HDTenEightyP/NetNews huggingface dataset:
From: yee@trident.arc.nasa.gov (Peter E. Yee)
Newsgroups: sci.space.news
Subject: Shuttle Status for 04/15/92 (Forwarded)
Date: 15 Apr 92 20:23:57 GMT
Followup-To: sci.space
Organization: NASA Ames Research Center, Moffett Field, CA
Apparently-To: sci-space-news@ames.arc.nasa.gov


        This KSC Status Report was prepared at 11 a.m., Wednesday, April 15.

             At Pad 39-B, the installation of the Intelsat booster and ASEM
        Tuesday evening.  All of the electrical connections with the orbiter
        had been completely established by 10:55 p.m.  At 10 a.m. this
        morning the Interface Verifcation Test, or IVT, began which verifies
        those connections, and the test is forecast to be finished about 4
        p.m. today.

             The STS-49 astronauts arrived last night from Houston by T-38
        jets at 11:10 p.m.  They are scheduled to conduct a payload
        inspection at 1 o'clock on Thursday afternoon.

             Over the next two days, the crew will have emergency egress
        training at the launch pad, and have fit checks of their helmets,
        gloves and launch and entry suits.  The crew will be aboard Endeavour
        for the last three hours of the countdown dress rehearsal on Friday
        as is customary, and will interface with the launch team located in
        Firing Room 1.  The clock will begin counting for the test at 8:30
        a.m. on Thursday.

             The main engine replacement on the Space Shuttle Endeavour which
        began Sunday is continuing and is on schedule.  The No. 2 engine was
        removed yesterday and the replacement is undergoing installation
        today.  The last engine will be removed tomorrow with the replacment
        installed on Friday.

             From the NASA Kennedy Space Center, this is George Diller.
Newsgroups: sci.space.news
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Magellan Update - 04/06/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Magellan, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Wed, 8 Apr 1992 04:09:27 GMT

Forwarded from the Magellan project.

                    MAGELLAN STATUS REPORT
                        April 6, 1992

1.  Magellan continues to map Venus under  the  M2094  command
    sequence  which  started  Friday.  All systems are nominal
    and pointing accuracy of the antenna is excellent.    Only
    one star calibration was missed over the weekend.

2.  Magellan  is  sending  radar  image data using the 360 kHz
    subcarrier at 115.2.

3.  The spacecraft temperatures  are  remaining  stable,  with
    Transmsitter  B  now  at  51.2 degrees C  with a cycle depth
    of q2 degrees.

4.  Early this afternoon the spacecraft will perform a 5-orbit
    polarimetry test.  The radar mapping  parameters  for  the
    test were uplinked Friday.  While the test is in progress,
    new  radar  parameters  will  be  uplinked  to  return the
    spacecraft to normal,  left-looking radar mapping  at  the
    end of the polarimetry test about 3:40 pm tomorrow.

5.  Magellan  is  now over a third of the way through Cycle 3.
    In spite of problems with the on-board  transmitter  which
    reduced  the  playback  data  rate,  we have obtain stereo
    coverage of about 14% of the Venus surface and  may  reach
    35 to 40% by the end of Cycle 3.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     |
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Magellan Update - 04/14/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Magellan, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Wed, 15 Apr 1992 05:42:37 GMT

Forwarded from the Magellan Project

                        MAGELLAN STATUS REPORT
                           April 14, 1992

1.  Magellan continues to map Venus under the M2094 command
    sequence .  All systems are nominal, temperatures of critical
    systems are stable, and all starcals (star calibrations)
    yesterday were successful.

2.  Magellan is sending radar image data using the 360 kHz
    subcarrier at 115.2 kbps, but most science data received over
    by the 34 meter DSN (Deep Space Network) stations is not usable.

3.  Today spacecraft controllers will be sending updates to the
    Kalman gains and reference star pair in preparation for
    Thursday's uplink of the M2108 command sequence.  The new
    command sequence will go active on Friday, and will include
    gravity data collection on every eighth orbit starting April
    22nd.

4.  During last week's festivities in Washington, when Magellan
    was honored with the Goddard trophy, Dr. Steve Saunders also
    gave a science briefing for NASA Headquarters, emphasizing
    the recent results and potential studies in future cycles.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     |
From: yee@trident.arc.nasa.gov (Peter E. Yee)
Newsgroups: sci.space.news
Subject: Payload Status for 04/10/92 (Forwarded)
Date: 13 Apr 92 22:25:54 GMT
Article-I.D.: news.1992Apr13.222554.29012
Followup-To: sci.space
Organization: NASA Ames Research Center, Moffett Field, CA
Apparently-To: sci-space-news@ames.arc.nasa.gov


                              Payload Test & Activity Sheet
                                 Kennedy Space Center

                               STS-49 INTELSAT 1R /ASEM
                                    April 10, 1992

          George Diller
          407/867-2468


          UPCOMING TESTS & ACTIVITY

          Payloads arrive Pad 39-B  4/10
          Payload Installation into PCR  4/11
          Intelsat booster state of health checks  4/11-4/13
          Install payloads into Endeavour  4/14
          Interface Verification Test (IVT)  4/15
          Astronaut payload sharp edge inspection  4/15
          Intelsat booster ordnance installation  4/27
          Intelsat booster fuel tank pressurization  4/28
          Payload Closeouts  4/29-4/30
          Close orbiter payload bay doors  4/30


          TESTS & ACTIVITY COMPLETED

          Intelsat perigee solid motor arrives Astrotech  1/2
          Intelsat flight cradle arrives Astrotech  1/24
          Mate booster with flight cradle  2/5
          Intelsat booster/cradle arrives VPF  2/26
          Intelsat capture bar installation  2/26
          Intelsat booster placed in East test cell  2/27
          Intelsat booster stand-alone testing  2/28
          ASEM arrives VPF  3/5
          ASEM stand-alone verification checks  3/9
          Astronaut sharp edge inspection  3/10
          ASEM installation into East test cell  3/12
          Install payloads into transportation canister  3/26
Newsgroups: sci.space.news
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Galileo Update #2 - 04/16/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Galileo, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Fri, 17 Apr 1992 05:58:49 GMT

Forwarded from:
PUBLIC INFORMATION OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109.  TELEPHONE (818) 354-5011

                     GALILEO MISSION STATUS
                         April 16, 1992

     The Galileo spacecraft is almost 408 million kilometers
(more than 253 million miles) from Earth, and 322 million
kilometers or 201 million miles from the Sun. Its speed in orbit
is 16.26 kilometers per second, or 36,369 mph.  Round-trip
communication time is 45 minutes, 16 seconds.

     The spacecraft is operating normally, transmitting coded
telemetry at 10 bits per second.  Wednesday night it turned back
to the Sun-pointed cruise-mode attitude at the conclusion of the
sixth cooling turn, part of the program to free Galileo's stuck
high-gain antenna and permit it to be fully deployed.  Post-turn
data from the spacecraft sun-gate sensor indicated no change in
the antenna configuration.

                              #####
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | Denial is always the first
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | sympton.
|_____|/  |_|/       |_____|/                     | 

Newsgroups: sci.space.news
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Galileo Update - 04/10/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Galileo, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Sat, 11 Apr 1992 01:10:56 GMT

Forwarded from Bill O'Neil, Galileo Project Manager

                                GALILEO STATUS REPORT
                                   April 10, 1992

     The Galileo Spacecraft appears to be operating normally in the all-spin
mode and transmitting coded telemetry at 10 bps.  In accordance with Cooling
Turn No. 6 mini-sequence, we are operating in a S-Band TWTA low power mode and
have not been able to process telemetry consistently since Monday afternoon,
as expected.

     Yesterday, no Spacecraft activity was scheduled.  Tracking was scheduled
over DSS-43 (Canberra 70 meter antenna).

     Today, April 10, 1992, under stored sequence control, the S-Band TWTA
will be commanded to the high power mode to process telemetry for approximately
2 1/2 hours.

     Over the weekend, no Spacecraft activity is scheduled.  Tracking is
scheduled over DSS-43 and DSS-14 (Goldstone 70 meter antenna).
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     | 

Newsgroups: sci.space.news
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Galileo Update - 04/06/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Galileo, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Tue, 7 Apr 1992 01:51:46 GMT

Forwarded from Bill O'Neil, Galileo Project Manager

                           GALILEO STATUS REPORT
                               April 6, 1992

     The Galileo Spacecraft is operating normally in the all-spin mode and
transmitting coded telemetry at 10 bps (bits/second).

     Over the weekend, no Spacecraft activity or tracking was scheduled.

     Today, April 6, 1992, the pre-cool portion of Cooling Turn No. 6 is
scheduled to begin and will continue through April 13.   Tracking is scheduled
over DSS-43 (Canberra 70 meter antenna).

     Tomorrow, no Spacecraft activity is scheduled.  Tracking is scheduled
over DSS-43.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     |
From: oler@rho.uleth.ca (Cary Oler)
Newsgroups: sci.space.news
Subject: Daily Summary of Solar Geophysical Activity for 15 April
Date: 16 Apr 92 20:02:18 GMT
Article-I.D.: honte.oler.703454538
Followup-To: sci.space
Organization: University of Lethbridge
Apparently-To: sci-space-news@ames.arc.nasa.gov


                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                  DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY

                                15 APRIL, 1992

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 15 APRIL
---------------------------------------------------

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 106, 04/15/92
10.7 FLUX=149.3  90-AVG=193        SSN=113      BKI=3213 2212  BAI=008
BGND-XRAY=B4.7     FLU1=5.9E+05  FLU10=8.2E+03  PKI=3212 2222  PAI=009
  BOU-DEV=032,011,007,022,010,010,006,012   DEV-AVG=013 NT     SWF=00:000
 XRAY-MAX= C2.8   @ 2337UT    XRAY-MIN= B4.5   @ 0845UT   XRAY-AVG= B6.6
NEUTN-MAX= +003%  @ 1515UT   NEUTN-MIN= -003%  @ 1705UT  NEUTN-AVG= +0.1%
  PCA-MAX= +0.2DB @ 1900UT     PCA-MIN= -0.2DB @ 1935UT    PCA-AVG= +0.0DB
BOUTF-MAX=55287NT @ 0027UT   BOUTF-MIN=55233NT @ 1735UT  BOUTF-AVG=55266NT
GOES7-MAX=P:+113NT@ 1939UT   GOES7-MIN=N:-014NT@ 1015UT  G7-AVG=+079,+035,+007
GOES6-MAX=P:+127NT@ 2058UT   GOES6-MIN=E:-021NT@ 1949UT  G6-AVG=+094,+001,+023
 FLUXFCST=STD:150,155,160;SESC:152,156,159 BAI/PAI-FCST=010,010,010/010,015,015
    KFCST=2223 3322 2223 3222  27DAY-AP=006,006   27DAY-KP=2111 2221 2111 2232
 WARNINGS=
   ALERTS=
!!END-DATA!!


BRIEF SUMMARY OF EVENTS
-----------------------

     Solar activity was low.  Activity has continued fairly dormant, although
there was an indication of slightly increasing background x-ray flux late in
the UT day.  The largest event was a C2.8/SB flare from Region 7128 at 23:37
UT.

     A small filament disappeared from N31W35 early in the day.  The six
spotted regions visible at this time were dormant throughout the period.

     A single new region rotated fully into view today as Region 7134
(N02E59).

     Solar activity is expected to continue low.  There is a chance the level
of energetic activity may increase over the next 48 to 72 hours when old
Regions 7116 and 7117 are due to return.  Of these two regions, Region 7116
was the most energetic, producing three M-class events on its last rotation.
Region 7117 was responsible for numerous other C-class events.

     The geomagnetic field was quiet to unsettled.  It is expected to
continue generally unsettled to quiet over the next 72 hours.

     HF propagation conditions were normal over all regions.  No significant
changes are expected over the next 72 hours.  Near-normal propagation can be
expected over most regions during the next 3 days.


**  End of Daily Update  **
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Newsgroups: sci.space.news
Subject: Galileo Update - 04/13/92
Keywords: Galileo, JPL
Date: 14 Apr 92 05:27:42 GMT
Article-I.D.: news.1992Apr13.212910.24591
Reply-To: baalke@kelvin.jpl.nasa.gov
Followup-To: sci.space
Organization: Jet Propulsion Laboratory
News-Software: VAX/VMS VNEWS 1.3-4

Forwarded from Bill O'Neil, Galileo Project Manager

                                GALILEO STATUS REPORT
                                   April 13, 1992

     The Galileo Spacecraft appears to be operating normally in the all-spin
mode and transmitting coded telemetry at 10 bps.  On Friday, the S-band TWTA
was commanded to the high power mode and telemetry data was processed for
approximately 2-1/4 hours indicating the Spacecraft is operating normally.

     Over the weekend, no Spacecraft activity was scheduled. Tracking was
scheduled over DSS-43 (Canberra 70 meter antenna) and DSS-14 (Goldstone 70
meter antenna).

     Today, April 13, 1992, Cooling Turn No. 6 to a 165 degree off-sun attitude
is scheduled to begin at approximately 1423 PDT.  Loss of downlink carrier is
expected to occur at approximately 1522 PDT during the maneuver to the cooling
attitude.  The Spacecraft will remain at the cooling attitude for approximately
50 hours.  Tracking is scheduled over DSS-43.

     Tomorrow, no Spacecraft activity is scheduled.  Tracking is scheduled over
DSS-63 (Madrid 70 meter antenna) and DSS-43.  Coverage is required as a
precautionary measure to assure the earliest possible warning of a Spacecraft
problem since telemetry data at the cooling attitude is not expected.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     |
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Newsgroups: sci.space.news
Subject: Magellan Update - 04/10/92
Keywords: Magellan, JPL
Date: 11 Apr 92 05:53:01 GMT
Reply-To: baalke@kelvin.jpl.nasa.gov
Followup-To: sci.space
Organization: Jet Propulsion Laboratory
News-Software: VAX/VMS VNEWS 1.3-4

Fowarded from the Magellan Project.

                     MAGELLAN STATUS REPORT
                        April 10, 1992

1.  Magellan continues to map Venus under the M2094 command
    sequence including the bi-weekly psuedo tweak uplinked
    yesterday.  All systems are nominal and all starcals
    (star calibrations) yesterday were successful.

2.  Spacecraft temperatures have dropped slightly again, with
    Transmitter B now at 50 degrees C.  The Transmitter B
    performance for controlling x-band modulation continues
    to be very sensitive to temperature and temperature
    changes.

3.  A test ran yesterday by switching to 1200 bps engineering
    telemetry during orbit 4588, show that the character of
    the spurious radio system signal spur is very dependant on
    Transmitter B temperature.  An additional test is being
    performed today on orbit 4596 during which time the radio
    spectrum will be video recorded for further analysis.

4.  Science radar data acquisition continues to be marginally
    acceptable over DSN (Deep Space Network) 34 meter HEF
    (High Efficiency) stations and very poor over DSN
    34 meter standard stations.  Additional station coverage
    upgrades are being planned in coming months, with the
    addition of array passes, and a few DSN 70 meter stations
    for special tests.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | People will believe
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | anything if you whisper it.
|_____|/  |_|/       |_____|/                     | 
Newsgroups: sci.space.news
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Subject: Galileo Update - 04/15/92
Followup-To: sci.space
News-Software: VAX/VMS VNEWS 1.3-4   
Keywords:  Galileo, JPL
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
Date: Thu, 16 Apr 1992 01:46:17 GMT

Forwarded from Bill O'Neil, Galileo Project Manager

                           GALILEO STATUS REPORT
                              April 15, 1992

     The Galileo Spacecraft is at the cooling attitude and appears to be
operating normally in the all-spin mode and transmitting coded telemetry at
10 bps.

     Yesterday, no Spacecraft activity was scheduled.  Short tracking passes
were scheduled over DSS-63 (Madrid 70 meter antenna) and DSS-43 (Canberra
70 meter antenna).  Coverage is required to provide an indication of a
downlink signal in case of a Spacecraft safing action; due to geometric
conditions, there is no downlink signal while at the cooling attitude.

     Today, April 15, 1992, the Spacecraft, under stored sequence control, will
return from the cooling attitude to a 5 degree off-sun attitude; the sun
acquisition will complete at approximately 2041 PDT.  Tracking is scheduled
over DSS-43 and DSS-63.

     Tomorrow, real-time commands are scheduled to checkout the Star Scanner
(SS) and reacquire celestial reference along with collecting wobble ID data.
Tracking is scheduled over DSS-63, DSS-14 (Goldstone 70 meter antenna), and
DSS-43.
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | Denial is always the first
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | sympton.
|_____|/  |_|/       |_____|/                     | 

Newsgroups: sci.space.news
From: yee@trident.arc.nasa.gov (Peter E. Yee)
Subject: Hubble and Compton discoveries briefing set for April 8 (Forwarded)
Apparently-To: sci-space-news@ames.arc.nasa.gov
Followup-To: sci.space
Organization: NASA Ames Research Center, Moffett Field, CA
Date: Mon, 6 Apr 1992 20:14:18 GMT

Paula Cleggett-Haleim
Headquarters, Washington, D.C                  April 6, 1992
(Phone:  202/453-1547)

Randee Exler
Goddard Space Flight Center, Greenbelt, Md.
(Phone:  301/286-7277)


NOTE TO EDITORS:  N92-28

HUBBLE AND COMPTON DISCOVERIES BRIEFING SET FOR APRIL 8


     The most exotic and powerful objects in the universe will be the
subject of a media briefing on Wednesday, April 8, 1992, at 1:00 p.m.
EDT in the NASA auditorium, 400 Maryland Ave., S.W.

     New information about a potential, massive black hole in our galactic
backyard only 2.3 million light years away, will be presented by Dr.
Tod Lauer, a Hubble Space Telescope scientist.  The result is based on
analysis by Dr. Lauer of the National Optical Astronomy Observatories,
Tucson, Ariz., and the Wide Field/Planetary Camera imaging team.

     The discovery of a new class of "gamma ray quasars," which may emit
huge energies in directed beams, will be announced by Dr. Neil Gehrels,
Project Scientist for the Compton Gamma Ray Observatory, at NASA's
Goddard Space Flight Center, Greenbelt, Md.

     The significance of the new findings and their context in the
unfolding knowledge of the universe will be discussed by a panel of
distinguished astronomers, including Dr. Bruce Margon, Professor of
Astronomy and Chairman of the Department of Astronomy, University of
Washington, Seattle; Dr. Daniel Weedman, Professor of Astronomy at
Pennsylvania State University, University Park; and Dr. Steve Maran,
Senior Staff Scientist at NASA's Goddard Space Flight Center.

     This event will be carried on NASA Select Television (Satcom F-2R,
Transponder 13, 72 degrees west longitude, frequency 3960.0 MHz, audio
6.8 MHz).  Questions will be taken from reporters at Headquarters and
at NASA centers.

     An image and a 4-minute video to accompany this briefing are available
to news media by calling NASA's Broadcast and Audio Visual Branch on
202/453-8594.  The image, available in color and black and white,
depicts the compact core of galaxy M32 and the video depicts an
imaginary view from the core of galaxy M32 and a collapsing core of
galaxy M32.

	B & W: 	92-H-224
	Color: 	92-HC-191
Newsgroups: sci.space.news