January 1972 lunar eclipse


A total lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, January 30, 1972, 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, the Moon's apparent diameter was smaller.

Visibility

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.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude2.09866
Umbral Magnitude1.04971
Gamma−0.42729
Sun Right Ascension20h48m23.2s
Sun Declination-17°50'13.7"
Sun Semi-Diameter16'14.2"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension08h47m46.4s
Moon Declination+17°27'35.5"
Moon Semi-Diameter15'28.8"
Moon Equatorial Horizontal Parallax0°56'48.6"
ΔT42.3 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months 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.
January 16, 1972|January 16]
Ascending node
January 30
Descending node
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133

Related eclipses

Eclipses in 1972

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 133

Inex

Triad

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days. This lunar eclipse is related to two annular solar eclipses of Solar Saros 140.
January 25, 1963February 4, 1981