May 2031 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, May 7, 2031,[1] with an umbral magnitude of −0.0892. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 about 2 days before perigee (on May 9, 2031, at 3:35 UTC), the Moon's apparent diameter will be larger.[2]

Visibility

The eclipse will be completely visible over eastern North America, South America, Antarctica, and west Africa, seen rising over western North America and the eastern Pacific Ocean and setting over Africa, Europe, and the Middle East.[3]

File:Lunar eclipse from moon-2031May07.png File:Lunar eclipse chart close-2031May07.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

May 7, 2031 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.88267
Umbral Magnitude −0.08921
Gamma −1.06949
Sun Right Ascension 02h55m49.7s
Sun Declination +16°44'40.2"
Sun Semi-Diameter 15'51.2"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 14h54m58.0s
Moon Declination -17°47'29.4"
Moon Semi-Diameter 16'18.7"
Moon Equatorial Horizontal Parallax 0°59'52.0"
ΔT 74.5 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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.

Eclipse season of May–June 2031
May 7
Ascending node (full moon)
May 21
Descending node (new moon)
June 5
Ascending node (full moon)
File:Lunar eclipse chart close-2031May07.png File:SE2031May21A.png File:Lunar eclipse chart close-2031Jun05.png
Penumbral lunar eclipse
Lunar Saros 112
Annular solar eclipse
Solar Saros 138
Penumbral lunar eclipse
Lunar Saros 150

Related eclipses

Eclipses in 2031

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 112

Inex

Triad

Lunar eclipses of 2031–2034

Template:Lunar eclipse set 2031-2034

Saros 112

Template:Lunar Saros series 112

Metonic series

Template:Metonic lunar eclipse 2031-2088

Tritos series

Template:Lunar Tritos series July 2009

Inex series

Template:Lunar Inex series May 2002

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two partial solar eclipses of Solar Saros 119.

April 30, 2022 May 11, 2040
File:SE2022Apr30P.png File:SE2040May11P.png

See also

Notes

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  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

Template:Lunar eclipses