August 1943 lunar eclipse


A partial lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, August 15, 1943, with an umbral magnitude of 0.8697. 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 10 hours after 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 eastern South America, west Africa, and Europe and setting over northeast Asia and eastern Australia.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.81515
Umbral Magnitude0.86970
Gamma−0.55335
Sun Right Ascension09h37m47.7s
Sun Declination+14°09'07.3"
Sun Semi-Diameter15'47.7"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension21h38m19.9s
Moon Declination-14°42'08.2"
Moon Semi-Diameter16'42.3"
Moon Equatorial Horizontal Parallax1°01'18.6"
ΔT26.2 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 1
Ascending node
August 15
Descending node
Annular solar eclipse
Solar Saros 125
Partial lunar eclipse
Lunar Saros 137

Related eclipses

Eclipses in 1943

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 137

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 total solar eclipses of Solar Saros 144.
August 10, 1934August 20, 1952