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January 1972 lunar eclipse

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January 1972 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateJanuary 30, 1972
Gamma−0.4273
Magnitude1.0497
Saros cycle133 (24 of 71)
Totality34 minutes, 48 seconds
Partiality203 minutes, 23 seconds
Penumbral340 minutes, 19 seconds
Contacts (UTC)
P18:03:16
U19:11:39
U210:35:57
Greatest10:53:23
U311:10:45
U412:35:03
P413:43:35

A total lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, January 30, 1972,[1] with an umbral magnitude of 1.0497. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 6.6 days before apogee (on February 6, 1972, at 0:45 UTC), the Moon's apparent diameter was smaller.[2]

Visibility

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The eclipse was completely visible over northeast Asia, western and central North America, and the central Pacific Ocean, seen rising over much of Asia and Australia and setting over eastern North America and South America.[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]

January 30, 1972 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.09866
Umbral Magnitude 1.04971
Gamma −0.42729
Sun Right Ascension 20h48m23.2s
Sun Declination -17°50'13.7"
Sun Semi-Diameter 16'14.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h47m46.4s
Moon Declination +17°27'35.5"
Moon Semi-Diameter 15'28.8"
Moon Equatorial Horizontal Parallax 0°56'48.6"
ΔT 42.3 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 January 1972
January 16
Ascending node (new moon)
January 30
Descending node (full moon)
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133
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Eclipses in 1972

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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 133

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Inex

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Triad

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Lunar eclipses of 1969–1973

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Lunar eclipse series sets from 1969–1973
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
108 1969 Aug 27
Penumbral
−1.54066 113 1970 Feb 21
Partial
0.96198
118 1970 Aug 17
Partial
−0.80534 123 1971 Feb 10
Total
0.27413
128 1971 Aug 06
Total
−0.07944 133 1972 Jan 30
Total
−0.42729
138 1972 Jul 26
Partial
0.71167 143 1973 Jan 18
Penumbral
−1.08446
148 1973 Jul 15
Penumbral
1.51782
Last set 1969 Sep 25 Last set 1969 Apr 02
Next set 1973 Jun 15 Next set 1973 Dec 10

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 annular solar eclipses of Solar Saros 140.

January 25, 1963 February 4, 1981

See also

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Notes

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  1. ^ "January 29–30, 1972 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 3 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 3 January 2025.
  3. ^ "Total Lunar Eclipse of 1972 Jan 30" (PDF). NASA. Retrieved 3 January 2025.
  4. ^ "Total Lunar Eclipse of 1972 Jan 30". EclipseWise.com. Retrieved 3 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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