May 1956 lunar eclipse
partial
DateMay 24, 1956
Gamma−0.4726
Magnitude0.9647
Saros ser120
Saros no55 of 84
Partiality204 minutes, 27 seconds
Penumbral348 minutes, 32 seconds
P 112:37:06
U 113:49:05
Greatest15:31:20
U 417:13:32
P 418:25:38
PreviousNovember 1955
NextNovember 1956

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, May 24, 1956,[1] 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.[2]

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.[3]

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

May 24, 1956 Lunar Eclipse Parameters
ParameterValue
Penumbral Magnitude2.01740
Umbral Magnitude0.96473
Gamma−0.47260
Sun Right Ascension04h05m33.5s
Sun Declination+20°50'30.4"
Sun Semi-Diameter15'47.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension16h05m23.2s
Moon Declination-21°16'24.6"
Moon Semi-Diameter15'00.0"
Moon Equatorial Horizontal Parallax0°55'03.0"
ΔT31.6 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 May–June 1956
May 24
Ascending node (full moon)
June 8
Descending node (new moon)
Partial lunar eclipse
Lunar Saros 120
Total solar eclipse
Solar Saros 146

Eclipses in 1956

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 120

Inex

Triad

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two total solar eclipses of Solar Saros 127.

May 20, 1947May 30, 1965

See also

Notes

  1. ^ "May 24–25, 1956 Partial Lunar Eclipse". timeanddate. Retrieved 25 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 December 2024.
  3. ^ "Partial Lunar Eclipse of 1956 May 24". NASA. Retrieved 25 December 2024.
  4. ^ "Partial Lunar Eclipse of 1956 May 24". EclipseWise.com. Retrieved 25 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros