August 2036 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 Thursday, August 7, 2036,[1] with an umbral magnitude of 1.4556. 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 only about 11 hours after apogee (on August 6, 2036, at 16:00 UTC), the Moon's apparent diameter will be smaller.[2]

This is the last central lunar eclipse of Saros cycle 129.

Visibility

The eclipse will be completely visible over South America and west Africa, seen rising over much of North America and the eastern Pacific Ocean and setting over Africa, Europe, and west, central, and south Asia.[3]

File:Lunar eclipse from moon-2036Aug07.png File:Lunar eclipse chart close-2036Aug07.png

Eclipse details

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

August 7, 2036 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.52786
Umbral Magnitude 1.45557
Gamma 0.20044
Sun Right Ascension 09h10m39.1s
Sun Declination +16°16'20.8"
Sun Semi-Diameter 15'46.3"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 21h10m30.3s
Moon Declination -16°05'44.3"
Moon Semi-Diameter 14'42.5"
Moon Equatorial Horizontal Parallax 0°53'58.8"
ΔT 77.2 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 July–August 2036
July 23
Ascending node (new moon)
August 7
Descending node (full moon)
August 21
Ascending node (new moon)
File:SE2036Jul23P.png File:Lunar eclipse chart close-2036Aug07.png File:SE2036Aug21P.png
Partial solar eclipse
Solar Saros 117
Total lunar eclipse
Lunar Saros 129
Partial solar eclipse
Solar Saros 155

Related eclipses

Eclipses in 2036

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 129

Inex

Triad

Lunar eclipses of 2035–2038

Template:Lunar eclipse set 2035-2038

Saros 129

Template:Lunar Saros series 129

Tritos series

Template:Lunar Tritos series November 2003

Inex series

Template:Lunar Inex series August 2007

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 total solar eclipses of Solar Saros 136.

August 2, 2027 August 12, 2045
File:SE2027Aug02T.png File:SE2045Aug12T.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