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May 1976 lunar eclipse

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May 1976 lunar eclipse
Partial eclipse
The Moon's hourly motion shown right to left
DateMay 13, 1976
Gamma0.9586
Magnitude0.1217
Saros cycle140 (23 of 80)
Partiality75 minutes, 23 seconds
Penumbral251 minutes, 49 seconds
Contacts (UTC)
P117:48:25
U119:16:36
Greatest19:54:21
U420:31:59
P422:00:14

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, May 13, 1976,[1] with an umbral magnitude of 0.1217. 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 1.1 days after perigee (on May 12, 1976, at 17:30 UTC), the Moon's apparent diameter was larger.[2]

Visibility

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The eclipse was completely visible over central and east Africa, eastern Europe, the western half of Asia, western Australia, and Antarctica, seen rising over eastern South America, west Africa, and western Europe and setting over east and northeast Asia and eastern Australia.[3]

Eclipse details

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

May 13, 1976 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.07612
Umbral Magnitude 0.12170
Gamma 0.95860
Sun Right Ascension 03h23m03.9s
Sun Declination +18°33'49.8"
Sun Semi-Diameter 15'49.5"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 15h23m42.3s
Moon Declination -17°36'13.1"
Moon Semi-Diameter 16'34.8"
Moon Equatorial Horizontal Parallax 1°00'51.1"
ΔT 46.9 s

Eclipse season

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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 April–May 1976
April 29
Descending node (new moon)
May 13
Ascending node (full moon)
Annular solar eclipse
Solar Saros 128
Partial lunar eclipse
Lunar Saros 140
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Eclipses in 1976

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 140

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Inex

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Triad

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Lunar eclipses of 1973–1976

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Lunar eclipse series sets from 1973–1976
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
110 1973 Jun 15
Penumbral
−1.32166 115 1973 Dec 10
Partial
0.96441
120 1974 Jun 04
Partial
−0.54887 125 1974 Nov 29
Total
0.30540
130 1975 May 25
Total
0.23674 135 1975 Nov 18
Total
−0.41343
140 1976 May 13
Partial
0.95860 145 1976 Nov 06
Penumbral
−1.12760
Last set 1973 Jul 15 Last set 1973 Jan 18
Next set 1977 Apr 04 Next set 1977 Sep 27

Half-Saros cycle

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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 partial solar eclipses of Solar Saros 147.

May 9, 1967 May 19, 1985

See also

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Notes

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  1. ^ "May 13–14, 1976 Partial Lunar Eclipse". timeanddate. Retrieved 4 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 4 January 2025.
  3. ^ "Partial Lunar Eclipse of 1976 May 13" (PDF). NASA. Retrieved 4 January 2025.
  4. ^ "Partial Lunar Eclipse of 1976 May 13". EclipseWise.com. Retrieved 4 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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