May 2040 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, May 26, 2040,[1] with an umbral magnitude of 1.5365. 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 1.4 days before perigee (on May 27, 2040, at 22:25 UTC), the Moon's apparent diameter will be larger.[2]

This is the second central lunar eclipse of Saros series 131. Since this lunar event will occur near perigee, it will be referred to as a "super flower blood moon" or "super blood moon", though not quite as close to Earth as the eclipse of May 26, 2021.

Visibility

The eclipse will be completely visible over Antarctica, Australia, and the Pacific Ocean, seen rising over east and south Asia and setting over North and South America.[3]

File:Lunar eclipse from moon-2040May26.png File:Lunar eclipse chart close-2040May26.png

Eclipse details

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

May 26, 2040 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.49551
Umbral Magnitude 1.53646
Gamma −0.18720
Sun Right Ascension 04h15m46.6s
Sun Declination +21°16'35.1"
Sun Semi-Diameter 15'47.2"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 16h15m33.4s
Moon Declination -21°27'28.2"
Moon Semi-Diameter 16'27.7"
Moon Equatorial Horizontal Parallax 1°00'24.9"
ΔT 79.3 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.

Eclipse season of May 2040
May 11
Ascending node (new moon)
May 26
Descending node (full moon)
File:SE2040May11P.png File:Lunar eclipse chart close-2040May26.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131

Related eclipses

Eclipses in 2040

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 131

Inex

Triad

Lunar eclipses of 2038–2042

Template:Lunar eclipse set 2038-2042

Saros 131

Template:Lunar Saros series 131

Tritos series

Template:Lunar Tritos series August 2007

Inex series

Template:Lunar Inex series June 2011

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 annular solar eclipses of Solar Saros 138.

May 21, 2031 May 31, 2049
File:SE2031May21A.png File:SE2049May31A.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

References

  • Bao-Lin Liu, Canon of Lunar Eclipses 1500 B.C.-A.D. 3000, 1992

Template:Lunar eclipses