August 1952 lunar eclipse


A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, August 5, 1952, with an umbral magnitude of 0.5318. 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 only about 1.5 hours before perigee, the Moon's apparent diameter was larger.

Visibility

The eclipse was completely visible over east Africa, much of Asia, western Australia, and Antarctica, seen rising over west Africa, Europe, and eastern South America and setting over northeast Asia and eastern Australia.

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.47418
Umbral Magnitude0.53177
Gamma−0.73835
Sun Right Ascension09h03m03.1s
Sun Declination+16°50'04.8"
Sun Semi-Diameter15'46.2"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension21h04m14.8s
Moon Declination-17°32'03.6"
Moon Semi-Diameter16'44.0"
Moon Equatorial Horizontal Parallax1°01'24.7"
ΔT30.1 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.
August 5
Ascending node
August 20, 1952|August 20]
Descending node
Partial lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144

Related eclipses

Eclipses in 1952

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 118

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 125.
August 1, 1943August 11, 1961