Solar eclipse of June 10, 2021

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Solar eclipse of June 10, 2021
SE2021Jun10A.png
Map
Type of eclipse
Nature Annular
Gamma 0.9152
Magnitude 0.9435
Maximum eclipse
Duration 231 sec (3 m 51 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 527 km (327 mi)
Times (UTC)
Greatest eclipse 10:43:07
References
Saros 147 (23 of 80)
Catalog # (SE5000) 9555

An annular solar eclipse will occur on June 10, 2021. 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. This eclipse will be unusual as the path of the total eclipse will move to the north east, then north, north west, west, south west, south, and finally south east across the Arctic, while most eclipse paths move west to east. This reversal is only possible in polar regions.

While the eclipse is visible primarily in the relatively unpopulated area near the Arctic Circle, in the northeastern United States and Canada, the sun will be partially eclipsed at sunrise.

Images

File:SE2021Jun10A.gif
Animated path

Related eclipses

Solar eclipses of 2018-2021

Each member 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.

Note: Partial solar eclipses on February 15, 2018, and August 11, 2018, occur during the previous semester series.

Solar eclipse series sets from 2018–2021
Ascending node   Descending node
117 July 13, 2018
SE2018Jul13P.png
Partial
122 January 6, 2019
SE2019Jan06P.png
Partial
127 July 2, 2019
SE2019Jul02T.png
Total
132 December 26, 2019
SE2019Dec26A.png
Annular
137 June 21, 2020
SE2020Jun21A.png
Annular
142 December 14, 2020
SE2020Dec14T.png
Total
147 June 10, 2021
SE2021Jun10A.png
Annular
152 December 4, 2021
SE2021Dec04T.png
Total

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).

This series has 20 eclipse events between June 10, 1964 and August 21, 2036.

June 10–11 March 27–29 January 15–16 November 3 August 21–22
117 119 121 123 125
150px
June 10, 1964
SE1968Mar28P.png
March 28, 1968
SE1972Jan16A.png
January 16, 1972
SE1975Nov03P.png
November 3, 1975
SE1979Aug22A.png
August 22, 1979
127 129 131 133 135
SE1983Jun11T.png
June 11, 1983
SE1987Mar29H.png
March 29, 1987
SE1991Jan15A.png
January 15, 1991
SE1994Nov03T.png
November 3, 1994
SE1998Aug22A.png
August 22, 1998
137 139 141 143 145
SE2002Jun10A.png
June 10, 2002
SE2006Mar29T.png
March 29, 2006
SE2010Jan15A.png
January 15, 2010
SE2013Nov03H.png
November 3, 2013
SE2017Aug21T.png
August 21, 2017
147 149 151 153 155
SE2021Jun10A.png
June 10, 2021
SE2025Mar29P.png
March 29, 2025
SE2029Jan14P.png
January 14, 2029
SE2032Nov03P.png
November 3, 2032
SE2036Aug21P.png
August 21, 2036

Notes

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References


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