Loading AI tools
Penumbral lunar eclipse December 20, 1983 From Wikipedia, the free encyclopedia
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, December 20, 1983,[1] with an umbral magnitude of −0.1167. 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 2.7 days before perigee (on December 22, 1983, at 18:25 UTC), the Moon's apparent diameter was larger.[2]
| Penumbral eclipse | |||||||||
The Moon's hourly motion shown right to left | |||||||||
| Date | December 20, 1983 | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Gamma | 1.0747 | ||||||||
| Magnitude | −0.1167 | ||||||||
| Saros cycle | 144 (14 of 71) | ||||||||
| Penumbral | 242 minutes, 15 seconds | ||||||||
| |||||||||
The eclipse was completely visible over much of North America, South America, Europe, much of Africa, and west and north Asia, seen rising over western North America and the eastern Pacific Ocean and setting over southeast Africa and central and south Asia.[3]
 |
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
| Parameter | Value |
|---|---|
| Penumbral Magnitude | 0.88903 |
| Umbral Magnitude | −0.11673 |
| Gamma | 1.07468 |
| Sun Right Ascension | 17h49m31.1s |
| Sun Declination | -23°25'11.7" |
| Sun Semi-Diameter | 16'15.5" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 05h48m58.9s |
| Moon Declination | +24°28'31.2" |
| Moon Semi-Diameter | 16'09.9" |
| Moon Equatorial Horizontal Parallax | 0°59'19.5" |
| ΔT | 53.7 s |
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.
| December 4 Descending node (new moon) | December 20 Ascending node (full moon) |
|---|---|
 | |
| Annular solar eclipse Solar Saros 132 | Penumbral lunar eclipse Lunar Saros 144 |
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.[5]
The penumbral lunar eclipses on March 1, 1980 and August 26, 1980 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on May 15, 1984 and November 8, 1984 occur in the next lunar year eclipse set.
| Lunar eclipse series sets from 1980 to 1984 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
| 109 | 1980 Jul 27 |
Penumbral |
1.4139 | 114 | 1981 Jan 20 |
Penumbral |
−1.0142 | |
| 119 | 1981 Jul 17 |
Partial |
0.7045 | 124 | 1982 Jan 09 |
Total |
−0.2916 | |
| 129 | 1982 Jul 06 |
Total |
−0.0579 | 134 | 1982 Dec 30 |
Total |
0.3758 | |
| 139 | 1983 Jun 25 |
Partial |
−0.8152 | 144 | 1983 Dec 20 |
Penumbral |
1.0747 | |
| 149 | 1984 Jun 13 |
Penumbral |
−1.5240 | |||||
This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on July 29, 1749. It contains partial eclipses from March 28, 2146 through June 23, 2290; total eclipses from July 4, 2308 through January 28, 2651; and a second set of partial eclipses from February 8, 2669 through June 8, 2867. The series ends at member 71 as a penumbral eclipse on September 4, 3011.
The longest duration of totality will be produced by member 38 at 104 minutes, 53 seconds on September 7, 2416. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]
| Greatest | First | |||
|---|---|---|---|---|
| The greatest eclipse of the series will occur on 2416 Sep 07, lasting 104 minutes, 53 seconds.[7] | Penumbral | Partial | Total | Central |
| 1749 Jul 29 |
2146 Mar 28 |
2308 Jul 04 |
2362 Aug 06 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 2488 Oct 20 |
2651 Jan 28 |
2867 Jun 08 |
3011 Sep 04 | |
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 4–26 occur between 1801 and 2200: | |||||
|---|---|---|---|---|---|
| 4 | 5 | 6 | |||
| 1803 Sep 01 | 1821 Sep 11 | 1839 Sep 23 | |||
| 7 | 8 | 9 | |||
| 1857 Oct 03 | 1875 Oct 14 | 1893 Oct 25 | |||
| 10 | 11 | 12 | |||
| 1911 Nov 06 | 1929 Nov 17 | 1947 Nov 28 | |||
 |
 |
 |
 |
 |
 |
| 13 | 14 | 15 | |||
| 1965 Dec 08 | 1983 Dec 20 | 2001 Dec 30 | |||
 |
 |
|
|
 |
 |
| 16 | 17 | 18 | |||
| 2020 Jan 10 | 2038 Jan 21 | 2056 Feb 01 | |||
 |
 |
 |
 |
 |
 |
| 19 | 20 | 21 | |||
| 2074 Feb 11 | 2092 Feb 23 | 2110 Mar 06 | |||
| 22 | 23 | 24 | |||
| 2128 Mar 16 | 2146 Mar 28 | 2164 Apr 07 | |||
| 25 | 26 | ||||
| 2182 Apr 18 | 2200 Apr 30 | ||||
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 2147 | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| 1809 Apr 30 (Saros 128) |
1820 Mar 29 (Saros 129) |
1831 Feb 26 (Saros 130) |
1842 Jan 26 (Saros 131) |
1852 Dec 26 (Saros 132) | |||||
| 1863 Nov 25 (Saros 133) |
1874 Oct 25 (Saros 134) |
1885 Sep 24 (Saros 135) |
1896 Aug 23 (Saros 136) |
1907 Jul 25 (Saros 137) | |||||
 |
 | ||||||||
| 1918 Jun 24 (Saros 138) |
1929 May 23 (Saros 139) |
1940 Apr 22 (Saros 140) |
1951 Mar 23 (Saros 141) |
1962 Feb 19 (Saros 142) | |||||
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
| 1973 Jan 18 (Saros 143) |
1983 Dec 20 (Saros 144) |
1994 Nov 18 (Saros 145) |
2005 Oct 17 (Saros 146) |
2016 Sep 16 (Saros 147) | |||||
 |
 |
|
|
 |
 |
 |
 |
 |
 |
| 2027 Aug 17 (Saros 148) |
2038 Jul 16 (Saros 149) |
2049 Jun 15 (Saros 150) |
|||||||
 |
 |
|
|
 |
 |
||||
| 2114 Dec 12 (Saros 156) |
|||||||||
| 2147 Sep 09 (Saros 159) | |||||||||
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[8] This lunar eclipse is related to two partial solar eclipses of Solar Saros 151.
| December 13, 1974 | December 24, 1992 |
|---|---|
 |
 |
Seamless Wikipedia browsing. On steroids.
Every time you click a link to Wikipedia, Wiktionary or Wikiquote in your browser's search results, it will show the modern Wikiwand interface.
Wikiwand extension is a five stars, simple, with minimum permission required to keep your browsing private, safe and transparent.
