April 2033 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A total lunar eclipse will occur at the Moon’s ascending node of orbit on Thursday, April 14, 2033,[1] with an umbral magnitude of 1.0955. 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 2.9 days before apogee (on April 11, 2033, at 22:30 UTC), the Moon's apparent diameter will be smaller.[2]

This lunar eclipse is the third of a tetrad, with four total lunar eclipses in series, the others being on April 25, 2032; October 18, 2032; and October 8, 2033.

Visibility

The eclipse will be completely visible over east Africa, most of Asia, and western Australia, seen rising over west and central Africa, Europe, and eastern South America and setting over northeast Asia and Australia.[3]

File:Lunar eclipse from moon-2033Apr14.png File:Lunar eclipse chart close-2033Apr14.png

Eclipse details

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

April 14, 2033 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.17223
Umbral Magnitude 1.09553
Gamma 0.39543
Sun Right Ascension 01h33m13.7s
Sun Declination +09°43'50.2"
Sun Semi-Diameter 15'56.7"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 13h33m37.2s
Moon Declination -09°23'08.7"
Moon Semi-Diameter 14'48.5"
Moon Equatorial Horizontal Parallax 0°54'21.0"
ΔT 75.5 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.

Eclipse season of March–April 2033
March 30
Descending node (new moon)
April 14
Ascending node (full moon)
File:SE2033Mar30T.png File:Lunar eclipse chart close-2033Apr14.png
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132

Related eclipses

Eclipses in 2033

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 132

Inex

Triad

Lunar eclipses of 2031–2034

Template:Lunar eclipse set 2031-2034

Saros 132

Template:Lunar Saros series 132

Tritos series

Template:Lunar Tritos series July 2000

Inex series

Template:Lunar Inex series May 2004

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 139.

April 8, 2024 April 20, 2042
File:SE2024Apr08T.png File:SE2042Apr20T.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