May 1994 lunar eclipse


A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, May 25, 1994, with an umbral magnitude of 0.2432. 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 23.5 hours after perigee, the Moon's apparent diameter was larger.

Visibility

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

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.19408
Umbral Magnitude0.24318
Gamma0.89334
Sun Right Ascension04h06m48.5s
Sun Declination+20°53'35.0"
Sun Semi-Diameter15'47.5"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension16h07m09.9s
Moon Declination-19°59'22.3"
Moon Semi-Diameter16'36.4"
Moon Equatorial Horizontal Parallax1°00'56.9"
ΔT60.3 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.
May 10
Descending node
May 25
Ascending node
Annular solar eclipse
Solar Saros 128
Partial lunar eclipse
Lunar Saros 140

Related eclipses

Eclipses in 1994

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 140

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 solar eclipses of Solar Saros 147.
May 19, 1985May 31, 2003