing theword AUTO SELECT before any of the command lines activates Automatic Mode and,
when selected, Autostar automatically searches and finds the designated object.
The following is a list of command lines, complete with keywords and necessarystrings:
TITLE
Title must be the first keyword in your tour after any comment lines and must be 15
characters or less. Autostar displays this title when "Guided Tour" is selected from themenus.
For example: TITLE "A Star's Life"TEXT "title string" "description string"This command allows you to display a text title and description.
USER ra dec "title string" "description string"This command line allows you to access a specific object with your own description.
Enter USER, then the RA and DEC of a desired object and its title and description.
Use the format described in the Command Line section.

34

The following commands specify objects that are already in the Autostar database. If
these commands follow the command AUTO SELECT, the object's title displays online 1 and its description scrolls across line 2.
Do not add a description string after the following command lines; these commands
access objects with existing description in the Autostar database.
NGC xxxx
Enter NGC followed by the desired New General Catalog number and Autostar
provides the user with a description of the object from its database. For example:
NGC 4256
IC xxxxEnter IC followed by the desired Index Catalog number and Autostar provides the user
with a description of the object from its database. For example: IC 1217
SAO xxxxxx
Enter SAO followed by the desired SAO number and Autostar provides the user witha description of the object from its database. For example: SAO 30200
Messier xxx
Enter MESSIER followed by the desired Messier number and Autostar provides theuser with a description of the object from its database. For example: M 101
CALDWELL xxx
Enter CALDWELL followed by the Caldwell number and Autostar provides the user
with a description of the object from its database. For example: CALDWELL 17
PLANET "name"Enter PLANET and then the name of the desired planet in quotes. Autostar provides
the user with a description of the selected planet from its database. For example:
PLANET "Pluto"
MOON
This command accesses information about the Moon from the Autostar database.
SATELLITE "name"Enter SATELLITE and then the name of the desired satellite in quotes. Autostar
displays information about the satellite from its database. For example: SATELLITE:"Intl Space Stn"
ASTEROID "name"Enter ASTEROID and then the name of the desired asteroid in quotes. Autostar
displays information about the asteroid from its database. For example: ASTEROID:"Ceres"COMET "name"Enter COMET and then the name of the desired comet in quotes. Autostar displays
information about the comet from its database. For example: COMET: "Halley"
LUNAR ECLIPSE
If LUNAR ECLIPSE is part of the tour, Autostar checks its database every time thetour is activated to see if a lunar eclipse is visible that evening. If no eclipse is visible,
this option is skipped and the tour proceeds on to the next object.
METEOR SHOWER
If METEOR SHOWER is part of the tour, Autostar checks its database every time thetour is activated to see if a meteor shower is visible that evening. If no meteor
shower is visible, this option is skipped and the tour proceeds on to the the next
object.
DEEP SKY "name"Enter DEEP SKY followed by the name of the desired object in quotes. For example:
DEEP SKY "Small Magellanic Cloud"
CONSTELLATION "name"Enter CONSTELLATION followed by the name of the desired constellation in quotes.
For example: CONSTELLATION "Leo Major"

35

STAR "name"Enter STAR followed by the name of the desired star in quotes. For example: STAR
"Vega"LANDMARK az alt "title" "description"
Enter the azimuth (az) for the desired object in the following format: xxxdxxmxxs. For
example: 123d27m00s. Then enter the altitude of the desired object in the following
format: xxdxxmxxs. Then enter the title string and description string in quotes. For
example:LANDMARK 123d27m00s 57d20m20s "Landmark 1" "North corner of apartmentbuilding"
PICK ONE / PICK END
These two statements are used to surround a list of items that Autostar can choose
from during a tour. Autostar begins at the top of the PICK ONE list and displays thefirst object from the list that is above the horizon and ignores the rest.
This statement is useful for developing tours that can be presented year round. For
each object type you wish to use to illustrate in your tour, pick 10 to 12 examples
spaced across the range of right ascension. Bracket them by the PICK ONE / PICKEND statements. One current example displays for the user. For example:
AUTO SELECT TEXT "Globular Cluster" "Globular clusters are huge balls of stars.""They contain 50,000 to 100,000 stars and are located on the fringes of our""galaxy."
PICK ONE
AUTO SELECT MESSIER 13
AUTO SELECT MESSIER 15
AUTO SELECT MESSIER 92
AUTO SELECT MESSIER 4
AUTO SELECT MESSIER 68
AUTO SELECT NGC 1234
AUTO SELECT TEXT "None Available" "I'm sorry. There are no bright globular""clusters visible at this time."
PICK END
AUTO SLEW ON / AUTO SLEW OFF
With AUTO SLEW ON enabled in the tour, Autostar automatically slews the telescope
to objects first before displaying the text description. This feature is useful when
designing tours in which observing certain objects is required. For example, anastronomy professor may require his students to observe six objects, four of which
Autostar automatically slews to in a tour. The students would have to manually slew
to the last two objects. He would then place AUTO SLEW ON before his first required
object and AUTO SLEW OFF after the fourth object.
#END
To end a tour, type the command #END on a separate line at the very end of the tour.
Downloading Tours
Once a tour is written and stored as an ASCII file (saved either as a "text only" or "MS
DOS text" file), load it into Autostar using the Autostar Update Utility on your PC. As
tours are downloaded into the handbox, Autostar examines the programming. If it
doesn't understand the terminology used within a tour, it flags questionable areas anddisplays them in a pop-up window on your computer screen. Make the necessary
corrections and try to download again. See the instruction sheet with your #505 Cable
Connector Kit for more information about downloading data to and interfacing with
Autostar.

Landmarks
This menu option allows you to define and store terrestrial objects in the Landmark
database. First, a landmark needs to be stored in memory using the "Landmark: Add"
option. To view a landmark, use the "Landmark: Select" option. Landmarks may also
be viewed using the "Landmark Survey" option in the Utilities menu.

36

To Add a landmark to the database:In this procedure, you will store the location of terrestrial landmarks in Autostar's
memory.
1.

Set the telescope in the home position, if necessary. Note for future reference
where the telescope is located and if you have aligned the telescope, whichalignment method is used.
Important Note: To use the Landmark function, the telescope must be
located and aligned exactly as when the landmark(s) was added to the
database.

2.

3.
4.
5.
6.
7.
8.

9.

Display the "Setup: Targets" menu option. Choose "Terrestrial" and press ENTER– "Setup: Targets" displays again. Choosing this option turns off tracking for
astronomical objects and is not useful for the viewing of terrestrial objects suchas those in the Landmark database. Be sure to change this option back to"Astronomical" when you wish to view celestial objects again.
Press MODE once. "Select Item: Setup" displays.
Press the Scroll Down key once and "Select Item: Object" displays. Press
ENTER. "Object: Solar System" displays.
Press the Scroll Up key twice and "Object: Landmarks" displays. Press ENTER.
"Landmark: Select" displays.
Press the Scroll Down key once. "Landmark: Add" displays. Press ENTER.
"Landmark Name" displays. Using Arrow keys, enter a name for the landmark
you wish to add to the database. When finished, press ENTER.
"Center Landmark. Press Enter" displays. Using only the Arrow keys (do not
manually move the telescope), move the telescope to the desired landmark andcenter the object in the eyepiece. Press ENTER. The object is now stored inmemory.
"Landmark: Add" displays. If you wish to add more landmarks, repeat steps 5through 7.

To Select a landmark from the database:
1. Make sure the telescope is located and aligned exactly as when the desired
landmark was entered into memory.
2. Display the "Landmark: Select" menu option. Press ENTER.
3. Use the Scroll keys to scroll through the list of objects you have previously
entered. When the desired object displays, press ENTER to select the object.
Use the Scroll keys to scroll through location information about the object, if
desired. Press GO TO to slew the telescope to the landmark.
4. Press MODE to exit.
To perform a Landmark Survey
This procedure allows you to perform a tour of the objects entered in the "Object:
Landmark" menu option—note that the Landmark Survey will function only if you havepreviously entered objects in the Landmark menu.
1. Navigate to "Utilities: Landmark Survey" menu and press ENTER.
2. "Landmark Survey: Slewing..." displays. The telescope moves to the first object
on the Survey list and displays the name of the object.
3. Press MODE to pause the Survey. Press ENTER to restart the survey at the firstobject of the survey.
To check on the available amount of memory in Autostar.
Autostar has a limited amount of memory. Once you begin to store Landmarks, User
Objects and other bits of information in Autostar, you will begin to use up memory.
This procedure allows you to check on how much memory is still available.
1.
2.

Navigate to the "Setup: Statistics" menu option and press ENTER.
"Statistics: 37.2K Char. Free" displays. This is the amount of memory that is stillavailable to the user.

Identify
This procedure allows you to use Autostar to identify objects you have found in thenight sky using the Arrow keys. If the object is not in Autostar's database, Autostar dis-37

plays information about an object in its database that is closest to the one you queried
about.
IMPORTANT NOTE: For this function to operate properly, you must first
set the telescope in the home position and initialize Autostar. If you
physically move the telescope after initialization, this function will fail tooperate properly.
In this procedure, you will center an object you wish to have identified by Autostar in
the telescope eyepiece and use the "Identify" menu to find out information about theobject or the nearest object to it in the Autostar database.
1.
2.
3.
4.

Center the object you wish to have identified in the telescope's eyepiece.
Navigate to the "Object: Identify" option and press ENTER.
"Searching..." displays. When Autostar finishes calculating, the name of theclosest object displays.
Press a Scroll key to display information about this object. Autostar displays
some or all the following information about the object with each press of a Scroll
key:

Displayed information:
Catalog or common name of object
Type of object
Right Ascension
Declination
Constellation
Magnitude
Size
Scrolling message

Example:Messier 107, NGC6171 orion Nebula, etc
Globular Cluster, Nebula, Black Hole, etc.
16:32:413°03'
Virgo orion, etc.
32'"This Globular Cluster is 10,000 lightyears away...."

Advanced Alt/Az Alignment
If you would rather choose your own alignment stars from the Autostar databaseduring the Alt/Az alignment procedure, Autostar offers two methods. Information forEquatorial (Polar) alignment is discussed in APPENDIX A, page 51.
Two-Star Alt/Az Alignment
Two-Star Alignment requires some knowledge of the night sky. Autostar provides a
database of bright stars and two stars from this database are chosen by theobserver for alignment.
1.
2.

Perform steps 1 through 7 as described in EASY (TWO STAR) ALIGN, page 19.
With "Align: Easy" displayed, use the Scroll keys to display "Align: Two Star."Press ENTER.
3. Place the telescope in the home position as described in the EASY ALIGN
procedure. When you have finished, press ENTER.
4 . "Select Star" displays. Autostar then displays a database of stars for theobserver to choose from. Use the Scroll keys to scroll to a star on the list that you
wish to align upon. Select a star that you can easily locate in the night sky. Press
ENTER.
5. The telescope slews to the star. Use the Arrow keys to move the telescope until
the star is centered in the eyepiece. Press ENTER.
6. Repeat procedure for the second alignment star. The telescope is aligned andyou are now ready to use Autostar's GO TO capabilities for a night of observing.
One-Star Alt/Az Alignment
One-Star Alignment requires some knowledge of the night sky. Autostar provides a
database of bright stars. One-Star Alignment is identical to Two-Star Alt/Az: Alignment(see TWO-STAR ALT/AZ ALIGNMENT, above), except only one star from this databaseis chosen by the observer for alignment.
IMPORTANT NOTE: The accuracy of One-Star Alt/Az Alignment, unlike
the Two-Star and Easy (Alt/Az) Alignment procedures, depends on how
well the observer levels the telescope and how close to North thetelescope is pointed when setting the Home Position. Because the othermethods use two stars to align upon, they are more precise than One-Star
Alignment.

38

BrowseThis menu allows you to search the database for objects with certain parameters,
much like a search engine. The "Edit Parameters" option lets you set various
parameters for the search and "Start Search" activates the search. A typical searchmight be performed as follows:
1.
2.
3.
4.

5.

6.

7.

8.

Select "Browse" from the Object menu. Press ENTER. "Browse: Start Search"displays.
Press one of the Scroll Keys and "Browse: Edit Parameters" displays. Press
ENTER.
"Edit Parameters: Largest (mins)" displays. "Mins" stands for arc-minutes. Press
ENTER.
"Largest (mins)" and a value displays. Using the Number keys, enter a size inarc-minutes. Autostar will search for objects up to this size and no larger. Press
ENTER.
"Edit Parameters: Largest (mins)" displays again. Press the Scroll Down key.
"Edit Parameters: Smallest (mins)" displays. Enter the value for the smallest sizeof an object that Autostar will search for in the database. Continue with
"Brightest," Faintest," and "Minimum Elevation," using the procedure described insteps 3 and 4.
After "Minimum Elevation," "Object Type" displays. Press ENTER." "+Black Hole"displays.If you do not wish to have "Black Holes" in your search, press ENTER
and the "+" changes to a "–." Press the Scroll Down to scroll to the next item.
"+Diffuse Nebula" displays. Continue to scroll through the list and press ENTER
if you wish to change the "+" to a "–" or vice-versa.
After you have scrolled to the last item on the "Object Type" list, press MODE
twice and the Scroll Down key once. "Browse: Start Search" displays. Press
ENTER. "Start Search: Next" displays. Press ENTER. Autostar searches the
database and displays the first object that matches the search parameters you
have entered. Use the scroll keys to display information about the object. Press
MODE and "Start Search: Next" displays again. Press ENTER and the next item
matching the parameters displays. Repeat this procedure to display all theobjects.
Press MODE repeatedly to leave this menu.

ETX TIPS
Observing Considerations•

Try to pick an observing site away from street and house lights and carheadlights. While this is not always possible, the darker the site, the better.

•

Give your eyes about ten minutes to adjust to the darkness before observing.
Give your eyes a rest from observing every ten or fifteen minutes to relieve
eyestrain.

•

Try not to use a standard flashlight. Experienced observers use red LED
flashlights, the red utility light on the Autostar handbox or tape red cellophane
over their flashlights to use for setup and map reading so they don’t have tocontinually readjust their eyes to the darkness. Be careful not to shine bright
lights if there are other observers in the area. Do not shine a flashlight into thetelescope while someone is observing!

•

Dress warmly. It gets chilly when you’re sitting for prolonged periods.

•

Practice setting up your equipment during the day or in a lighted area tobecome familiar with it before going to a dark site.

•

Use your 26mm eyepiece to view terrestrial objects and wider areas of space,such as open star clusters. Use optional higher power eyepieces, such as a
9mm eyepiece (see OPTIONAL ACCESSORIES, page 43 for more details), when
you wish to view something up close, such as craters on the Moon or the ringsof Saturn.

•Bring your instructions manual along with you when you observe. Become
familiar with its layout, so it will be easier for you to look up information withjust a (red) flashlight.

•

Invite your friends and family to come and observe with you. But practicelocating 3 or 4 objects to show them beforehand; if you have long delays, they
will become bored and lose interest. Also, demonstrate how to focus thetelescope in a well-lit area before you go to to the observing site.

39

PHOTOGRAPHY
7

2

6

4

1

3

5

Fig. 28: Example of photography through the ETX using the #64 T-Adapter: (1) Shortsection of #64 T-Adapter; (2) Extension section of #64 T-Adapter; (3) Knurled attachment ring;(4) T-mount; (5) Flip-mirror control in “down” position; (6) 35mm camera body; (7) Format 1.

Fig. 29a: Flip mirror control inthe “up” position.

Fig. 29b: Flip mirror control inthe “down” position.

Fig. 30: Example of a format
1 photo.

Photography with a 35mm Camera
Photography through your ETX model requires the addition of the optional #64
T-Adapter (see OPTIONAL ACCESSORIES, page 43). With the #64 T-Adapter attachedto the telescope (Fig. 28), through-the-telescope photography is possible with any
35mm camera body with a removable lens. In this way the telescope effectively
becomes the lens of the camera.
For through-the-telescope photography, turn the flip-mirror control (5, Fig. 28) to the“down” position, allowing light to pass straight through the telescope and out the photo
port (Figs. 29a and 29b). With the flip-mirror control in the “down” position and thephoto port’s dust cover removed, you can see the front lens of the telescope when you
look through the photo port. The #64 T-Adapter threads onto the photo port, followed
by a T-mount for the particular brand of 35mm camera being used, followed by thecamera body (with the camera lens removed).
The #64 T-Adapter consists of two sections (1 and 2, Fig. 28), which are threaded
together in shipment. You may use either of the following photographic mounting
formats to couple the camera body to the telescope’s photo port thread.
• Format 1: Camera Body + T-Mount + Section (1) of the #64 T-Adapter (7, Fig. 28).
ETX-90AT
1250mm at f/13.8
ETX-105AT
1640mm at f/15.6
ETX-125AT
1900mm at f/15
Format 1 utilizes only the short section of the #64 T-Adapter to permit close-couplingof a camera body to the telescope. In this format vignetting will occur; thephotographic image will appear on film with a slight darkening at the corners of the
35mm frame (see Fig. 30).
• Format 2: Camera Body + T-Mount + Sections (1) and (2) of the #64 T-Adapter (seeFig. 28).
ETX-90AT
ETX-105AT
ETX-125AT

Fig. 31: Example of a format
2 photo.

1450mm at f/16
1830mm at f/17.42310mm at f/18

Format 2 utilizes both sections of the #64 T-Adapter threaded together to form a rigid
unit. In this configuration there is no field vignetting; images are illuminated to theedges of a standard 35mm frame (see Fig. 31).
To frame an object in the viewfinder of the 35mm camera body, slightly loosen theknurled attachment ring (3, Fig. 28), which threads the #64 T-Adapter to thetelescope’s photo port; rotate the camera body to achieve proper framing of theobject; then re-tighten the knurled ring.

40

Photography through a long lens, such as the ETX, requires special technique forgood results. The photographer should expect to use several rolls film in acquiring thistechnique. Long-lens photography has its own rewards, however, which short-focus
lenses cannot duplicate.
A Few Tips on Photography
1.Use the standard tripod or the optional table tripod ( see OPTIONAL ACCESSORIES,
page 43) as a platform for the telescope. At effective focal lengths of 1250mm to1450mm (ETX-90AT), 1640mm to 1830mm (ETX-105AT) or 1900mm to 2310mm(ETX–125AT), even small external vibrations can easily ruin an otherwise good
photo.
Caution: With the #64 T-Adapter and a camera body mounted to the ETX
photo port, the telescope can be rotated vertically only 45°. Moving past thispoint may damage the telescope and camera.
2. Use a cable-operated shutter release with your camera. Touching the camera bodyto operate the shutter will almost certainly introduce undesirable vibrations.
3. Focus the image with extreme care. While observing the subject through thecamera’s reflex viewfinder, turn the ETX's focus knob (8, Fig. 1) to achieve the
sharpest possible focus. Note that some 35mm cameras may have an optional
focusing screen (available from the manufacturer) for use with a long telephotolens. This screen provides a brighter and clearer image to focus and is highly
recommended.
4. Correct shutter speeds vary widely, depending on lighting conditions and film used.
Trial-and-error is the best way to determine proper shutter speed in any given
application.
Note: The camera used with an ETX model may have an exposure meterthat is still active when the standard lens is removed and the body isconnected to the telescope with the T-mount. If used for terrestrial
photography, the camera meter should be acceptable. If used for
astrophotography, the meter probably will not provide good results sincecamera meters are not made to compensate for a dark sky.
5. Terrestrial photography through an ETX model is sensitive to heat waves risingfrom the Earth’s surface. Long distance photography is best accomplished in theearly morning hours before the earth has had time to build up heat.
6. Photography of the Moon and planets through an ETX model can be especiallygratifying, but points 1 through 4 should be particularly noted in this case. Lunar orplanetary photography requires that the telescope be polar aligned (seeEQUATORIAL (POLAR) ALIGNMENT, page 51).
Note: Long-exposure photography of deep-sky objects is not practical withan ETX model, since this type of photography requires special electronic andoptical guiding devices not available for this telescope.
Photography with a Digital Camera
Although digital cameras still cannot match the quality of images provided bytraditional 35mm cameras, they provide some significant advantages to the casualastrophotographer: You do not have to develop the images (instant images), lower
costs, computer and internet readiness. And because unwanted photos are easily
discarded, they provide the freedom to experiment.
Digital cameras present some problems for the astrophotographer: Many models
have lenses that cannot be removed, difficulties in attaching to a telescope, possible
vignetting, lack manual focusing and shorter exposure times.
Shorter exposure times is one of the biggest drawback. Long exposures with digital
cameras introduce undesirable noise and artifacts into a digital image. This limits therange of astro images to the Moon, planets and bright stars.
Some tips for better photos:•

If you cannot remove the lens to your camera, look for a commercially available
digital t-adapter. New solutions for attaching a digital camera to a telescope are
becoming available as time goes by.

41

•

•
•

•
•
•
•
•
•

•

If the camera is not directly coupled to the eyepiece, keep it as close to theeyepiece as possible and center the image to be photographed to minimize
vignetting (darkening of the edges of the photo).
Try to block ambient light (from street lights, house, etc.) from the eyepiece andthe camera with a piece of cardboard, a screen, etc.
Keep extra (charged) batteries on hand for your camera as digital cameras often
drain batteries in a short period of time. Rechargeable Lithium batteries provide
power for a longer period than non-rechargeable batteries. If practical, use an AC
adapter.
Avoid short-focus eyepieces. They present many difficulties for digital cameras.
If using manual focus, set to infinity. Otherwise, using the camera's autofocus isOK.
Experiment with your camera's exposure, brightness and /or contrast settings.
Keep notes for future reference.
Clean eyepieces and camera lens as needed.
Many digital cameras have a manual ISO setting. Short exposures times work thebest.
Use your camera's highest image quality and lowest compression settings.
Although this fills up your camera's memory more quickly, it produces the best
quality photos.
Use the camera's timer or remote shutter release (if available for your camera) tominimize vibration. Wireless shutter releases may be available for some model
digital cameras. If you do not have a shutter release, use thecamera’s timer (sometimes called “self-timer”), which is available with mostdigital cameras. The timer may also minimize vibration.

Photography with Meade’s Autostar Suite
The Autostar Suite with Meade LPI (Lunar Planetary Imager) and Planetarium softwareturns your Meade ETX telescope, Autostar and PC into even more powerful and easyto-use astronomical instrument.
LPI (Lunar Planetary Imager, Fig. 32) combines the power of an electronic
astronomical imager with the simplicity of a web cam. Check out the following LPI
features:Fig. 32: The Lunar
Planetary Imager.

• Achieve great results the first time out on the Moon, planets, brighter deep-sky
objects and terrestrial targets.
• Easy to use with real-time display of object on your PC screen. Just center, focus
and shoot.
• Magic Eye software-assisted focusing.
• Automatic and manual exposure control from .001 to 15 seconds (up to 450x longer
than web cams).
• Automatically takes multiple exposures.
The Autostar Suite Software includes powerful tools to help you get the most fromyour Meade ETX telescope:• Sophisticated planetarium program with over 19 million objects.
• Select objects from the planetarium display and the telescope slews to thoseobjects.
• Create your own Guided Tours.
• Advanced Image Processing Software including Unsharp Masking, Convolution
Filtering and many other features.
• Control all Autostar functions from your PC.
• Talking Telescope software translates Autostar text to synthesized speech throughPC speaker.
• Includes a cable to connect your ETX model to your PC.
• Point-and-click Autostar tour generation.
• Create observing lists and download to Autostar.

42

OPTIONAL ACCESSORIES
A wide assortment of professional Meade accessories are available for the for ETX
telescopes. Meade accessories greatly extend many important applications to thetelescope, from low-power, wide-field terrestrial viewing to high-power lunar andplanetary observing. The premium quality of these accessories is well-suited to thequality of the instrument itself.
Meade telescopes and accessories, including optional accessories for ETX
telescopes, are available at more than 3,000 dealer locations in the U.S. and Canada
and through Meade international distributors worldwide. Once you have identified theaccessories you wish to order, contact your local Meade authorized dealer. To find a
dealer near you call (949) 451-1450 or visit the Meade website at www.meade.com.
Autostar Suite with Meade LPI (Lunar Planetary Imager) and Planetarium
software (Fig. 33) turns your Meade ETX telescope, Autostar and PC into even more
powerful and easy-to-use astronomical instruments. Includes cable for connecting
Autostar to your PC. See page 42 for more details.

Fig. 33: Autostar Suite with
Lunar Planetary Imager.

#505
Cable
Connector
Kit:
With
Meade
AstroFinder
software (Fig. 33) loaded into your PC, Autostar-equipped ETX–90AT, ETX-105AT,
and ETX-125AT telescopes may be remotely controlled from the PC display. The#505 Cable Connector Set, permitting connection of ETX, Autostar and PC, is included with each AstroFinder package.
Eyepieces: For higher and lower magnifications, Meade Super Plössl (SP) andSuper Wide Angle (SWA) eyepieces (Fig. 34), as well as the Series 4000 8mm to24mm Zoom eyepiece, yield high-resolution imaging with all ETX telescope models.
A useful selection includes the SP 9.7mm, SP 12.4mm and SWA 18mm. Under goodseeing conditions, Meade Ultra Wide Angle 4.7mm and 6.7mm eyepieces present thewidest obtainable fields of view at high powers and are well suited for observing theMoon and planets. Powers obtained with each eyepiece are shown in the following
table.

Fig. 34: Optional
Eyepieces yield higher andlower magnifying powers.

Fig. 35: Use the #126 2x
Barlow Lens to double themagnification of theeyepiece employed.

Eyepiece

ETX-90AT
Power 2x Barlow

ETX-105AT
ETX-125AT
Power 2x Barlow Power 2x Barlow

SP 6.4mm
SP 9.7mm
SP 12.4mm
SP 15mm
SP 20mm
SP 26mm *SP 32mm
SP 40mm

195X
129X
101X
83X
63X
48X
39X
31X

390X
258X
202X
166X
126X
96X
78X
62X

230
152
119
98
74
57
46
37

459
303
237
196
147
113
92
74

297X
196X
153X
127X
95X
73X
59X
48X

594X**
392X
306X
253X
190X
146X
119X
96X

SWA 13.8mm
SWA 18mm
SWA 24.5mm

91X
69X
51X

182X
138X
102X

107
82
60

213
163
120

138X
106X
78X

275X
211X
155X

UWA 4.7mm
UWA 6.7mm

266X
187X

N/A
374X **

313
219

N/A
439**

404X
284X

N/A
567X*** Included as standard-equipment with the ETX models.
** Use these eyepieces only under extremely steady atmospheric conditions.

#126 2x Barlow Lens: An amplifying lens, the multi-coated #126 2x Barlow (Fig. 35)
doubles the power of all eyepieces with which it is used. Insert the #126 into thetelescope’s eyepiece holder first, followed by an eyepiece. Example: By itself, the26mm eyepiece yields a power of 73X with the ETX-125AT; when used with the #126
2x Barlow Lens, this eyepiece yields 146X.
Fig. 36: #825 Right-Angle
Viewfinder.

#825 8 x 25mm Right-Angle Viewfinder: Included as standard-equipment on
ETX-105AT and ETX-125AT models, the 8 x 25mm Right-Angle Viewfinder (Fig. 36)
permits a comfortable 90° viewing position with 90mm ETX models as well. The #825
fits into the same bracket as the 8x21mm viewfinder supplied with ETX-90AT
telescopes. The viewfinder’s wide-angle 7.5° actual field facilitates object location.
Precise focusing of the image is accomplished with a helicoid mechanism.

43

#64 T-Adapter: The basic means of photography through any ETX Astro telescope,
the #64 T-Adapter threads to the rear cell of the telescope, followed by a T-Mountappropriate to the user’s brand of 35mm camera. In this way, the camera body isrigidly coupled to the telescope's optical system, which in effect becomes the camera's
lens (see PHOTOGRAPHY, page 40).

Fig. 37: The #932 45°
Erecting Prism.

Fig. 38: #774 Hard
Carrying Case shown withan ETX-90AT.

Fig. 39: The #765 Soft
Carry Bag for the
ETX-90AT.

#932 45° Erecting Prism: All ETX models include an internal optically-flat mirror toreflect light to the telescope’s 90° astronomical observing position. In this position thetelescope’s image is upright, but reversed. For terrestrial observing with an ETXmodel, the #932 Erecting Prism (Fig. 37) correctly orients the eyepiece image andprovides a convenient 45° observing angle.
#774 Hard Carrying Case (for the ETX-90AT), #776 Hard Carrying Case (for the
ETX-105AT) and #775 Hard Carrying Case (for the ETX-125AT): For secure
portability of ETX Astro Telescope models in the field, Meade hard carrying cases (Fig.
38) are fully lined with fitted foam inserts. They accept the complete ETX Astro
Telescope plus optional accessories.
#765 Soft Carry Bag: The Meade soft-padded carry bag (Fig. 39) is well suited totravel with the ETX-90AT Astro Telescope. Each carry bag includes a shoulder strap
and permits ready transport of the complete telescope, including accessories.
Power Adapters and Cords: In addition to their internal battery packs, ETX-90AT,
ETX-105AT, and ETX-125AT telescopes may be powered from standard 115vAC
home electricity with the #541 AC Adapter. The #541 plugs into any standard homeoutlet and includes a 25 ft. cord connecting to the telescope’s control panel. Input
voltage to the telescope is 12vDC. Alternately, an ETX telescope may be powered in
the field from an automobile cigarette lighter plug by using the #607 Power Cord, a
25-ft. cord that plugs into the telescope’s control panel and supplies 12vDC directlyfrom the car battery.
#1244 Electric Focuser (for the ETX-90AT and ETX-105AT) and #1247 Electric
Focuser (ETX-125AT): Meade-engineered for smooth, rapid focusing with any
ETX model, each electric focuser (Fig. 40) includes coarse and micro-fine speeds. The
standard-equipment hand controller accepts one (user-supplied) 9-volt battery andfocuses the ETX telescope. On the ETX models, the focuser plugs into and is
powered by, the telescope’s control panel, with operation effected through either the
Autostar or the optional #497 Autostar Computer Controller.
#887 Advanced Field Tripod for the ETX-105AT or ETX-125AT: For extra stability insensitive applications of the ETX-105AT or the ETX-125AT even at the highest magnifications, the fixed height #887 Tripod permits either altazimuth orequatorial orientation of the telescope for astronomical or terrestrial observing. The#887 includes an equatorial wedge for polar alignment. The tripod's 2"-diameter steel
legs collapse for easy transport in the field.

Fig. 40: #1244 Electric
Focuser.

#880 Table Tripod (for ETX-90AT) and #881 Table Tripod (for ETX-105AT and theETX-125AT): For fully automatic tracking, a table tripod may be added allowing forpolar alignment of the telescope. See Fig. 41.
Each table tripod includes two fixed legs and two variable-length legs inscribed with arange of latitude settings for quick polar alignment. At observing latitudes below about
25°, the optional #1422 Low-Latitude Balance Weight is recommended for ETX-90
Astro Telescope models; the low-latitude balance weight is included with the table
tripod for the ETX-105AT and the ETX-125AT Astro Telescopes.

Fig. 41: The #880 Table
Tripod.

44

MAINTENANCE
Your ETX model telescope is a precision optical instrument designed to yield alifetime of rewarding observations. Given the care and respect due any precision
instrument, the telescope will rarely require factory servicing or maintenance. Use thefollowing guidelines:
1. Avoid cleaning the telescope’s optics: a little dust on the front surface of thetelescope’s correcting lens causes virtually no degradation of image quality andshould not be considered reason to clean the lens.
2. When absolutely necessary, remove dust from the front lens with gentle strokes ofa camel-hair brush or blow it off with an ear syringe (available at any pharmacy).
Do not use a commercial photographic lens cleaner.
3. You may remove organic materials (e.g., fingerprints) from the front lens with asolution of 3 parts distilled water to 1 part isopropyl alcohol. A single drop of
biodegradable dishwashing soap may be added per pint of solution. Use soft, whitefacial tissues and make short, gentle strokes. Change tissues often.
Caution: Do not use scented, colored or lotioned tissues or damage could
result to the optics.
4. In the very rare situation where cleaning the inside surface of the corrector lensbecomes necessary, unthread the lens cell located at the front of the main tube.
The entire correcting lens and secondary mirror system are mounted in this cell.
You may use the lens-cleaner solution described in step 3 to clean the insidesurface of the lens.
Caution: Do not touch the aluminized circular surface of the secondary
mirror with a finger, a tissue or any other object. This will almost certainly
scratch the mirror surface.
Note: When cleaning the inside surface of the correcting lens, leave the lens
mounted in its metal cell throughout the process. Do not remove the lensfrom its metal housing or optical alignment of the lens will be lost,necessitating a return of the telescope to the Meade factory.
5. If your ETX model is used outdoors on a humid night, telescope surfaces may
accumulate water condensation. While such condensation does not normallycause any damage to the telescope, it is recommended that the entire telescope
be wiped down with a dry cloth before being packed away. Do not, however, wipe
any of the optical surfaces. Rather, simply allow the telescope to sit for some timein warm indoor air, so that the wet optical surfaces can dry unattended. In addition,
the dust cap should not be placed back on to the optical tube until the telescope isthoroughly dry.
6. If your ETX model is not to be used for an extended period, perhaps for one monthor more, it is advisable to remove the eight AA-size batteries from inside the drivebase. Batteries left installed for prolonged periods may leak, causing damage to thetelescope’s electronic circuitry (see HOW TO ASSEMBLE YOUR TELESCOPE AND TRIPOD, page 12).
7. The super-gloss anodized finish of any ETX model’s deep-violet optical tube fades
if left in direct sunlight for prolonged periods.
8. Do not leave your ETX model outdoors on a warm day or inside a sealed car for an
extended period of time; excessive ambient temperatures can damage thetelescope’s internal lubrication and electronic circuitry.
9. A set of two (English-format) hex wrenches is provided with ETX models. These
wrenches are used as follows:•
Small wrench (.05”): Use the small wrench to tighten the set-screws of
any knobs that may loosen (e.g., the focus knob or flip-mirror controlknob).
•
Medium wrench (1/16”): This wrench is used to detach the viewfinder
bracket from the telescope’s rear cell.

45

Storage and Transport
When the telescope is not in use, store it in a cool, dry place. Do not expose theinstrument to excessive heat or moisture. It is best to store the telescope in its
original box with the vertical and horizontal locks (6 and 9, Fig. 1) in the unlocked
positions. If shipping the telescope, use the original box and packing material toprotect the telescope during shipment.
When transporting the telescope, take care not to bump or drop the instrument; thistype of abuse can damage the optical tube and/or the objective lens and knock the
optics out of alignment. It is highly recommended to use an optional carry case totransport the telescope (see OPTIONAL ACCESSORIES, page 43).
Inspecting the Optics
A few words about the so-called “Flashlight Test:" If a flashlight or otherhigh-intensity light source is pointed down the main telescope tube, the view
(depending upon the observer’s line of sight and the angle of the light) may reveal
what appear to be scratches, dark or bright spots or uneven coatings, giving theappearance of poor quality optics. These effects are only seen when a high intensity
light is transmitted through lenses or reflected off the mirrors and can be seen on any
high-quality optical system, including giant research telescopes.
The optical quality of a telescope cannot be judged by the “flashlight” test; the true testof optical quality can only be conducted through careful star testing.
Troubleshooting
The following suggestions may be helpful with operation of the ETX-90AT,
ETX-105AT and ETX-125AT.
The power indicator light on the telescope does not come on or there is no
response when pressing the Autostar Arrow keys:• Verify that the Computer Control panel power switch (A, Fig. 2) is in the ON
position.
• Verify that the Autostar coil cord is firmly connected to the HBX port (C, Fig. 2).
• If using internal power (batteries), verify that the batteries are installed correctly andthat they have sufficient charge (see HOW TO ASSEMBLE YOUR TELESCOPE AND
TRIPOD, page 12).
Note: If the batteries are getting low on charge, there will be a marked
difference in the slew speed. The speed indicator lights may also flash andthe speed may change. If any of these symptoms occurs, turn the power off
and replace the batteries.
• If using an external power source, verify that it is properly connected between the
12-volt connector (D, Fig. 3) and either a wall plug (AC source) or a car cigarette
lighter (DC source).
• If Autostar does not respond to commands, move the power switch to OFF and thenback to ON.
• If the telescope does not slew after power is applied or if the motor quits or stalls,
verify that there are no physical obstructions that would impede telescope
movement.
• If all physical obstacles are removed and the telescope still does not moveproperly, turn off the power and unplug Autostar. Plug Autostar back in and turn the
power back on.
Unable to see an image through the eyepiece:• Confirm that the lens cover has been removed from the telescope.
• Confirm that the flip-mirror control (14, Fig. 1) is in the “up” position if using theeyepiece holder (4, Fig. 1) so that light is directed to the eyepiece (1, Fig. 1).
Confirm that the flip-mirror control is in the “down” position if using the #932
Erecting Prism or doing photography with an ETX model (see TELESCOPEFEATURES, page 6 and PHOTOGRAPHY, page 40).

46

Object appears in the viewfinder but not in the eyepiece:• The viewfinder is not properly aligned with the telescope (see ALIGNING THE
VIEWFINDER, page 14).
Slew speed does not change when you press the SPEED key or the telescopemoves slowly even though the fast slew speed is chosen:• The battery power may be low (see HOW TO ASSEMBLE, page 12).
Telescope does not track a celestial object:• Make sure that the telescope is correctly aligned. See EASY (TWO-STAR) ALIGN, page18, for more information.
Images through the eyepiece appear unfocused or distorted:• The magnification may be too high for the viewing conditions. Back off to a lower
power eyepiece (see CHOOSING AN EYEPIECE, page 15).
• If inside a warm house or building, move outside. Interior air conditions may distort
terrestrial or celestial images, making it difficult, if not impossible, to obtain a sharp
focus. For optimal viewing, use the telescope outside in the open air instead ofobserving through an open or closed window or screen.
• If viewing a land object on a warm day, heat waves will distort the image (seeTERRESTRIAL OBSERVING, page 16).
• For clear viewing of objects, turn the focus knob (8, Fig. 1) slowly since the “in-focus”
point of a telescope is precise. Turning the focus knob too quickly may cause thefocus point to pass without notice.
• The optics within the telescope need time to adjust to the outside ambient
temperature to provide the sharpest image. To cool down the optics, set thetelescope outside for 10 to 15 minutes before observing begins.
Telescope moves off a terrestrial object while observing:• Verify that the vertical and horizontal locks are tight (see TELESCOPE FEATURES,
page 6).
Telescope does not move past a certain point:• The built-in vertical or horizontal rotational “stops” may have been reached. See #6,
page 7.
Telescope pauses when changing slew direction:• This pause is normal.
A terrestrial object appears reversed left-for-right:• An eyepiece in the standard 90° observing position (4, Fig. 1) reverses an object
left-for-right: To view a correctly oriented image requires the optional #932 Erecting
Prism (see OPTIONAL ACCESSORIES, page 43).
Meade Customer Service
If you have a question concerning your ETX model, call the Meade Instruments
Customer Service Department at (949) 451-1450. Customer Service hours are 7:00
AM to 6:00 PM, Pacific Time, Monday through Friday. In the unlikely event that the
ETX requires factory servicing or repairs, write or call the Meade Customer Service
Department first, before returning the telescope to the factory, giving full particulars as
to the nature of the problem, as well as your name, address and daytime telephone
number. The great majority of servicing issues can be resolved by telephone,
avoiding return of the telescope to the factory.

47

SPECIFICATIONSSpecifications: ETX-90AT Astro Telescope
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain
Primary mirror diameter . . . . . . . . . . . . . . . . . . . 96mm (3.78”)
Clear aperture . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90mm (3.5”)
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1250mm
Focal ratio (photographic speed). . . . . . . . . . . . . . . . . . . f/13.8
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . 11.5 ft (3.5m)
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 1.3 arc secs
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 11.7
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.16°/inch
Maximum practical visual power . . . . . . . . . . . . . . . . . . . 325X
Optical tube dimensions(dia. x length) . . . . . . . . . . . 10.4cm x 27.9cm (4.1” x 11”)
Viewfinder . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 x 21mm
Secondary mirror obstruction (dia.; %) . . 27.9mm (1.1”); 9.6%
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine
Setting circle diameters . . . . . . . . . . . . . . . Dec.: 3.5”; R.A.: 7”
Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC
Motor Drive System DC servo motors with encoders, both axes
Bearings:
Altitude. . . . . . . . . . . . . . . . . . . . . . . UHMW polyethylene
Azimuth . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . PTFE
Materials:
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum
Mounting . . . . . . high-impact ABS, aluminum-reinforced
Primary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A
Telescope dimensions:. . . . . . . . . . . . . . . . 38cm x 18cm x 22cm (15” x 7” x 9”)
Telescope net weight:(incl. Autostar & batteries) . . . . . . . . . . . . 3.5kg (7.8 lbs)
Telescope shipping weight. . . . . . . . . . . . . . . . 5.8kg (12.8 lbs)
Battery Life (approx.):with Autostar. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs

Specifications: ETX-105AT Astro Telescope
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain
Primary mirror diameter . . . . . . . . . . . . . . . . . . 116mm (4.56”)
Clear aperture . . . . . . . . . . . . . . . . . . . . . . . . . . 105mm (4.13”)
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . 1470mm (57.8”)
Focal ratio (photographic speed) . . . . . . . . . . . . . . . . . . . . f/14
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . . . 4.6m (15 ft)
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 arc secs
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 12.1
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 0.99°/inch
Maximum practical visual power. . . . . . . . . . . . . . . . . . . . 420x
Optical tube dimensions(dia. x length) . . . . . . . . 12.4cm x 32.8cm (4.88” x 12.9”)
Viewfinder . . . . . . . . . . . . . . . . . . . . . . . . 8 x 25mm right-angle
Secondary mirror obstruction (dia.; %) . . . 3.3cm (1.32”); 9.4%
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine
Setting circle diameters . . . . . . . . . . . . . Dec.: 3.81”; R.A.: 7.8”
Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC
Motor Drive System . . . DC servo motors with encoders, both axes48

Bearings:
Altitude . . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings
Azimuth . . . . PTFE thrust bearing and radial ball bearing
Materials:
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum
Mounting . . . . . . ABS, with internal aluminum structurePrimary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A

Telescope dimensions:. . . . . . . . . . . . . 43cm x 25cm x 20cm (17” x 10” x 8”)
Telescope net weight:(incl. Autostar & batteries) . . . . . . . . . . . 6.1kg (13.5 lbs)
Telescope shipping weight. . . . . . . . . . . . . . . . 8.3kg (18.4 lbs)
Battery Life (approx.):with Autostar. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs

Specifications: ETX-125AT Astro Telescope
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain
Primary mirror diameter . . . . . . . . . . . . . . . . . . 138mm (5.43”)
Clear aperture . . . . . . . . . . . . . . . . . . . . . . . . . . . 127mm (5.0”)
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . 1900mm (74.8”)
Focal ratio (photographic speed) . . . . . . . . . . . . . . . . . . . . f/15
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . . . 4.6m (15 ft)
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 0.9 arc secs
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 12.5
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 0.76°/inch
Maximum practical visual power . . . . . . . . . . . . . . . . . . . 500X
Optical tube dimensions(dia. x length) . . . . . . . . . . 14.6cm x 36cm (5.75” x 14.2”)
Viewfinder . . . . . . . . . . . . . . . . . . . . . . . . 8 x 25mm right-angle
Secondary mirror obstruction (dia.; %) . . 39.4mm (1.6”); 9.6%
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine
Setting circle diameters . . . . . . . . . . . . . . . Dec.: 4.3”; R.A.: 9”Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC
Motor Drive System . . . DC servo motors with encoders, both axes
Bearings:
Altitude . . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings
Azimuth . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings
Materials:
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum
Mounting . . . . . . . ABS, with internal aluminum structurePrimary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A

Telescope dimensions:. . . . . . . . . . 48cm x 23cm x 27cm (19” x 8.9” x 10.8”)
Telescope net weight:(incl. Autostar & batteries) . . . . . . . . . . . 6.9kg (15.2 lbs)
Telescope shipping weight. . . . . . . . . . . . . . . 11.4kg (25.2 lbs)
Battery Life (approx.):with Autostar. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs

49

Autostar Specifications
Processor ............................................................................68HC11, 8MHz
Flash Memory ............................................................1MB, reloadable
Keypad ........................................................................20 key alphanumeric
Display ........................................................................2 line, 16 character LCD
Backlight......................................................................Red LED
Utility Light ..................................................................Yes
RS-232 ........................................................................Yes
Coil Cord ....................................................................24"
Database ....................................................................30,223 objects
Autostar Dimensions
Length ........................................................................6.56" (16.6cm)
Width (LCD end) ........................................................3.19" (80cm)
Width (Connector end) ................................................2.25" (57cm)
Depth ..........................................................................0.81" (21cm)
Autostar net weight ....................................................1.12 lbs (0.51kg)

50

APPENDIX A: EQUATORIAL(POLAR) ALIGNMENT
Equatorial Alignment
In equatorial (or "polar") Alignment, the telescope is oriented so that the horizontal andvertical axes of the telescope are lined up with the celestial coordinate system.

Important Note:
The "Telescope: Mount"option of the Setup menu is
set to "Alt/Az" as the default
mount by the factory. If thetelescope is equatoriallymounted, you must choosethe "Polar" option from theAutostar "Telescope: Mount"menu.

In order to equatorial align your telescope, it is essential to have an understanding of how
and where to locate celestial objects as they move across the sky. This section provides abasic introduction to the terminology of equatorial-aligned astronomy and includes
instructions for finding the celestial pole and for finding objects in the night sky using
Declination and Right Ascension.

Celestial Coordinates
A celestial coordinate system was created that maps an imaginary spheresurrounding the Earth upon which all stars appear to be placed. This mapping system issimilar to the system of latitude and longitude on Earth surface maps.
In mapping the surface of the Earth, lines of longitude are drawn between the North andSouth Poles and lines of latitude are drawn in an East-West direction, parallel to the Earth’s
equator. Similarly, imaginary lines have been drawn to form a latitude and longitude grid forthe celestial sphere. These lines are known as Right Ascension and Declination.
The celestial map also contains two poles and an equator just like a map of the Earth. The
poles of this coordinate system are defined as those two points where the Earth’s North andSouth poles (i.e., the Earth's axis), if extended to infinity, would cross the celestial sphere.
Thus, the North Celestial Pole (1, Fig. 42) is that point in the sky where an extension of theNorth Pole intersects the celestial sphere. The North Star, Polaris, is located very near the
North Celestial Pole (1, Fig. 42). The celestial equator (2, Fig. 42) is a projection of the
Earth’s equator onto the celestial sphere.

North
Celestial
Pole(Vicinityof Polaris)

Star

16

15

14

13 12

11

ation
clin
De

1
17
18
19

So just as an object's position on the Earth’s surface can be located by its latitude andlongitude, celestial objects may also be located using Right Ascension and Declination. For
example: You could locate Los Angeles, California, by its latitude (+34°) and longitude(118°). Similarly, you could locate the Ring Nebula (M57) by its Right Ascension (18hr) and
its Declination (+33°).

+90 Dec.

10

9Earth’s
Rotation

20 21

22

23

0

1

2

Right Ascension

3

8
4

■
7
6
5

Celestial
Equator
0 Dec.

2South
Celestial
Pole-90 Dec.

■
Fig. 42: Celestial Sphere.

Right Ascension (R.A.): This celestial version of longitude is measured in units ofhours (hr), minutes (min) and seconds (sec) on a 24-hour "clock" (similar to how
Earth's time zones are determined by longitude lines). The "zero" line was arbitrarily
chosen to pass through the constellation Pegasus, a sort of cosmic Greenwich meridian. R.A. coordinates range from 0hr 0min 0sec to 23hr 59min 59sec. There are 24
primary lines of R.A., located at 15-degree intervals along the celestial equator.
Objects located further and further East of the zero R.A. grid line (0hr 0min 0sec) carryhigher R.A. coordinates.
Declination (Dec.): This celestial version of latitude is measured in degrees,arc-minutes and arc-seconds (e.g., 15° 27' 33"). Dec. locations North of the celestial
equator are indicated with a plus (+) sign (e.g., the Dec. of the North celestial pole is+90°). Dec. locations South of the celestial equator are indicated with a minus (–) sign
(e.g., the Dec. of the South celestial pole is –90°). Any point on the celestial equator(such as the the constellations of Orion, Virgo and Aquarius) is said to have a
Declination of zero, shown as 0° 0' 0."

Polar Mounting your Telescope with the #884 Deluxe Field Tripod
As the Earth rotates on its axis, astronomical objects appear to move across the sky in anarc. This apparent motion is not obvious to the unaided eye, but when viewed through atelescope such as an ETX, this motion is rapid indeed. If the motor drive has not been
engaged,celestial
objects
viewedinthetelescope
eyepiecedrift
entirely out of the field of view in 15 to 60 seconds, depending on the magnification
employed.
However, by mounting your telescope and turning on the motor drive, you cancounteract the drift of objects in the eyepiece. The two basic types of mounting are:altazimuth (alt/az) and equatorial. For many ETX owners, it will not be necessary toequatorially mount the telescope; alt/az mounting will suffice. The Autostar Controller allows
the telescope to be mounted in the altazimuth (alt/az) mode for mostobserving purposes. See EASY (TWO-STAR) ALIGN, page 19, for more information.

51

However, owners who wish to perform astrophotography or use the Meade LPI (seePHOTOGRAPHY WITH MEADE’S AUTOSTAR SUITE, page 42, for more information) will findequatorial mounting indispensible to their needs.

2Equatorial Mount
Equatorial mounting lines up the telescope’s polar axis with the North Celestial Pole (or theSouth Celestial Pole if observing in the southern hemisphere).
When using an equatorially mounted telescope, tracking (following) celestial objects ispossible by turning on your ETX telescope's motor drive. The motor counteracts the Earth's
rotation and keeps objects in the field of view of the eyepiece for hands-off tracking.

A
Fig. 43: Loosen control latch.
High latitude
leg mounting
hole.
Attachment
knob.

Latitudecontrolbar.

Fig. 44: High latitude leg
mounting hole andcorresponding attachment
knob.

C

Fig. 45: Attach telescope totripod.

Equatorial Mounting Procedure
1. Assemble the tripod as described in Step #2 of How to Assemble Your Telescope andTripod, page 12.
2. Loosen the latitude control latch (1, Fig. 43) and lift up the tilt-plate (2, Fig. 43) so thatyou can easily access the underside of the plate. Relock the latitudecontrol latch, so the assembly doesn't slip while you are attaching the telescope.
3. Turn the tripod, so that the face of the tilt-plate points North (Figs. 47 and 48). If you
attach the telescope to the tripod indoors, be sure to orient the face of the tilt-plate topoint North after moving the telescope outdoors. Equivalently, point the tripod leg (5,Fig. 47) North. This is the leg opposite from the latitude control bar (4, Fig. 47).
4. Line up the mounting hole on the base of the telescope labeled "High Latitude Leg"with the attachment knob that is closest to the latitude control bar (see Fig. 44). Lineup the other mounting hole with the remaining attachment knob. Thread both
attachment knobs into the base of the telescope. Tighten to a firm-feel only.
5. Determine the latitude of your observing location from a road map, atlas or the
LATITUDE CHART FOR MAJOR CITIES OF THE WORLD, page 55. Loosen thelatitude control latch (1, Fig. 46) and adjust the latitude control bar (4, Fig. 46) so thatyour observing site's latitude is just visible above the flat surface of the tripod head.
Retighten the latch.
6. If you have not already done so orient the tripod leg (see Step #3 and 5, Fig. 47) sothat it is pointing due North (if the location of Polaris, the North Star, is known, point
the telescope directly at Polaris. Observers located in the Earth’s Southern
Hemisphere must point the telescope due South).
7. The telescope is now equatorially mounted; the tripod must not be moved or else thealignment will be lost. Instead, use one of the following methods to move thetelescope's optical tube to a desired celestial object.
(a) Loosen the vertical and/or horizontal locks (6 and 9, Fig. 1) to permit the opticaltube to be freely moved manually. Tighten the locks once you center on theobject.
(b) With the horizontal and vertical locks in their “locked” positions, use the Arrowkeys to move the optical tube.
Note: For most astronomical observing requirements, approximate
settings of the telescope's latitude and North-pointing tripod leg (Steps #5
and #6) are acceptable. Do not allow undue attention to precise equatorial
mounting of the telescope to interfere with your enjoyment of the instrument.
Using an Equatorially Mounted Telescope
Once your telescope is equatorially mounted, the telescope motor drive will keep acelestial object in the telescope eyepiece's field of view.
To Track a Star When Polar Mounted:
Make sure you have initialized your telescope before you try out this feature (seeINITIALIZING AUTOSTAR, page 18).
1. Tighten the vertical and horizontal locks (6 and 9, Fig. 1) if necessary.
2. Make sure that Autostar is connected to the HBX port (C, Fig. 2) of thetelescope’s computer control panel.
3. Flip the telescope power switch (A, Fig. 2) to the ON position.
The Autostar screen displays a copyright message displays, followed by a short beep.
Then Autostar takes a few moments to start up the system.
4. A message displays that warns not to look at the Sun. At the end of this message,press the key prompted by Autostar to signify that the message has been read andunderstood.

52

D
A
Fig. 46: Set latitude.

+

North
Celestial
Pole

D

E
Fig. 47: Example of Polar
Alignment. Note that the faceof the tilt-plate points North.

+

North
CelestialPole

5. Press ENTER repeatedly until “Setup: Align” displays.
6. Press the Scroll Down key repeatedly until "Setup: Telescope" displays. Press
ENTER. “Telescope: Telescope Model” displays.
7. Press the Scroll Down key repeatedly until "Telescope: Mount" displays. Press
ENTER. “Scope Mounting: Alt/az” displays.
8. Press the Scroll Down key once. "Scope Mounting: Alt/az" displays. Press ENTER.
"Telescope: Mount" displays again.
9. Press Mode once. “Setup: Telescope” displays.
10. Press the Scroll Down key once. "Setup: Targets" displays.
11. Press ENTER. "Targets: Terrestrial" displays. Press one of the Scroll keys once.
"Targets: Astronomical" now displays.
12. Use the Arrow keys to locate a bright star in the night sky. Use the viewfinder (2, Fig.
1) to help line up on the star. You may choose any unobstructed, bright star for the
purposes of this example. Use Autostar's Arrow keys to center the star in theeyepiece. Once the star is centered, press ENTER to select "Astronomical." Thetelescope's tracking motors then engage. It may take the tracking motors several
seconds to begin tracking. When they do, it may be necessary to once again center
the star in the eyepiece. The tracking motors will then keep the star you have chosen
in the center of the eyepiece.
13. Press and hold the ENTER key for a few seconds and then release to stop
tracking. You may repeat the procedure to locate another star or object using theArrow keys. Then press ENTER to re-engage the tracking motors.
Caution: Do not move the tripod or adjust the latitude setting whileobserving or the mounting alignment will be lost. The telescope's motor drive disengages when the Horizontal and the Vertical lock levers are unlocked andre-engages when the levers are relocked.
Autostar Polar Alignment
Autostar provides three different (manual) methods for polar alignment: Easy,
One-Star and Two-Star.
Easy Polar Alignment
Two alignment stars are chosen by Autostar based on the date, time and location. First,
choose "Polar" from the "Setup: Telescope: Mount" menu. The rest of theprocedure is identical to the Alt/Az EASY (TWO-STAR) ALIGN, page 19.
One-Star Polar Alignment
Polar One-Star Alignment requires some knowledge of the night sky. Autostar
provides a database of bright stars and one star from this database is chosen by theobserver for alignment. Polaris is chosen by Autostar. First, choose "Polar" from the "Setup:
Telescope: Mount" menu. The rest of the procedure is almost identical to the Alt/Az ONE
STAR ALT/AZ ALIGNMENT, page 38, except that Autostar prompts you to point thetelescope at Polaris and center it in the telescope eyepiece.

Fig. 48: Example of Polar
Alignment. Note that the faceof the tilt-plate points North.
This is the Polar home
position.
Important Note:
In order to select any ofthree polar alignment
options, you must first
select "Polar" in the"Mount" option of the"Setup: Telescope" menu.

Two-Star Polar Alignment
Polar Two-Star Alignment requires some knowledge of the night sky. Autostar provides a
database of bright stars and two stars from this database are chosen by the observer foralignment. First, choose "Polar" from the "Setup: Telescope: Mount" menu. The rest of theprocedure is almost identical to the Alt/Az TWO STAR ALT/AZ ALIGNMENT, page 39.
Locating the Celestial Pole
To get basic bearings at an observing location, take note of where the Sun rises (East) andsets (West) each day. After the site is dark, face North by pointing your left shoulder toward
where the Sun sets. To precisely point at the pole, find the North Star (Polaris) by using the
Big Dipper as a guide (Fig. 49).
Important Note: For almost all astronomical observing requirements,
approximate settings of the telescope’s latitude and Polar axis are
acceptable. Do not allow undue attention to precise Polar Alignment of thetelescope to interfere with your basic enjoyment of the instrument.

53

Little Dipper

Setting Circles
The ETX models are equipped with R.A. and Dec. setting circles (13 and 16, Fig. 1) to aid
in locating faint celestial objects when the telescope has been polar aligned. Setting circles
emulate the celestial coordinates found on star charts or in sky catalogs. Any charted object
is easily located by coordinates in R.A. (in hours, minutes and seconds, from 0h 0m 0s to
23h 59m 59s) and Dec. (in degrees from 0° to ±90°).

PolarisBig Dipper

Cassiopeia

With an ETX model polar aligned, use the Arrow keys to move the telescope in R.A. (leftand right keys) and Dec. (up and down keys).
Note: The Dec. setting circle is located on the left arm of the telescope fork
mount. The right arm of the mount contains a graduated circle (mounted behind
the knurled knob of the vertical lock), without Dec. numbers.

Fig. 49: Locating Polaris• Declination Setting Circle: The Dec. setting circle (Fig. 50) has been factory set to readthe correct Declination of celestial objects.
Because the smooth knob on this fork mount arm need never be loosened, the Dec.
setting circle should always remain calibrated. If for some reason this knob becomesloose and the Dec. setting circle must be recalibrated, level the optical tube (5, Fig. 1)
so that it is parallel to the drive base. Loosen the smooth knob covering the Dec. setting
circle until the setting circle moves freely. Reposition the setting circle so that the 0setting aligns with the Dec. pointer (the molded triangle beneath the setting circle).
Retighten the Dec. knob.

40

30

40

20

10

0

10

20

30

Fig. 50: Section of
Declination setting circle.

12
12

11
13

10
14

Fig. 51: Section of Right
Ascension setting circle.

• Right Ascension Setting Circle: Since celestial objects move in R.A., the R.A. setting
circle (Fig. 51) must be reset as each object is located during an observing session. The
R.A. pointer is located on the drive base 90° counterclockwise from the telescope’s
Computer Control panel (10, Fig. 1) immediately under the R.A. circle.
To use the setting circles to find astronomical objects, the ETX must first be polar aligned.
It is advisable that the motor drive be turned on and that a low-power eyepiece (e.g., a
26mm eyepiece) be employed. Then use the following procedure:
1. Identify the celestial coordinates (R.A. and Dec.) of a bright, easy-to-find object, such asa bright star. (Avoid using Polaris or any object near Polaris.) Coordinates of bright stars
are listed in astronomy magazines, text books or star charts. Center this object in thetelescope’s field of view.
2. Manually turn the R.A. circle (13, Fig. 1) to read the R.A. of the object at the R.A.
pointer (the molded triangle beneath this setting circle).
3. The R.A. circle is now calibrated to read the correct R.A. of any object at which thetelescope is pointed. The Dec. circle is already calibrated through polar alignment.
4. To find another object, again identify the R.A. and Dec. coordinates. Then, without
touching the setting circles, move the telescope (manually, by unlocking the vertical andhorizontal locks or by slewing the telescope using the Arrow keys) so that the R.A. andDec. pointers read the coordinates of the second object.
5. If the above procedure has been followed carefully, the second object will now be in thetelescope’s field of view.
Note: Since the second object (i.e., the object to be located) is in constantmotion, once the R.A. circle is calibrated (step 2, above) the telescope should
be moved rapidly to read the coordinates of the second object. Otherwise thesecond object will no longer be in the position indicated by the R.A. circle.
Using setting circles requires a developed technique. When using the circles for the firsttime, try hopping from one bright star (the calibration star) to another bright star of known
coordinates. Practice moving the telescope from one easy-to-find object to another. In thisway the precision required for accurate object location becomes familiar.

54

APPENDIX B: LATITUDE CHART
Latitude Chart for Major Cities of the WorldTo aid in the polar alignment procedure (see page 52), latitudes of major cities around the world are listed below. To determine the latitude ofan observing site not listed on the chart, locate the city closest to your site. Then follow the procedure below:
Northern hemisphere observers (N): If the site is over 70 miles (110 km) North of the listed city, add one degree for every 70 miles. If thesite is over 70 miles South of the listed city, subtract one degree per 70 miles.
Southern Hemisphere observers (S): If the site is over 70 miles (110 km) North of the listed city, subtract one degree for every 70 miles. If
the site is over 70 miles South of the listed city, add one degree per 70 miles.
NORTH AMERICA

SOUTH AMERICA

City

State/Prov./Country Latitude

City

Country

LatitudeAlbuquerqueAnchorage
Atlanta
BostonCalgary
ChicagoCleveland
DallasDenverDetroitHonolulu
JacksonKansas City
KenoshaLas Vegas
Little RockLos Angeles
Mexico City
Miami
Minneapolis
Nashville
New Orleans
New York
Oklahoma City
OttawaPhiladelphia
Phoenix
PortlandSalt Lake CitySan Antonio
San Diego
San Francisco
SeattleWashington
EUROPE

New Mexico
AlaskaGeorgia
Massachusetts
Alberta
Illinois
Ohio
Texas
Colorado
Michigan
Hawaii
Mississippi
Missouri
Wisconsin
NevadaArkansas
California
MexicoFloridaMinnesota
Tennessee
Louisiana
New York
Oklahoma
Ontario
Pennsylvania
Arizona
OregonUtah
Texas
California
California
Washington
District of Columbia

35° N
61° N
34° N
42° N
51° N
42° N
41° N
33° N
40° N
42° N
21° N
32° N
39° N
45° N
36° N
35° N
34° N
19° N
26° N
45° N
36° N
30° N
41° N
35° N
45° N
40° N
33° N
46° N
41° N
29° N
33° N
38° N
47° N
39° N

Bogotá
São Paulo
Buenos Aires
Montevideo
Santiago
CaracasASIA

Colombia
BrazilArgentina
Uruguay
Chile
Venezuela

4° N
23° S
35° S
35° S
34° S
10° N

City

Country

LatitudeAmsterdam
AthensBern
Copenhagen
DublinFrankfurt
Glasgow
Helsinki
LisbonLondonMadrid
Oslo
Paris
Rome
Stockholm
ViennaWarsaw

Netherlands
GreeceSwitzerland
Denmark
IrelandGermany
ScotlandFinland
Portugal
EnglandSpain
NorwayFrance
Italy
SwedenAustria
Poland

52° N
38° N
47° N
56° N
53° N
50° N
56° N
60° N
39° N
51° N
40° N
60° N
49° N
42° N
59° N
48° N
52° N

City

Country

LatitudeBeijingHong Kong
Seoul
TaipeiTokyo
SapporoBombayCalcutta
Hanoi
Jedda
AFRICA

China
China
South Korea
Taiwan
Japan
Japan
India
India
Vietnam
Saudi Arabia

40° N
23° N
37° N
25° N
36° N
43° N
19° N
22° N
21° N
21° N

City

Country

Cairo
Egypt
Cape Town
South Africa
Rabat
Morocco
Tunis
Tunisia
Windhoek
Namibia
AUSTRALIA AND OCEANIA

Latitude
30° N
34° S
34° N
37° N
23° S

City

State/Country

Latitude

Adelaide
Brisbane
Canberra
Alice Springs
HobartPerthSydneyMelbourne
AucklandSouth Australia
Queensland
New South Wales
Northern Territory
Tasmania
Western Australia
New South Wales
Victoria
New Zealand

35° S
27° S
35° S
24° S
43° S
32° S
34° S
38° S
37° S

55

APPENDIX C: TRAINING THE DRIVE
Train the telescope motors using Autostar. Perform this procedure if you are experiencing any pointing accuracy problems. Fig.
52 depicts the complete Drive Training procedure.
Note: Use a terrestrial object, such as a telephone pole or lamp post, to train the drive. Complete this exercise once

every 3 to 6 months to maintain the highest level of telescope pointing accuracy.

ETX TIPS
1

2

Verify that AUTOSTARINITIALIZATION iscomplete.
Press MODE until
Select Item is displayed.

Select Item
Object12

Scope slews left.
Bring target backto center using
ENTER the Right Arrow key.

3

Press the scroll
up key once.

Select Item
Setup

Further Study....

Press > until it
is centered4

Press < until it
is centered

13

Scope slews right.
Bring target backto center using
ENTER the Left Arrow key.

Access the Setup

ENTER menu.

Setup
Align

Train Drive
Az. Train

14

Menu returns to
Az. training.

5
Multiple presses.

Train Drive
Alt. Train
Setup
Telescope

15

Altitude

6

ENTER (vertical)
training.

Access the
ENTER Telescope menu.

Telescope
7
1
Telescope Model

Drive Setup
For this op. . .

16

Reminder to
ENTER use terrestrial
target.

Multiple presses.

Center reference
17
objectTelescope
Train Drive

8

Center target

ENTER using Arrowkeys.

Choose the Train

Train Drive
Az. Train

9

AzimuthENTER (horizontal)
training.

Press until it
is centered>

ENTER Drive option.

Scope slews down.
Bring target backto center using
ENTER the Up Arrow key.

Press until it
is centered>

Drive Setup
For this op. . .

10Reminder to
ENTER use terrestrial
target.

Center reference
11
object.
ENTER

Center target
using Arrow
keys.

56

19

Scope slews up.
Bring target backto center using
ENTER the Down Arrow key.

Train Drive
Az. Train
MODE

Also included below is a small sampling of books, magazinesand organizations that you might find helpful.
Topics1.
2.

How is a star born? How does a solar system form?
How is the distance to a star measured? What is a lightyear? What is red shift and blue shift?
3. How are the craters on our Moon formed? Is there water
under the surface of the Moon?
4. What is a black hole? A neutron star? A quark star? A
gamma burster? An Einstein lens?
5. What are stars made of? Why are stars different colors?
How is the elemental composition of a star determined?
What is an Lyman Alpha forest?
6. What is the difference between a Type 1 and a Type IIsupernova?
7. What is the importance of studying the composition ofcomets? Where do comets come from?
8. How old is our Sun? Will our Sun evolve into a planetarynebula or go supernova?
9. What is the Inflationary Big Bang? What is dark matter?
What are MACHO's?
10. How are extrasolar planets discovered? What is an accretion (or protoplanetary) disk?
11. What are the differences between elliptical, spiral and irregular galaxies? Can globular clusters be older than the universe itself?
Books
1.

The Guide to Amateur Astronomy by Jack Newton andPhilip Teece

2.

The Sky: A User’s Guide by David Levy

3.

Turn Left at Orion by Guy Consolmagno & Dan Davis

4.

Astrophotography for the Amateur by Michael Covington

Magazines
1.
2.

Sky & TelescopeBox 9111, Belmont, MA 02178
Astronomy
Box 1612, Waukesha, WI 53187

Organizations:
20

1.

Multiple presses.

2.
Select Item
ObjectFig. 52: Training the Drive Procedure.

18

This manual gives only the briefest introduction to astronomy. If
you are interested in pursuing further studies in astronomy, a
few topics are suggested below that are worth reading up on(some of the topics are easy and some are quite challenging).
Try looking up some of these in the Autostar glossary.

21

3.

Astronomical League
Executive Secretary
5675 Real del Norte, Las Cruces, NM 88012
The Astronomical Society of the Pacific
390 Ashton Ave., San Francisco, CA 94112
The Planetary Society
65 North Catalina Ave, Pasadena, CA 91106

And watch Jack Horkheimer, Star Gazer, on your local PBS
station. Visit Jack’s website at: www.jackstargazer.com

APPENDIX D:BASIC
ASTRONOMY
In the early 17th century Italian Scientist Galileo, using a telescope smaller than your
ETX, turned it skyward instead of looking at the distant trees and mountains. What hesaw and what he realized about what he saw, has forever changed the way mankind
thinks about the universe. Imagine what it must have been like being the first humanto see moons revolve around the planet Jupiter or to see the changing phases ofVenus! Because of his observations, Galileo correctly realized Earth's movement andposition around the Sun and in doing so, gave birth to modern astronomy. Yet
Galileo's telescope was so crude, he could not clearly make out the rings of Saturn.
Galileo's discoveries laid the foundation for understanding the motion and nature of
the planets, stars and galaxies. Building on his foundation, Henrietta Leavitt
determined how to measure the distance to stars, Edwin Hubble gave us a glimpse
into the possible origin of the universe, Albert Einstein unraveled the crucial
relationship of time and light and 21st-century astronomers are currently discovering
planets around stars outside our solar system. Almost daily, using sophisticatedsuccessors to Galileo's telescope, such as the Hubble Space Telescope and the
Chandra X-Ray Telescope, more and more mysteries of the universe are being
probed and understood. We are living in the golden age of astronomy.
Unlike other sciences, astronomy welcomes contributions from amateurs. Much of theknowledge we have on subjects such as comets, meteor showers, double andvariable stars, the Moon and our solar system comes from observations made byamateur astronomers. So as you look through your Meade ETX telescope, keep inmind Galileo. To him, a telescope was not merely a machine made of glass and metal,
but something far more—a window of incredible discovery.
Autostar Glossary
Be sure to make use of Autostar’s Glossary feature. The Glossary menu provides analphabetical listing of definitions and descriptions of common astronomical terms.
Access directly through the Glossary menu or through hypertext words embedded in
Autostar. See GLOSSARY MENU, page 26, for more information.

Fig. 53: The Moon. Notethe deep shadows in thecraters.

The Moon
The Moon is, on average, a distance of 239,000 miles (380,000km) from Earth and isbest observed during its crescent or half phase when Sunlight strikes the Moon’s
surface at an angle. It casts shadows and adds a sense of depth to the view (Fig. 53).
No shadows are seen during a full Moon, causing the overly bright Moon to appear
flat and rather uninteresting through the telescope. Be sure to use a neutral Moon
filter when observing the Moon. Not only does it protect your eyes from the bright glareof the Moon, but it also helps enhance contrast, providing a more dramatic image.
Using your ETX model, brilliant detail can be observed on the Moon, including
hundreds of lunar craters and maria, described below.
Craters are round meteor impact sites covering most of the Moon’s surface. With noatmosphere on the Moon, no weather conditions exist, so the only erosive force ismeteor strikes. Under these conditions, lunar craters can last for millions of years.
Maria (plural for mare, seas) are smooth, dark areas scattered across the lunar
surface. These areas are ancient impact basins that were filled with lava from theinterior of the Moon by the depth and force of the meteor or comet impact.
12 Apollo astronauts left their bootprints on the Moon in the late 1960’s and early
1970’s. However, no telescope on Earth can see these footprints or any otherartifacts. In fact, the smallest lunar features that may be seen with the largest
telescope on Earth are about one-half mile across.
Note: Except during its early or late crescent phases, the Moon can be an
exceptionally bright object to view through the telescope. To reduce thebrightness and glare, use the #905 Variable Polarizing Filter (see the MEADE
GENERAL CATALOG for more information).

57

Tip:
Enter a date in the Datemenu and you candetermine if a planet(s)—or any other object in the
database—will be visible
during the night of theentered date.
After entering a new date,go to the Object menu
and select the desired
planet from the menu.
Then keep pressing oneof the Scroll keys until therise and set times display.
Press MODE to exit.

Fig. 54: The planet Jupiter.
Jupiter's four largest
moons can be observed ina different position every
night.

Planets
Planets change positions in the sky as they orbit around the Sun. To locate theplanets on a given day or month, consult a monthly astronomy magazine, such as Sky
and Telescope or Astronomy. Listed below are the best planets for viewing throughyour ETX model telescope.
Venus is about nine-tenths the diameter of Earth. As Venus orbits the Sun, observers
can see it go through phases (crescent, half and full) much like those of the Moon.
The disk of Venus appears white, as sunlight is reflected off the thick cloud cover thatcompletely obscures any surface detail.
Mars is about half the diameter of Earth. Through the telescope it appears as a tiny
reddish-orange disk. You may see a hint of white at one of the planet’s polar ice caps.
Approximately every two years, when Mars is closest to Earth, additional detail andcoloring on the planet's surface may be visible.
Jupiter (Fig. 54) is the largest planet in our solar system, with a diameter 11 times
that of Earth. Jupiter appears as a disk with dark lines stretching across the surface.
These lines are cloud bands in the atmosphere. Four of Jupiter’s 29 (and still
counting!) moons (Io, Europa, Ganymede and Callisto) can be seen as star-like pointsof light when you use even the lowest magnification. The number of moons
visible on any given night changes as they circle around the giant planet.
Saturn (Fig. 55) is nine times the diameter of Earth and appears as a small, rounddisk with rings extending out from either side. In 1610, Galileo, the first person toobserve Saturn through a telescope, did not understand that what he was seeing wererings. Instead, he believed that Saturn had “ears.” Saturn’s rings are composed ofbillions of ice particles. The major division in Saturn's rings, called the Cassini
Division, is generally visible through all three ETX models. Titan, the largest of
Saturn’s moons, can also be seen as a bright, star-like object near the planet.
Deep-Sky Objects
You can use star charts to locate constellations, individual stars and deep-sky objects.
Examples of various deep-sky objects are given below:
Stars are large gaseous objects that are illuminated by nuclear fusion in their core.
Because of their vast distances from our solar system, all stars appear as pinpoints oflight, regardless of the size of the telescope used.
Nebulae are vast interstellar clouds of gas and dust where stars are formed. Most
impressive of these is the Great Nebula in Orion (M42), a diffuse nebula that appears
as a faint wispy gray cloud. M42 is 1600 light years from Earth.

Fig. 55: Saturn has themost extensive ring structure in our Solar System.

Fig. 56: The Pleiades is
one of the most beautiful
open clusters.

58

Open Clusters are loose groupings of young stars, all recently formed from the same
diffuse nebula. The Pleiades (Fig. 56) is an open cluster 410 light years from Earth.
Several hundred stars of the cluster are visible through your telescope.
Constellations are large, imaginary patterns of stars believed by ancient civilizations
to be the celestial equivalent of objects, animals, people or gods. These patterns are
too large to be seen through a telescope. To learn the constellations, start with aneasy grouping of stars, such as the Big Dipper in Ursa Major. Then use a star chart to
explore across the sky.
Galaxies are large assemblies of stars, nebulae and star clusters that are bound by
gravity. The most common shape is spiral (such as our own Milky Way), but galaxies
can also be elliptical or even irregular blobs. The Andromeda Galaxy (M31) is the closest spiral-type galaxy to our own. This galaxy appears fuzzy and cigar-shaped. It is
2.2 million light years away in the constellation Andromeda.

MEADE LIMITED WARRANTY
Every Meade telescope, spotting scope and telescope accessory is warranted by Meade Instruments Corporation (“Meade”)
to be free of defects in materials and workmanship for a period of ONE YEAR from the date of original purchase in the U.S.A.
and Canada. Meade will repair or replace a product or part thereof, found by Meade to be defective, provided the defective
part is returned to Meade, freight-prepaid, with proof of purchase. This warranty applies to the original purchaser only and is
non-transferable. Meade products purchased outside North America are not included in this warranty, but are covered under
separate warranties issued by Meade international distributors.
RGA Number Required: Prior to the return of any product or part, a Return Goods Authorization (RGA) number must be
obtained from Meade by writing or calling (949) 451-1450. Each returned part or product must include a written statement
detailing the nature of the claimed defect, as well as the owner’s name, address and phone number.
This warranty is not valid in cases where the product has been abused or mishandled, where unauthorized repairs have been
attempted or performed or where depreciation of the product is due to normal wear-and-tear. Meade specifically disclaims
special, indirect or consequential damages or lost profit which may result from a breach of this warranty. Any implied warranties
which cannot be disclaimed are hereby limited to a term of one year from the date of original retail purchase.
This warranty gives you specific rights. You may have other rights which vary from state to state.
Meade reserves the right to change product specifications or to discontinue products without notice.

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