A total lunar eclipse occurred at the Moon’s descending node of orbit on Monday, May 16, 2022,[1] with an umbral magnitude of 1.4155. It was a central lunar eclipse, in which part of the Moon passed 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 about 1.3 days after perigee (on May 17, 2022, at 11:30 UTC), the Moon's apparent diameter was larger.[2]
Total eclipse | |||||||||||||||||
Date | May 16, 2022 | ||||||||||||||||
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Gamma | −0.2532 | ||||||||||||||||
Magnitude | 1.4155 | ||||||||||||||||
Saros cycle | 131 (34 of 72) | ||||||||||||||||
Totality | 84 minutes, 53 seconds | ||||||||||||||||
Partiality | 207 minutes, 14 seconds | ||||||||||||||||
Penumbral | 318 minutes, 40 seconds | ||||||||||||||||
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Because this event occurred near lunar perigee, it was referred to some in media coverage as a "super flower blood moon"[Note 1][3][4][5] and elsewhere as a "super blood moon",[6][7][8] a supermoon that coincides with a total lunar eclipse. This was the longest total lunar eclipse visible from nearly all of North America since August 17, 1989 until the next eclipse on November 8.[9][10]
The eclipse was a dark one with the northern limb of the Moon passing through the center of Earth's shadow. This was the first central eclipse of Lunar Saros 131.
This lunar eclipse was the third of an almost tetrad, with the others being on May 26, 2021 (total); November 19, 2021 (partial); and November 8, 2022 (total).
The eclipse was completely visible over North and South America, seen rising over western North America and the central Pacific Ocean and setting over Europe and Africa.[11]
Visibility map |
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[12]
Parameter | Value |
---|---|
Penumbral Magnitude | 2.37433 |
Umbral Magnitude | 1.41545 |
Gamma | −0.25323 |
Sun Right Ascension | 03h31m49.5s |
Sun Declination | +19°05'13.4" |
Sun Semi-Diameter | 15'49.2" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 15h31m27.8s |
Moon Declination | -19°19'40.4" |
Moon Semi-Diameter | 16'29.9" |
Moon Equatorial Horizontal Parallax | 1°00'33.1" |
ΔT | 70.4 s |
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.
April 30 Ascending node (new moon) |
May 16Descending node (full moon) | |
---|---|---|
Partial solar eclipse Solar Saros 119 |
Total lunar eclipse Lunar Saros 131 |
This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[13]
The penumbral lunar eclipses on January 10, 2020 and July 5, 2020 occur in the previous lunar year eclipse set.
Lunar eclipse series sets from 2020 to 2023 | ||||||||
---|---|---|---|---|---|---|---|---|
Descending node | Ascending node | |||||||
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
111 |
2020 Jun 05 |
Penumbral |
1.2406 | 116 |
2020 Nov 30 |
Penumbral |
−1.1309 | |
121 |
2021 May 26 |
Total |
0.4774 | 126 |
2021 Nov 19 |
Partial |
−0.4553 | |
131 |
2022 May 16 |
Total |
−0.2532 | 136 |
2022 Nov 08 |
Total |
0.2570 | |
141 |
2023 May 05 |
Penumbral |
−1.0350 | 146 |
2023 Oct 28 |
Partial |
0.9472 |
This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 10, 1427. It contains partial eclipses from July 25, 1553 through March 22, 1932; total eclipses from April 2, 1950 through September 3, 2202; and a second set of partial eclipses from September 13, 2220 through April 9, 2563. The series ends at member 72 as a penumbral eclipse on July 7, 2707.
The longest duration of totality will be produced by member 38 at 100 minutes, 36 seconds on June 28, 2094. All eclipses in this series occur at the Moon’s descending node of orbit.[14]
Greatest | First | |||
---|---|---|---|---|
The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds.[15] |
Penumbral | Partial | Total | Central |
1427 May 10 |
1553 Jul 25 |
1950 Apr 02 |
2022 May 16 | |
Last | ||||
Central | Total | Partial | Penumbral | |
2148 Jul 31 |
2202 Sep 03 |
2563 Apr 09 |
2707 Jul 07 |
Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
Series members 22–43 occur between 1801 and 2200: | |||||
---|---|---|---|---|---|
22 | 23 | 24 | |||
1806 Jan 05 | 1824 Jan 16 | 1842 Jan 26 | |||
25 | 26 | 27 | |||
1860 Feb 07 | 1878 Feb 17 | 1896 Feb 28 | |||
28 | 29 | 30 | |||
1914 Mar 12 | 1932 Mar 22 | 1950 Apr 02 | |||
31 | 32 | 33 | |||
1968 Apr 13 | 1986 Apr 24 | 2004 May 04 | |||
34 | 35 | 36 | |||
2022 May 16 | 2040 May 26 | 2058 Jun 06 | |||
37 | 38 | 39 | |||
2076 Jun 17 | 2094 Jun 28 | 2112 Jul 09 | |||
40 | 41 | 42 | |||
2130 Jul 21 | 2148 Jul 31 | 2166 Aug 11 | |||
43 | |||||
2184 Aug 21 | |||||
This eclipse is the third of four Metonic cycle lunar eclipses on the same date, 15–16 May, each separated by 19 years.
The Moon's path through the Earth's shadow near its descending node progresses southward through each sequential eclipse. The second and third are total eclipses.
The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will be in nearly the same location relative to the background stars.
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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).[16] This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.
May 10, 2013 | May 21, 2031 |
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