# November 1955 lunar eclipse

A partial lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, November 29, 1955, with an umbral magnitude of 0.1190. 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 18.5 hours before perigee (on November 30, 1955, at 11:25 UTC), the Moon's apparent diameter was larger.

## Visibility

The eclipse was completely visible over eastern Europe, Asia, and Australia, seen rising over Africa and western Europe and setting over the central Pacific Ocean and northwestern North America.

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
November 29, 1955 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 1.09167 |
| Umbral Magnitude | 0.11899 |
| Gamma | 0.95514 |
| Sun Right Ascension | 16h19m25.1s |
| Sun Declination | -21°25'59.1" |
| Sun Semi-Diameter | 16'13.0" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 04h19m06.8s |
| Moon Declination | +22°24'16.1" |
| Moon Semi-Diameter | 16'40.3" |
| Moon Equatorial Horizontal Parallax | 1°01'11.3" |
| ΔT | 31.4 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 November–December 1955 :
| November 29 Descending node (full moon) | December 14 Ascending node (new moon) |
| Partial lunar eclipse Lunar Saros 115 | Annular solar eclipse Solar Saros 141 |

## Related eclipses
### Eclipses in 1955

* A penumbral lunar eclipse on January 8.
* A penumbral lunar eclipse on June 5.
* A total solar eclipse on June 20.
* A partial lunar eclipse on November 29.
* An annular solar eclipse on December 14.

### Metonic

* Preceded by: Lunar eclipse of February 11, 1952
* Followed by: Lunar eclipse of September 17, 1959

### Tzolkinex

* Preceded by: Lunar eclipse of October 18, 1948
* Followed by: Lunar eclipse of January 9, 1963

### Half-Saros

* Preceded by: Solar eclipse of November 23, 1946
* Followed by: Solar eclipse of December 4, 1964

### Tritos

* Preceded by: Lunar eclipse of December 29, 1944
* Followed by: Lunar eclipse of October 29, 1966

### Lunar Saros 115

* Preceded by: Lunar eclipse of November 18, 1937
* Followed by: Lunar eclipse of December 10, 1973

### Inex

* Preceded by: Lunar eclipse of December 19, 1926
* Followed by: Lunar eclipse of November 8, 1984

### Triad

* Preceded by: Lunar eclipse of January 28, 1869
* Followed by: Lunar eclipse of September 29, 2042

### Lunar eclipses of 1955–1958

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 penumbral lunar eclipse on January 8, 1955 occurs in the previous lunar year eclipse set, and the penumbral lunar eclipse on April 4, 1958 occurs in the next lunar year eclipse set.
Lunar eclipse series sets from 1955 to 1958 :
| Ascending node | Ascending node | Ascending node | Ascending node | Descending node | Descending node | Descending node | Descending node |
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 110 | 1955 Jun 05 | Penumbral | −1.2384 | 115 | 1955 Nov 29 | Partial | 0.9551 |
| 120 | 1956 May 24 | Partial | −0.4726 | 125 | 1956 Nov 18 | Total | 0.2917 |
| 130 | 1957 May 13 | Total | 0.3046 | 135 | 1957 Nov 07 | Total | −0.4332 |
| 140 | 1958 May 03 | Partial | 1.0188 | 145 | 1958 Oct 27 | Penumbral | −1.1571 |

### Saros 115

This eclipse is a part of Saros series 115, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on April 21, 1000. It contains partial eclipses from July 6, 1126 through September 30, 1270; total eclipses from October 11, 1288 through July 20, 1739; and a second set of partial eclipses from July 30, 1757 through February 13, 2082. The series ends at member 72 as a penumbral eclipse on June 13, 2280.
The longest duration of totality was produced by member 36 at 99 minutes, 47 seconds on May 15, 1631. All eclipses in this series occur at the Moon’s descending node of orbit.
| Greatest | First | First | First | First |
| The greatest eclipse of the series occurred on 1631 May 15, lasting 99 minutes, 47 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series occurred on 1631 May 15, lasting 99 minutes, 47 seconds. | 1000 Apr 21 | 1126 Jul 06 | 1288 Oct 11 | 1541 Mar 12 |
| Last ||||
| The greatest eclipse of the series occurred on 1631 May 15, lasting 99 minutes, 47 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series occurred on 1631 May 15, lasting 99 minutes, 47 seconds. | 1685 Jun 16 | 1739 Jul 20 | 2082 Feb 13 | 2280 Jun 13 |
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 46–67 occur between 1801 and 2200: :
| 46 | 46 | 47 | 47 | 48 | 48 |
| 1811 Sep 02 | 1811 Sep 02 | 1829 Sep 13 | 1829 Sep 13 | 1847 Sep 24 | 1847 Sep 24 |
| 49 | 49 | 50 | 50 | 51 | 51 |
| 1865 Oct 04 | 1865 Oct 04 | 1883 Oct 16 | 1883 Oct 16 | 1901 Oct 27 | 1901 Oct 27 |
| 52 | 52 | 53 | 53 | 54 | 54 |
| 1919 Nov 07 | 1919 Nov 07 | 1937 Nov 18 | 1937 Nov 18 | 1955 Nov 29 | 1955 Nov 29 |
| 55 | 55 | 56 | 56 | 57 | 57 |
| 1973 Dec 10 | 1973 Dec 10 | 1991 Dec 21 | 1991 Dec 21 | 2009 Dec 31 | 2009 Dec 31 |
| 58 | 58 | 59 | 59 | 60 | 60 |
| 2028 Jan 12 | 2028 Jan 12 | 2046 Jan 22 | 2046 Jan 22 | 2064 Feb 02 | 2064 Feb 02 |
| 61 | 61 | 62 | 62 | 63 | 63 |
| 2082 Feb 13 | 2082 Feb 13 | 2100 Feb 24 | 2100 Feb 24 | 2118 Mar 07 | 2118 Mar 07 |
| 64 | 64 | 65 | 65 | 66 | 66 |
| 2136 Mar 18 | 2136 Mar 18 | 2154 Mar 29 | 2154 Mar 29 | 2172 Apr 09 | 2172 Apr 09 |
| 67 ||
| 2190 Apr 20 ||

### 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 :
| 1803 Feb 06 (Saros 101) | 1803 Feb 06 (Saros 101) | 1814 Jan 06 (Saros 102) | 1814 Jan 06 (Saros 102) | 1824 Dec 06 (Saros 103) | 1824 Dec 06 (Saros 103) | | | 1846 Oct 04 (Saros 105) | 1846 Oct 04 (Saros 105) |
| 1857 Sep 04 (Saros 106) | 1857 Sep 04 (Saros 106) | 1868 Aug 03 (Saros 107) | 1868 Aug 03 (Saros 107) | 1879 Jul 03 (Saros 108) | 1879 Jul 03 (Saros 108) | 1890 Jun 03 (Saros 109) | 1890 Jun 03 (Saros 109) | 1901 May 03 (Saros 110) | 1901 May 03 (Saros 110) |
| 1912 Apr 01 (Saros 111) | 1912 Apr 01 (Saros 111) | 1923 Mar 03 (Saros 112) | 1923 Mar 03 (Saros 112) | 1934 Jan 30 (Saros 113) | 1934 Jan 30 (Saros 113) | 1944 Dec 29 (Saros 114) | 1944 Dec 29 (Saros 114) | 1955 Nov 29 (Saros 115) | 1955 Nov 29 (Saros 115) |
| 1966 Oct 29 (Saros 116) | 1966 Oct 29 (Saros 116) | 1977 Sep 27 (Saros 117) | 1977 Sep 27 (Saros 117) | 1988 Aug 27 (Saros 118) | 1988 Aug 27 (Saros 118) | 1999 Jul 28 (Saros 119) | 1999 Jul 28 (Saros 119) | 2010 Jun 26 (Saros 120) | 2010 Jun 26 (Saros 120) |
| 2021 May 26 (Saros 121) | 2021 May 26 (Saros 121) | 2032 Apr 25 (Saros 122) | 2032 Apr 25 (Saros 122) | 2043 Mar 25 (Saros 123) | 2043 Mar 25 (Saros 123) | 2054 Feb 22 (Saros 124) | 2054 Feb 22 (Saros 124) | 2065 Jan 22 (Saros 125) | 2065 Jan 22 (Saros 125) |
| 2075 Dec 22 (Saros 126) | 2075 Dec 22 (Saros 126) | 2086 Nov 20 (Saros 127) | 2086 Nov 20 (Saros 127) | 2097 Oct 21 (Saros 128) | 2097 Oct 21 (Saros 128) | 2108 Sep 20 (Saros 129) | 2108 Sep 20 (Saros 129) | 2119 Aug 20 (Saros 130) | 2119 Aug 20 (Saros 130) |
| 2130 Jul 21 (Saros 131) | 2130 Jul 21 (Saros 131) | 2141 Jun 19 (Saros 132) | 2141 Jun 19 (Saros 132) | 2152 May 18 (Saros 133) | 2152 May 18 (Saros 133) | 2163 Apr 19 (Saros 134) | 2163 Apr 19 (Saros 134) | 2174 Mar 18 (Saros 135) | 2174 Mar 18 (Saros 135) |
| 2185 Feb 14 (Saros 136) | 2185 Feb 14 (Saros 136) | 2196 Jan 15 (Saros 137) | 2196 Jan 15 (Saros 137) |

### 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 :
| 1811 Mar 10 (Saros 110) | 1811 Mar 10 (Saros 110) | 1840 Feb 17 (Saros 111) | 1840 Feb 17 (Saros 111) | 1869 Jan 28 (Saros 112) | 1869 Jan 28 (Saros 112) |
| 1898 Jan 08 (Saros 113) | 1898 Jan 08 (Saros 113) | 1926 Dec 19 (Saros 114) | 1926 Dec 19 (Saros 114) | 1955 Nov 29 (Saros 115) | 1955 Nov 29 (Saros 115) |
| 1984 Nov 08 (Saros 116) | 1984 Nov 08 (Saros 116) | 2013 Oct 18 (Saros 117) | 2013 Oct 18 (Saros 117) | 2042 Sep 29 (Saros 118) | 2042 Sep 29 (Saros 118) |
| 2071 Sep 09 (Saros 119) | 2071 Sep 09 (Saros 119) | 2100 Aug 19 (Saros 120) | 2100 Aug 19 (Saros 120) | 2129 Jul 31 (Saros 121) | 2129 Jul 31 (Saros 121) |
| 2158 Jul 11 (Saros 122) | 2158 Jul 11 (Saros 122) | 2187 Jun 20 (Saros 123) | 2187 Jun 20 (Saros 123) |

### 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 122.
| November 23, 1946 | December 4, 1964 |