April 2051 lunar eclipse


A total lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, April 26, 2051, with an umbral magnitude of 1.2034. 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 about 2.6 days after apogee, the Moon's apparent diameter will be smaller.
This lunar eclipse is the third of a tetrad, with four total lunar eclipses in series, the others being on May 6, 2050; October 30, 2050; and October 19, 2051.

Visibility

The eclipse will be completely visible over South America and west Africa, seen rising over North America and the eastern Pacific Ocean and setting over central and east Africa, Europe, and west, central, and south Asia.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude2.27848
Umbral Magnitude1.20339
Gamma0.33710
Sun Right Ascension02h14m06.4s
Sun Declination+13°27'39.8"
Sun Semi-Diameter15'53.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension14h14m24.0s
Moon Declination-13°09'52.9"
Moon Semi-Diameter14'47.3"
Moon Equatorial Horizontal Parallax0°54'16.4"
ΔT85.9 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 11, 2051|April 11]
Descending node
April 26
Ascending node
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132

Related eclipses

Eclipses in 2051

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 132

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 139.
April 20, 2042April 30, 2060