Solar eclipse of May 20, 2050

Last updated

Solar eclipse of May 20, 2050
SE2050May20H.png
Map
Type of eclipse
NatureHybrid
Gamma −0.8688
Magnitude 1.0038
Maximum eclipse
Duration21 s (0 min 21 s)
Coordinates 40°06′S123°42′W / 40.1°S 123.7°W / -40.1; -123.7
Max. width of band27 km (17 mi)
Times (UTC)
Greatest eclipse20:42:50
References
Saros 148 (23 of 75)
Catalog # (SE5000) 9619

A total solar eclipse will occur at the Moon's descending node of orbit on Friday, May 20, 2050, with a magnitude of 1.0038. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Contents

This hybrid eclipse is notable in that it does not hit land anywhere on Earth.

Eclipses in 2050

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 148

Inex

Triad

Solar eclipses of 2047–2050

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [1]

The partial solar eclipses on January 26, 2047 and July 22, 2047 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2047 to 2050
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 June 23, 2047
SE2047Jun23P.png
Partial
1.3766123 December 16, 2047
SE2047Dec16P.png
Partial
−1.0661
128 June 11, 2048
SE2048Jun11A.png
Annular
0.6468133 December 5, 2048
SE2048Dec05T.png
Total
−0.3973
138 May 31, 2049
SE2049May31A.png
Annular
−0.1187143 November 25, 2049
SE2049Nov25H.png
Hybrid
0.2943
148 May 20, 2050
SE2050May20H.png
Hybrid
−0.8688153 November 14, 2050
SE2050Nov14P.png
Partial
1.0447

Saros 148

This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. Its 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.

The longest duration of annularity will be produced by member 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit. [2]

Series members 10–31 occur between 1801 and 2200:
101112
SE1815Dec30P.gif
December 30, 1815
SE1834Jan09P.gif
January 9, 1834
SE1852Jan21P.gif
January 21, 1852
131415
SE1870Jan31P.gif
January 31, 1870
SE1888Feb11P.gif
February 11, 1888
SE1906Feb23P.png
February 23, 1906
161718
SE1924Mar05P.png
March 5, 1924
SE1942Mar16P.png
March 16, 1942
SE1960Mar27P.png
March 27, 1960
192021
SE1978Apr07P.png
April 7, 1978
SE1996Apr17P.png
April 17, 1996
SE2014Apr29A.png
April 29, 2014
222324
SE2032May09A.png
May 9, 2032
SE2050May20H.png
May 20, 2050
SE2068May31T.png
May 31, 2068
252627
SE2086Jun11T.png
June 11, 2086
Saros148 26van75 SE2104Jun22T.jpg
June 22, 2104
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
282930
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
SE2158Jul25T.png
July 25, 2158
Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
31
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

21 eclipse events between May 21, 1993 and May 20, 2069
May 20–21March 9December 25–26October 13–14August 1–2
118120122124126
SE1993May21P.png
May 21, 1993
SE1997Mar09T.png
March 9, 1997
SE2000Dec25P.png
December 25, 2000
SE2004Oct14P.png
October 14, 2004
SE2008Aug01T.png
August 1, 2008
128130132134136
SE2012May20A.png
May 20, 2012
SE2016Mar09T.png
March 9, 2016
SE2019Dec26A.png
December 26, 2019
SE2023Oct14A.png
October 14, 2023
SE2027Aug02T.png
August 2, 2027
138140142144146
SE2031May21A.png
May 21, 2031
SE2035Mar09A.png
March 9, 2035
SE2038Dec26T.png
December 26, 2038
SE2042Oct14A.png
October 14, 2042
SE2046Aug02T.png
August 2, 2046
148150152154156
SE2050May20H.png
May 20, 2050
SE2054Mar09P.png
March 9, 2054
SE2057Dec26T.png
December 26, 2057
SE2061Oct13A.png
October 13, 2061
SE2065Aug02P.png
August 2, 2065
158
SE2069May20P.png
May 20, 2069

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1810Apr04A.gif
April 4, 1810
(Saros 126)
SE1821Mar04T.gif
March 4, 1821
(Saros 127)
SE1832Feb01A.gif
February 1, 1832
(Saros 128)
SE1842Dec31A.gif
December 31, 1842
(Saros 129)
SE1853Nov30T.png
November 30, 1853
(Saros 130)
SE1864Oct30A.gif
October 30, 1864
(Saros 131)
SE1875Sep29A.gif
September 29, 1875
(Saros 132)
SE1886Aug29T.png
August 29, 1886
(Saros 133)
SE1897Jul29A.gif
July 29, 1897
(Saros 134)
SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)
SE1930Apr28H.png
April 28, 1930
(Saros 137)
SE1941Mar27A.png
March 27, 1941
(Saros 138)
SE1952Feb25T.png
February 25, 1952
(Saros 139)
SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1973Dec24A.png
December 24, 1973
(Saros 141)
SE1984Nov22T.png
November 22, 1984
(Saros 142)
SE1995Oct24T.png
October 24, 1995
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2017Aug21T.png
August 21, 2017
(Saros 145)
SE2028Jul22T.png
July 22, 2028
(Saros 146)
SE2039Jun21A.png
June 21, 2039
(Saros 147)
SE2050May20H.png
May 20, 2050
(Saros 148)
SE2061Apr20T.png
April 20, 2061
(Saros 149)
SE2072Mar19P.png
March 19, 2072
(Saros 150)
SE2083Feb16P.png
February 16, 2083
(Saros 151)
SE2094Jan16T.png
January 16, 2094
(Saros 152)
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)
SE2115Nov16A.png
November 16, 2115
(Saros 154)
SE2126Oct16T.png
October 16, 2126
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)
Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
(Saros 158)
Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)
Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1818Oct29T.png
October 29, 1818
(Saros 140)
SE1847Oct09A.png
October 9, 1847
(Saros 141)
SE1876Sep17T.png
September 17, 1876
(Saros 142)
SE1905Aug30T.png
August 30, 1905
(Saros 143)
SE1934Aug10A.png
August 10, 1934
(Saros 144)
SE1963Jul20T.png
July 20, 1963
(Saros 145)
SE1992Jun30T.png
June 30, 1992
(Saros 146)
SE2021Jun10A.png
June 10, 2021
(Saros 147)
SE2050May20H.png
May 20, 2050
(Saros 148)
SE2079May01T.png
May 1, 2079
(Saros 149)
Saros150 22van71 SE2108Apr11P.jpg
April 11, 2108
(Saros 150)
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
(Saros 151)
Saros152 21van70 SE2166Mar02T.jpg
March 2, 2166
(Saros 152)
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195
(Saros 153)

Notes

  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.
  2. "NASA - Catalog of Solar Eclipses of Saros 148". eclipse.gsfc.nasa.gov.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of April 17, 1996</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Wednesday, April 17, 1996, with a magnitude of 0.8799. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of May 31, 2049</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, May 31, 2049, with a magnitude of 0.9631. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of March 29, 2025</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon’s ascending node of orbit on Saturday, March 29, 2025, with a magnitude of 0.9376. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of September 11, 1988</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, September 11, 1988, with a magnitude of 0.9377. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible in southeastern Somalia, the Indian Ocean and Macquarie Island of Australia.

<span class="mw-page-title-main">Solar eclipse of May 9, 1967</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, May 9, 1967, with a magnitude of 0.7201. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of January 25, 1963</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, January 25, 1963, with a magnitude of 0.9951. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity crossed Chile, Argentina, South Africa, southern Basutoland and Malagasy Republic. Occurring 3.7 days before perigee, the Moon's apparent diameter was larger. The moon was 374,860 km from the Earth.

<span class="mw-page-title-main">Solar eclipse of March 27, 1960</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 27, 1960, with a magnitude of 0.7058. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This eclipse was observable from parts of the Antarctic Ocean and Indian Ocean.

<span class="mw-page-title-main">Solar eclipse of April 30, 2041</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, April 30, 2041, with a magnitude of 1.0189. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of October 25, 2041</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, October 25, 2041, with a magnitude of 0.9467. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of November 14, 2050</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 14, 2050, with a magnitude of 0.8874. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of November 25, 2049</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, November 25, 2049, with a magnitude of 1.0057. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of September 22, 2052</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, September 22, 2052, with a magnitude of 0.9734. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of February 17, 2064</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 17, 2064, with a magnitude of 0.9262. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of July 13, 2075</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, July 13, 2075, with a magnitude of 0.9467. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometers wide.

<span class="mw-page-title-main">Solar eclipse of October 24, 2079</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 24, 2079, with a magnitude of 0.9484. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of March 21, 2099</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, March 21, 2099, with a magnitude of 0.93. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of March 10, 2100</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit between Wednesday, March 10 and Thursday, March 11, 2100, with a magnitude of 0.9338. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometers wide. The path of annularity will move from Indonesia at sunrise, over the islands of Hawaii and Maui around noon, and through the northwestern United States at sunset.

<span class="mw-page-title-main">Solar eclipse of July 3, 2084</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, July 3, 2084, with a magnitude of 0.9421. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometers wide.

<span class="mw-page-title-main">Solar eclipse of August 10, 1934</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, August 10, 1934, with a magnitude of 0.9436. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of February 23, 1906</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Friday, February 23, 1906, with a magnitude of 0.5386. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

References