April 2032 lunar eclipse

A total lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, April 25, 2032,[1] with an umbral magnitude of 1.1925. 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. The Moon's apparent diameter will be near the average diameter because it will occur 6.7 days after apogee (on April 18, 2032, at 23:00 UTC) and 8.1 days before perigee (on May 3, 2032, at 16:45 UTC).[2]

April 2032 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateApril 25, 2032
Gamma−0.3558
Magnitude1.1925
Saros cycle122 (57 of 75)
Totality65 minutes, 32 seconds
Partiality211 minutes, 11 seconds
Penumbral342 minutes, 26 seconds
Contacts (UTC)
P112:22:16
U113:27:58
U214:40:47
Greatest15:14:51
U315:46:19
U416:59:09
P418:04:42

This lunar eclipse is the first of a tetrad, with four total lunar eclipses in series, the others being on October 18, 2032; April 14, 2033; and October 8, 2033.

Visibility

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The eclipse will be completely visible over east Asia, Australia, and Antarctica, seen rising over east and central Africa, eastern Europe, and west and central Asia and setting over the eastern Pacific Ocean and western North America.[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 25, 2032 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.22037
Umbral Magnitude 1.19249
Gamma −0.35578
Sun Right Ascension 02h14m38.2s
Sun Declination 13°30'28.8"
Sun Semi-Diameter 15'53.8"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 14h14m18.6s
Moon Declination -13°50'06.1"
Moon Semi-Diameter 15'27.9"
Moon Equatorial Horizontal Parallax 0°56'45.4"
ΔT 75.0 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 April–May 2032
April 25
Ascending node (full moon)
May 9
Descending node (new moon)
   
Total lunar eclipse
Lunar Saros 122
Annular solar eclipse
Solar Saros 148
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Eclipses in 2032

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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 122

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Inex

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Triad

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Lunar eclipses of 2031–2034

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Lunar eclipse series sets from 2031-2034
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
112 2031 May 07
 
Penumbral
 
117 2031 Oct 30
 
Penumbral
 
122 2032 Apr 25
 
Total
 
127 2032 Oct 18
 
Total
 
132 2033 Apr 14
 
Total
 
137 2033 Oct 08
 
Total
 
142 2034 Apr 03
 
Penumbral
 
147 2034 Sep 28
 
Partial
 
Last set 2031 Jun 05 Last set 2030 Dec 09
Next set 2035 Feb 22 Next set 2035 Aug 19

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 partial solar eclipses of Solar Saros 129.

April 20, 2023 April 30, 2041
   

See also

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Notes

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  1. ^ "April 25–26, 2032 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 21 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 21 November 2024.
  3. ^ "Total Lunar Eclipse of 2032 Apr 25" (PDF). NASA. Retrieved 21 November 2024.
  4. ^ "Total Lunar Eclipse of 2032 Apr 25". EclipseWise.com. Retrieved 21 November 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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