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April 2052 lunar eclipse

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April 2052 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateApril 14, 2052
Gamma1.0628
Magnitude−0.1294
Saros cycle142 (20 of 73)
Penumbral276 minutes, 0 seconds
Contacts (UTC)
P123:58:26
Greatest2:16:28
P44:34:26

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, April 14, 2052,[1] with an umbral magnitude of −0.1294. 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 2.4 days before apogee (on April 16, 2052, at 13:00 UTC), the Moon's apparent diameter will be smaller.[2]

Visibility

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

Eclipse details

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

April 14, 2052 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.94777
Umbral Magnitude −0.12938
Gamma 1.06290
Sun Right Ascension 01h32m05.6s
Sun Declination +09°37'10.9"
Sun Semi-Diameter 15'56.9"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 13h33m09.3s
Moon Declination -08°41'36.6"
Moon Semi-Diameter 14'48.3"
Moon Equatorial Horizontal Parallax 0°54'20.2"
ΔT 86.6 s

Eclipse season

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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 2052
March 30
Descending node (new moon)
April 14
Ascending node (full moon)
Total solar eclipse
Solar Saros 130
Penumbral lunar eclipse
Lunar Saros 142
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Eclipses in 2052

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 142

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Inex

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Triad

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Lunar eclipses of 2049–2052

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Lunar eclipse series sets from 2049-2052
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
112 2049 May 17
Penumbral
117 2049 Nov 09
Penumbral
122 2050 May 06
Total
127 2050 Oct 30
Total
132 2051 Apr 26
Total
137 2051 Oct 19
Total
142 2052 Apr 14
Penumbral
147 2052 Oct 08
Partial
Last set 2049 Jun 15 Last set 2048 Dec 20
Next set 2053 Mar 04 Next set 2053 Aug 29

Half-Saros cycle

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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 149.

April 9, 2043 April 20, 2061

See also

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Notes

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  1. ^ "April 13–14, 2052 Penumbral Lunar Eclipse". timeanddate. Retrieved 12 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 December 2024.
  3. ^ "Penumbral Lunar Eclipse of 2052 Apr 14" (PDF). NASA. Retrieved 12 December 2024.
  4. ^ "Penumbral Lunar Eclipse of 2052 Apr 14". EclipseWise.com. Retrieved 12 December 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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