June 2031 lunar eclipse

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Thursday, June 5, 2031,[1] with an umbral magnitude of −0.8185. 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 only about 20.5 hours before perigee (on June 6, 2031, at 8:10 UTC), the Moon's apparent diameter will be larger.[2]

June 2031 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateJune 5, 2031
Gamma1.4732
Magnitude−0.8185
Saros cycle150 (2 of 71)
Penumbral95 minutes, 33 seconds
Contacts (UTC)
P110:56:16
Greatest11:45:17
P412:31:49

Visibility

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The eclipse will be completely visible over the Pacific Ocean, Australia, and Antarctica, seen rising over east Asia and setting over western North and South 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]

June 5, 2031 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.13062
Umbral Magnitude −0.81845
Gamma 1.47322
Sun Right Ascension 04h53m21.6s
Sun Declination +22°33'01.5"
Sun Semi-Diameter 15'45.9"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 16h53m29.4s
Moon Declination -21°03'14.0"
Moon Semi-Diameter 16'36.6"
Moon Equatorial Horizontal Parallax 1°00'57.7"
ΔT 74.6 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of May–June 2031
May 7
Ascending node (full moon)
May 21
Descending node (new moon)
June 5
Ascending node (full moon)
     
Penumbral lunar eclipse
Lunar Saros 112
Annular solar eclipse
Solar Saros 138
Penumbral lunar eclipse
Lunar Saros 150
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Eclipses in 2031

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Metonic

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Tzolkinex

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Tritos

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Lunar Saros 150

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Inex

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Triad

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Lunar eclipses of 2027–2031

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Lunar eclipse series sets from 2027–2031
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
110 2027 Jul 18
 
Penumbral
 
-1.57589 115 2028 Jan 12
 
Partial
 
0.98177
120 2028 Jul 06
 
Partial
 
-0.79040 125 2028 Dec 31
 
Total
 
0.32583
130 2029 Jun 26
 
Total
 
0.01240 135 2029 Dec 20
 
Total
 
-0.38110
140 2030 Jun 15
 
Partial
 
0.75346 145 2030 Dec 09
 
Penumbral
 
-1.07315
150 2031 Jun 05
 
Penumbral
 
1.47322
Last set 2027 Aug 17 Last set 2027 Feb 20
Next set 2031 May 07 Next set 2031 Oct 30

Saros 150

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This is the first lunar eclipse of Saros series 150.[5] The next occurrence will also be a penumbral eclipse on June 15, 2049.

Partial eclipses in series 150 will occur between 2157 Aug 20 and past the year 3000. Total eclipses will occur between 2572 Apr 29 - 2770 Aug 28.

See also

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Notes

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  1. ^ "June 5, 2031 Penumbral Lunar Eclipse". timeanddate. Retrieved 21 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 21 November 2024.
  3. ^ "Penumbral Lunar Eclipse of 2031 Jun 05" (PDF). NASA. Retrieved 21 November 2024.
  4. ^ "Penumbral Lunar Eclipse of 2031 Jun 05". EclipseWise.com. Retrieved 21 November 2024.
  5. ^ "Lunar Eclipses in Saros Series 150". Hermit Eclipse. Retrieved 30 December 2021.
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