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June 2076 lunar eclipse

A total lunar eclipse will occur at the Moon’s descending node of orbit on Wednesday, June 17, 2076, with an umbral magnitude of 1.7959. It will be a central lunar eclipse, in which part of the Moon will pass 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 about 1.9 days before perigee, the Moon's apparent diameter will be larger.

Visibility
The eclipse will be completely visible over South America, west Africa, and Antarctica, seen rising over North America and the eastern Pacific Ocean and setting over Europe, west and south Asia, and central and east Africa. == Eclipse details ==
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse. == Eclipse season ==
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) 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. The first and last eclipse in this sequence is separated by one synodic month. == Related eclipses ==
Related eclipses
Eclipses in 2076 A total solar eclipse on January 6. • A partial solar eclipse on June 1. • A total lunar eclipse on June 17.A partial solar eclipse on July 1. • A partial solar eclipse on November 26. • A total lunar eclipse on December 10. Metonic • Preceded by: Lunar eclipse of August 28, 2072 • Followed by: Lunar eclipse of April 4, 2080 Tzolkinex • Preceded by: Lunar eclipse of May 6, 2069 • Followed by: Lunar eclipse of July 29, 2083 Half-Saros • Preceded by: Solar eclipse of June 11, 2067 • Followed by: Solar eclipse of June 22, 2085 Tritos • Preceded by: Lunar eclipse of July 17, 2065 • Followed by: Lunar eclipse of May 17, 2087 Lunar Saros 131 • Preceded by: Lunar eclipse of June 6, 2058 • Followed by: Lunar eclipse of June 28, 2094 Inex • Preceded by: Lunar eclipse of July 7, 2047 • Followed by: Lunar eclipse of May 28, 2105 Triad • Preceded by: Lunar eclipse of August 16, 1989 • Followed by: Lunar eclipse of April 19, 2163 Lunar eclipses of 2074–2078 This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. The penumbral lunar eclipses on February 11, 2074 and August 7, 2074 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 27, 2078 and October 21, 2078 occur in the next lunar year eclipse set. Saros 131 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 (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 138. == See also ==
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