# September 2006 lunar eclipse

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, September 7, 2006, with an umbral magnitude of 0.1837. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 4 hours before perigee (on September 7, 2006, at 23:00 UTC), the Moon's apparent diameter was larger.

## Visibility

The eclipse was completely visible over Asia, east Africa, eastern Europe and western Australia, seen rising over west Africa and western Europe and setting over eastern Australia and the western Pacific Ocean.
| | Hourly motion shown right to left | The Moon's hourly motion across the Earth's shadow in the constellation of Aquarius. |
| Visibility map |||

## Gallery

Degania A, Israel
* North Wales, UK
* Sofia, Bulgaria
* Jaipur, India
* Shizuoka City, Japan

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
September 7, 2006 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 1.13488 |
| Umbral Magnitude | 0.18568 |
| Gamma | −0.92619 |
| Sun Right Ascension | 11h04m47.1s |
| Sun Declination | +05°54'23.1" |
| Sun Semi-Diameter | 15'52.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 23h06m35.6s |
| Moon Declination | -06°44'25.6" |
| Moon Semi-Diameter | 16'43.3" |
| Moon Equatorial Horizontal Parallax | 1°01'22.3" |
| ΔT | 65.1 s |

## Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
Eclipse season of September 2006 :
| September 7 Ascending node (full moon) | September 22 Descending node (new moon) |
| Partial lunar eclipse Lunar Saros 118 | Annular solar eclipse Solar Saros 144 |

## Related eclipses
### Eclipses in 2006

* A penumbral lunar eclipse on March 14.
* A total solar eclipse on March 29.
* A partial lunar eclipse on September 7.
* An annular solar eclipse on September 22.

### Metonic

* Preceded by: Lunar eclipse of November 20, 2002
* Followed by: Lunar eclipse of June 26, 2010

### Tzolkinex

* Preceded by: Lunar eclipse of July 28, 1999
* Followed by: Lunar eclipse of October 18, 2013

### Half-Saros

* Preceded by: Solar eclipse of September 2, 1997
* Followed by: Solar eclipse of September 13, 2015

### Tritos

* Preceded by: Lunar eclipse of October 8, 1995
* Followed by: Lunar eclipse of August 7, 2017

### Lunar Saros 118

* Preceded by: Lunar eclipse of August 27, 1988
* Followed by: Lunar eclipse of September 18, 2024

### Inex

* Preceded by: Lunar eclipse of September 27, 1977
* Followed by: Lunar eclipse of August 19, 2035

### Triad

* Preceded by: Lunar eclipse of November 7, 1919
* Followed by: Lunar eclipse of July 8, 2093

### Lunar eclipses of 2006–2009

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
The lunar eclipses on July 7, 2009 (penumbral) and December 31, 2009 (partial) occur in the next lunar year eclipse set.
Lunar eclipse series sets from 2006 to 2009 :
| Descending node | Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node | Ascending node |
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 113 | 2006 Mar 14 | Penumbral | 1.0211 | 118 | 2006 Sep 7 | Partial | −0.9262 |
| 123 | 2007 Mar 03 | Total | 0.3175 | 128 | 2007 Aug 28 | Total | −0.2146 |
| 133 | 2008 Feb 21 | Total | −0.3992 | 138 | 2008 Aug 16 | Partial | 0.5646 |
| 143 | 2009 Feb 09 | Penumbral | −1.0640 | 148 | 2009 Aug 06 | Penumbral | 1.3572 |

### Metonic series

The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will in nearly the same location relative to the background stars.
| 2006 Mar 14.99 - penumbral (113) 2025 Mar 14.29 - total (123) 2044 Mar 13.82 - total (133) 2063 Mar 14.67- partial (143) | 2006 Sep 07.79 - partial (118) 2025 Sep 07.76 - total (128) 2044 Sep 07.47 - partial (138) 2063 Sep 07.86 - penumbral (148) |

### Saros 118

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on March 2, 1105. It contains partial eclipses from June 8, 1267 through August 12, 1375; total eclipses from August 22, 1393 through June 22, 1880; and a second set of partial eclipses from July 3, 1898 through September 18, 2024. The series ends at member 73 as a penumbral eclipse on May 7, 2403.
The longest duration of totality was produced by member 37 at 99 minutes, 22 seconds on April 7, 1754. All eclipses in this series occur at the Moon’s ascending node of orbit.
| Greatest | First | First | First | First |
| The greatest eclipse of the series occurred on 1754 Apr 07, lasting 99 minutes, 22 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series occurred on 1754 Apr 07, lasting 99 minutes, 22 seconds. | 1105 Mar 02 | 1267 Jun 08 | 1393 Aug 22 | 1465 Oct 04 |
| Last ||||
| The greatest eclipse of the series occurred on 1754 Apr 07, lasting 99 minutes, 22 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series occurred on 1754 Apr 07, lasting 99 minutes, 22 seconds. | 1826 May 21 | 1880 Jun 22 | 2024 Sep 18 | 2403 May 07 |
Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
Series members 40–61 occur between 1801 and 2200: :
| 40 | 40 | 41 | 41 | 42 | 42 |
| 1808 May 10 | 1808 May 10 | 1826 May 21 | 1826 May 21 | 1844 May 31 | 1844 May 31 |
| 43 | 43 | 44 | 44 | 45 | 45 |
| 1862 Jun 12 | 1862 Jun 12 | 1880 Jun 22 | 1880 Jun 22 | 1898 Jul 03 | 1898 Jul 03 |
| 46 | 46 | 47 | 47 | 48 | 48 |
| 1916 Jul 15 | 1916 Jul 15 | 1934 Jul 26 | 1934 Jul 26 | 1952 Aug 05 | 1952 Aug 05 |
| 49 | 49 | 50 | 50 | 51 | 51 |
| 1970 Aug 17 | 1970 Aug 17 | 1988 Aug 27 | 1988 Aug 27 | 2006 Sep 07 | 2006 Sep 07 |
| 52 | 52 | 53 | 53 | 54 | 54 |
| 2024 Sep 18 | 2024 Sep 18 | 2042 Sep 29 | 2042 Sep 29 | 2060 Oct 09 | 2060 Oct 09 |
| 55 | 55 | 56 | 56 | 57 | 57 |
| 2078 Oct 21 | 2078 Oct 21 | 2096 Oct 31 | 2096 Oct 31 | 2114 Nov 12 | 2114 Nov 12 |
| 58 | 58 | 59 | 59 | 60 | 60 |
| 2132 Nov 23 | 2132 Nov 23 | 2150 Dec 04 | 2150 Dec 04 | 2168 Dec 14 | 2168 Dec 14 |
| 61 ||
| 2186 Dec 26 ||

### Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
Series members between 1801 and 2200 :
| 1810 Mar 21 (Saros 100) | 1810 Mar 21 (Saros 100) | 1821 Feb 17 (Saros 101) | 1821 Feb 17 (Saros 101) | 1832 Jan 17 (Saros 102) | 1832 Jan 17 (Saros 102) | 1842 Dec 17 (Saros 103) | 1842 Dec 17 (Saros 103) | | |
| 1864 Oct 15 (Saros 105) | 1864 Oct 15 (Saros 105) | 1875 Sep 15 (Saros 106) | 1875 Sep 15 (Saros 106) | 1886 Aug 14 (Saros 107) | 1886 Aug 14 (Saros 107) | 1897 Jul 14 (Saros 108) | 1897 Jul 14 (Saros 108) | 1908 Jun 14 (Saros 109) | 1908 Jun 14 (Saros 109) |
| 1919 May 15 (Saros 110) | 1919 May 15 (Saros 110) | 1930 Apr 13 (Saros 111) | 1930 Apr 13 (Saros 111) | 1941 Mar 13 (Saros 112) | 1941 Mar 13 (Saros 112) | 1952 Feb 11 (Saros 113) | 1952 Feb 11 (Saros 113) | 1963 Jan 09 (Saros 114) | 1963 Jan 09 (Saros 114) |
| 1973 Dec 10 (Saros 115) | 1973 Dec 10 (Saros 115) | 1984 Nov 08 (Saros 116) | 1984 Nov 08 (Saros 116) | 1995 Oct 08 (Saros 117) | 1995 Oct 08 (Saros 117) | 2006 Sep 07 (Saros 118) | 2006 Sep 07 (Saros 118) | 2017 Aug 07 (Saros 119) | 2017 Aug 07 (Saros 119) |
| 2028 Jul 06 (Saros 120) | 2028 Jul 06 (Saros 120) | 2039 Jun 06 (Saros 121) | 2039 Jun 06 (Saros 121) | 2050 May 06 (Saros 122) | 2050 May 06 (Saros 122) | 2061 Apr 04 (Saros 123) | 2061 Apr 04 (Saros 123) | 2072 Mar 04 (Saros 124) | 2072 Mar 04 (Saros 124) |
| 2083 Feb 02 (Saros 125) | 2083 Feb 02 (Saros 125) | 2094 Jan 01 (Saros 126) | 2094 Jan 01 (Saros 126) | 2104 Dec 02 (Saros 127) | 2104 Dec 02 (Saros 127) | 2115 Nov 02 (Saros 128) | 2115 Nov 02 (Saros 128) | 2126 Oct 01 (Saros 129) | 2126 Oct 01 (Saros 129) |
| 2137 Aug 30 (Saros 130) | 2137 Aug 30 (Saros 130) | 2148 Jul 31 (Saros 131) | 2148 Jul 31 (Saros 131) | 2159 Jun 30 (Saros 132) | 2159 Jun 30 (Saros 132) | 2170 May 30 (Saros 133) | 2170 May 30 (Saros 133) | 2181 Apr 29 (Saros 134) | 2181 Apr 29 (Saros 134) |
| 2192 Mar 28 (Saros 135) ||

### Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
Series members between 1801 and 2200 :
| 1804 Jan 26 (Saros 111) | 1804 Jan 26 (Saros 111) | 1833 Jan 06 (Saros 112) | 1833 Jan 06 (Saros 112) | 1861 Dec 17 (Saros 113) | 1861 Dec 17 (Saros 113) |
| 1890 Nov 26 (Saros 114) | 1890 Nov 26 (Saros 114) | 1919 Nov 07 (Saros 115) | 1919 Nov 07 (Saros 115) | 1948 Oct 18 (Saros 116) | 1948 Oct 18 (Saros 116) |
| 1977 Sep 27 (Saros 117) | 1977 Sep 27 (Saros 117) | 2006 Sep 07 (Saros 118) | 2006 Sep 07 (Saros 118) | 2035 Aug 19 (Saros 119) | 2035 Aug 19 (Saros 119) |
| 2064 Jul 28 (Saros 120) | 2064 Jul 28 (Saros 120) | 2093 Jul 08 (Saros 121) | 2093 Jul 08 (Saros 121) | 2122 Jun 20 (Saros 122) | 2122 Jun 20 (Saros 122) |
| 2151 May 30 (Saros 123) | 2151 May 30 (Saros 123) | 2180 May 09 (Saros 124) | 2180 May 09 (Saros 124) |

### Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two partial solar eclipses of Solar Saros 125.
| September 2, 1997 | September 13, 2015 |