October 1930 lunar eclipse


A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, October 7, 1930, with an umbral magnitude of 0.0253. 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 about 4.4 days after apogee, the Moon's apparent diameter was smaller.

Visibility

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

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.09067
Umbral Magnitude0.02525
Gamma−0.98118
Sun Right Ascension12h50m44.6s
Sun Declination-05°26'30.5"
Sun Semi-Diameter16'00.5"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension00h52m28.2s
Moon Declination+04°38'57.1"
Moon Semi-Diameter15'01.5"
Moon Equatorial Horizontal Parallax0°55'08.6"
ΔT24.1 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.
October 7
Ascending node
October 21
Descending node
Partial lunar eclipse
Lunar Saros 116
Total solar eclipse
Solar Saros 142

Related eclipses

Eclipses in 1930

Saros 116

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 123.
October 1, 1921October 12, 1939