# December 1944 lunar eclipse

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, December 29, 1944, with an umbral magnitude of −0.0176. It was a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 about 6 days after perigee (on December 23, 1944, at 12:40 UTC), the Moon's apparent diameter was larger.
This eclipse was the last of four penumbral lunar eclipses in 1944, with the others occurring on February 9, July 6, and August 4.
Saturn was conjunct with the Moon during this eclipse.

## Visibility

The eclipse was completely visible over much of Asia, Australia, and northwestern North America, seen rising over Europe, east Africa, and the Middle East and setting over much of North America and the eastern Pacific Ocean.

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
December 29, 1944 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 1.02198 |
| Umbral Magnitude | −0.01757 |
| Gamma | −1.01151 |
| Sun Right Ascension | 18h33m56.1s |
| Sun Declination | -23°12'58.6" |
| Sun Semi-Diameter | 16'15.9" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 06h34m05.9s |
| Moon Declination | +22°14'56.3" |
| Moon Semi-Diameter | 15'38.8" |
| Moon Equatorial Horizontal Parallax | 0°57'25.5" |
| ΔT | 26.9 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 December 1944–January 1945 :
| December 29 Ascending node (full moon) | January 14 Descending node (new moon) |
| Penumbral lunar eclipse Lunar Saros 114 | Annular solar eclipse Solar Saros 140 |

## Related eclipses
### Eclipses in 1944

* A total solar eclipse on January 25.
* A penumbral lunar eclipse on February 9.
* A penumbral lunar eclipse on July 6.
* An annular solar eclipse on July 20.
* A penumbral lunar eclipse on August 4.
* A penumbral lunar eclipse on December 29.

### Metonic

* Preceded by: Lunar eclipse of March 13, 1941
* Followed by: Lunar eclipse of October 18, 1948

### Tzolkinex

* Preceded by: Lunar eclipse of November 18, 1937
* Followed by: Lunar eclipse of February 11, 1952

### Half-Saros

* Preceded by: Solar eclipse of December 25, 1935
* Followed by: Solar eclipse of January 5, 1954

### Tritos

* Preceded by: Lunar eclipse of January 30, 1934
* Followed by: Lunar eclipse of November 29, 1955

### Lunar Saros 114

* Preceded by: Lunar eclipse of December 19, 1926
* Followed by: Lunar eclipse of January 9, 1963

### Inex

* Preceded by: Lunar eclipse of January 20, 1916
* Followed by: Lunar eclipse of December 10, 1973

### Triad

* Preceded by: Lunar eclipse of February 27, 1858
* Followed by: Lunar eclipse of October 30, 2031

### Lunar eclipses of 1944–1947

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 eclipses on February 9, 1944 and August 4, 1944 occur in the previous lunar year eclipse set.
Lunar eclipse series sets from 1944 to 1947 :
| 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 |
| 109 | 1944 Jul 06 | Penumbral | 1.2597 | 114 | 1944 Dec 29 | Penumbral | −1.0115 |
| 119 | 1945 Jun 25 | Partial | 0.5370 | 124 | 1945 Dec 19 | Total | −0.2845 |
| 129 | 1946 Jun 14 | Total | −0.2324 | 134 | 1946 Dec 08 | Total | 0.3864 |
| 139 | 1947 Jun 03 | Partial | −0.9850 | 144 | 1947 Nov 28 | Penumbral | 1.0838 |

### Saros 114

This eclipse is a part of Saros series 114, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on May 13, 971 AD. It contains partial eclipses from August 7, 1115 through February 18, 1440; total eclipses from February 28, 1458 through July 17, 1674; and a second set of partial eclipses from July 28, 1692 through November 26, 1890. The series ends at member 71 as a penumbral eclipse on June 22, 2233.
The longest duration of totality was produced by member 35 at 106 minutes, 5 seconds on May 24, 1584. 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 1584 May 24, lasting 106 minutes, 5 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series occurred on 1584 May 24, lasting 106 minutes, 5 seconds. | 971 May 13 | 1115 Aug 07 | 1458 Feb 28 | 1530 Apr 12 |
| Last ||||
| The greatest eclipse of the series occurred on 1584 May 24, lasting 106 minutes, 5 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series occurred on 1584 May 24, lasting 106 minutes, 5 seconds. | 1638 Jun 26 | 1674 Jul 17 | 1890 Nov 26 | 2233 Jun 22 |
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 48–69 occur between 1801 and 2200: :
| 48 | 48 | 49 | 49 | 50 | 50 |
| 1818 Oct 14 | 1818 Oct 14 | 1836 Oct 24 | 1836 Oct 24 | 1854 Nov 04 | 1854 Nov 04 |
| 51 | 51 | 52 | 52 | 53 | 53 |
| 1872 Nov 15 | 1872 Nov 15 | 1890 Nov 26 | 1890 Nov 26 | 1908 Dec 07 | 1908 Dec 07 |
| 54 | 54 | 55 | 55 | 56 | 56 |
| 1926 Dec 19 | 1926 Dec 19 | 1944 Dec 29 | 1944 Dec 29 | 1963 Jan 09 | 1963 Jan 09 |
| 57 | 57 | 58 | 58 | 59 | 59 |
| 1981 Jan 20 | 1981 Jan 20 | 1999 Jan 31 | 1999 Jan 31 | 2017 Feb 11 | 2017 Feb 11 |
| 60 | 60 | 61 | 61 | 62 | 62 |
| 2035 Feb 22 | 2035 Feb 22 | 2053 Mar 04 | 2053 Mar 04 | 2071 Mar 16 | 2071 Mar 16 |
| 63 | 63 | 64 | 64 | 65 | 65 |
| 2089 Mar 26 | 2089 Mar 26 | 2107 Apr 07 | 2107 Apr 07 | 2125 Apr 18 | 2125 Apr 18 |
| 66 | 66 | 67 | 67 | 68 | 68 |
| 2143 Apr 29 | 2143 Apr 29 | 2161 May 09 | 2161 May 09 | 2179 May 21 | 2179 May 21 |
| 69 ||
| 2197 May 31 ||

### 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 :
| 1829 Mar 20 (Saros 110) | 1829 Mar 20 (Saros 110) | 1858 Feb 27 (Saros 111) | 1858 Feb 27 (Saros 111) | 1887 Feb 08 (Saros 112) | 1887 Feb 08 (Saros 112) |
| 1916 Jan 20 (Saros 113) | 1916 Jan 20 (Saros 113) | 1944 Dec 29 (Saros 114) | 1944 Dec 29 (Saros 114) | 1973 Dec 10 (Saros 115) | 1973 Dec 10 (Saros 115) |
| 2002 Nov 20 (Saros 116) | 2002 Nov 20 (Saros 116) | 2031 Oct 30 (Saros 117) | 2031 Oct 30 (Saros 117) | 2060 Oct 09 (Saros 118) | 2060 Oct 09 (Saros 118) |
| 2089 Sep 19 (Saros 119) | 2089 Sep 19 (Saros 119) | 2118 Aug 31 (Saros 120) | 2118 Aug 31 (Saros 120) | 2147 Aug 11 (Saros 121) | 2147 Aug 11 (Saros 121) |
| 2176 Jul 21 (Saros 122) ||

### 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 total solar eclipses of Solar Saros 121.
| December 25, 1935 | January 5, 1954 |