Partial eclipse | |||||||||||||
The Moon's hourly motion shown right to left | |||||||||||||
Date | May 24, 1956 | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | −0.4726 | ||||||||||||
Magnitude | 0.9647 | ||||||||||||
Saros cycle | 120 (55 of 84) | ||||||||||||
Partiality | 204 minutes, 27 seconds | ||||||||||||
Penumbral | 348 minutes, 32 seconds | ||||||||||||
| |||||||||||||
← November 1955November 1956 → |
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, May 24, 1956, with an umbral magnitude of 0.9647. 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 about 4.3 days before apogee (on May 28, 1956, at 22:10 UTC), the Moon's apparent diameter was smaller.
This lunar eclipse was the first of an almost tetrad, with the others being on November 18, 1956 (total); May 13, 1957 (total); and November 7, 1957 (total).
This was the first eclipse of the last partial set in Lunar Saros 120.
Visibility
The eclipse was completely visible over east Asia, Australia, and Antarctica, seen rising over central and east Africa, eastern Europe, and the western half of Asia and setting over 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.
Parameter | Value |
---|---|
Penumbral Magnitude | 2.01740 |
Umbral Magnitude | 0.96473 |
Gamma | −0.47260 |
Sun Right Ascension | 04h05m33.5s |
Sun Declination | +20°50'30.4" |
Sun Semi-Diameter | 15'47.4" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 16h05m23.2s |
Moon Declination | -21°16'24.6" |
Moon Semi-Diameter | 15'00.0" |
Moon Equatorial Horizontal Parallax | 0°55'03.0" |
ΔT | 31.6 s |
Eclipse season
See also: Eclipse cycleThis 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.
May 24 Ascending node (full moon) |
June 8 Descending node (new moon) |
---|---|
Partial lunar eclipse Lunar Saros 120 |
Total solar eclipse Solar Saros 146 |
Related eclipses
Eclipses in 1956
- A partial lunar eclipse on May 24.
- A total solar eclipse on June 8.
- A total lunar eclipse on November 18.
- A partial solar eclipse on December 2.
Metonic
- Preceded by: Lunar eclipse of August 5, 1952
- Followed by: Lunar eclipse of March 13, 1960
Tzolkinex
- Preceded by: Lunar eclipse of April 13, 1949
- Followed by: Lunar eclipse of July 6, 1963
Half-Saros
- Preceded by: Solar eclipse of May 20, 1947
- Followed by: Solar eclipse of May 30, 1965
Tritos
- Preceded by: Lunar eclipse of June 25, 1945
- Followed by: Lunar eclipse of April 24, 1967
Lunar Saros 120
- Preceded by: Lunar eclipse of May 14, 1938
- Followed by: Lunar eclipse of June 4, 1974
Inex
- Preceded by: Lunar eclipse of June 15, 1927
- Followed by: Lunar eclipse of May 4, 1985
Triad
- Preceded by: Lunar eclipse of July 23, 1869
- Followed by: Lunar eclipse of March 25, 2043
Lunar eclipses of 1955–1958
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Date viewing |
Type chart |
Saros | Date viewing |
Type chart | |
110 | 1955 Jun 5 |
Penumbral |
115 | 1955 Nov 29 |
Partial | |
120 | 1956 May 24 |
Partial |
125 | 1956 Nov 18 |
Total | |
130 | 1957 May 13 |
Total |
135 | 1957 Nov 7 |
Total | |
140 | 1958 May 3 |
Partial |
145 | 1958 Oct 27 |
Penumbral | |
Last set | 1954 Jul 16 | Last set | 1955 Jan 8 | |||
Next set | 1958 Apr 4 | Next set | 1959 Sep 17 |
Tritos series
The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.
This series produces 20 total eclipses between April 24, 1967 and August 11, 2185, only being partial on November 19, 2021.
Tritos eclipse series (subset 1901–2087) | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Date Viewing |
Type chart |
Saros | Date Viewing |
Type chart | |
115 | 1901 Oct 27 |
Partial |
116 | 1912 Sep 26 |
Partial | |
117 | 1923 Aug 26 |
Partial |
118 | 1934 Jul 26 |
Partial | |
119 | 1945 Jun 25 |
Partial |
120 | 1956 May 24 |
Partial | |
121 | 1967 Apr 24 |
Total |
122 | 1978 Mar 24 |
Total | |
123 | 1989 Feb 20 |
Total |
124 | 2000 Jan 21 |
Total | |
125 | 2010 Dec 21 |
Total |
126 | 2021 Nov 19 |
Partial | |
127 | 2032 Oct 18 |
Total |
128 | 2043 Sep 19 |
Total | |
129 | 2054 Aug 18 |
Total |
130 | 2065 Jul 17 |
Total | |
131 | 2076 Jun 17 |
Total |
132 | 2087 May 17 |
Total | |
133 | 2098 Apr 15 |
Total |
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 127.
May 20, 1947 | May 30, 1965 |
---|---|
See also
Notes
- "May 24–25, 1956 Partial Lunar Eclipse". timeanddate. Retrieved 25 December 2024.
- "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 December 2024.
- "Partial Lunar Eclipse of 1956 May 24" (PDF). NASA. Retrieved 25 December 2024.
- "Partial Lunar Eclipse of 1956 May 24". EclipseWise.com. Retrieved 25 December 2024.
- Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
- 1956 May 24 chart Eclipse Predictions by Fred Espenak, NASA/GSFC
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