December 1965 lunar eclipse


A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, December 8, 1965, with an umbral magnitude of −0.1200. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 2.5 days before perigee, the Moon's apparent diameter was larger.

Visibility

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

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude0.88203
Umbral Magnitude−0.12004
Gamma1.07748
Sun Right Ascension17h00m58.1s
Sun Declination-22°45'04.3"
Sun Semi-Diameter16'14.4"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension05h00m02.9s
Moon Declination+23°47'53.1"
Moon Semi-Diameter16'12.3"
Moon Equatorial Horizontal Parallax0°59'28.5"
ΔT36.5 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.
November 23
Descending node
December 8
Ascending node
Annular solar eclipse
Solar Saros 132
Penumbral lunar eclipse
Lunar Saros 144

Related eclipses

Eclipses in 1965

Saros 144

Tritos series

Inex series

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 partial solar eclipses of Solar Saros 151.
December 2, 1956December 13, 1974