April 1949 lunar eclipse


A total lunar eclipse occurred at the Moon’s descending node of orbit on Wednesday, April 13, 1949, with an umbral magnitude of 1.4251. It was a central lunar eclipse, in which part of the Moon passed through the center of the Earth's shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 19 hours after perigee, the Moon's apparent diameter was larger.
This lunar eclipse was the first of a tetrad, with four total lunar eclipses in series, the others being on October 7, 1949; April 2, 1950; and September 26, 1950.

Visibility

The eclipse was completely visible over central and eastern North America, South America, and Antarctica, seen rising over western North America and the central Pacific Ocean and setting over Africa, Europe, and the Middle East.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude2.38255
Umbral Magnitude1.42511
Gamma0.24740
Sun Right Ascension01h24m45.8s
Sun Declination+08°54'38.8"
Sun Semi-Diameter15'56.9"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension13h25m14.0s
Moon Declination-08°41'13.4"
Moon Semi-Diameter16'39.4"
Moon Equatorial Horizontal Parallax1°01'07.9"
ΔT28.8 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.
April 13
Descending node 		April 28
Ascending node
Total lunar eclipse
Lunar Saros 121		Partial solar eclipse
Solar Saros 147

Related eclipses

Eclipses in 1949

Saros 121

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 128.
April 7, 1940April 19, 1958