August 1988 lunar eclipse


A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, August 27, 1988, with an umbral magnitude of 0.2916. 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 7 hours before perigee, the Moon's apparent diameter was larger.

Visibility

The eclipse was completely visible over eastern Australia, western North America, and much of the Pacific Ocean, seen rising over western Australia and the eastern half of Asia and setting over much of North America and South America.

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
ParameterValue
Penumbral Magnitude1.23803
Umbral Magnitude0.29159
Gamma−0.86816
Sun Right Ascension10h25m02.1s
Sun Declination+09°54'10.9"
Sun Semi-Diameter15'50.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension22h26m40.4s
Moon Declination-10°41'41.3"
Moon Semi-Diameter16'43.7"
Moon Equatorial Horizontal Parallax1°01'23.7"
ΔT56.1 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.
August 27
Ascending node
September 11
Descending node
Partial lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144

Related eclipses

Eclipses in 1988

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 118

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 125.
August 22, 1979September 2, 1997