July 1936 lunar eclipse


A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, July 4, 1936, with an umbral magnitude of 0.2668. 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. The Moon's apparent diameter was near the average diameter because it occurred 6.8 days after apogee and 7.2 days before perigee.

Visibility

The eclipse was completely visible over south and east Asia, Australia, and Antarctica, seen rising over Africa, Europe, and west and central Asia and setting over northeast Asia 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 Magnitude1.27781
Umbral Magnitude0.26679
Gamma0.86423
Sun Right Ascension06h54m24.6s
Sun Declination+22°51'29.8"
Sun Semi-Diameter15'43.8"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension18h53m44.0s
Moon Declination-22°03'02.9"
Moon Semi-Diameter15'33.6"
Moon Equatorial Horizontal Parallax0°57'06.2"
ΔT23.8 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.
June 19
Descending node
July 4
Ascending node
Total solar eclipse
Solar Saros 126
Partial lunar eclipse
Lunar Saros 138

Related eclipses

Eclipses in 1936

Saros 138

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 total solar eclipses of Solar Saros 145.
June 29, 1927July 9, 1945