Solar eclipse of June 10, 2021

Solar eclipse of June 10, 2021
Solar eclipse of June 10, 2021
	Partial from Halifax, Canada
	Map
Type of eclipse
Nature	Annular
Gamma	0.9152
Magnitude	0.9435
Maximum eclipse
Duration	231 s (3 min 51 s)
Coordinates	80°48′N 66°48′W / 80.8°N 66.8°W
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 occurred at the Moon’s ascending node of orbit on Thursday, June 10, 2021,^[1]^[2]^[3] with a magnitude of 0.9435. An annular solar eclipse is a solar eclipse whose presentation looks like a ring, or annulus; it occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most, but not all, of the Sun's light. The annular eclipse was visible from parts of northeastern Canada, Greenland, the Arctic Ocean (passing over the North Pole),^[4] and the Russian Far East, whilst the eclipse appeared partial from a region thousands of kilometres wide, which included northeastern North America, most of Europe, and northern Asia.^[5]

Path[edit]

Animated image showing the path of the eclipse shadows.

The annular eclipse started at 09:55 UTC for 3 minutes 37 seconds along the northern shore of Lake Superior in Ontario, Canada. The path of the antumbral shadow then headed across Hudson Bay through northwestern Quebec and the Hudson Strait to Baffin Island in Nunavut, where the town of Iqaluit saw 3 minutes and 5 seconds of annularity. After this, it then travelled across Baffin Bay and along the northwestern coast of Greenland, where the point of greatest eclipse occurred at 10:41 UTC in Nares Strait for 3 minutes 51 seconds. The shadow then crossed Ellesmere Island and the Arctic Ocean, passing over the North Pole (which was located away from the central line of the eclipse but saw 2 minutes and 36 seconds of annularity), before heading south towards northeastern Siberia, where the city of Srednekolymsk saw 3 minutes and 35 seconds of annularity at 11:27 UTC. Shortly afterwards, the central line of the annular eclipse ended at 11:29 UTC.^[6]^[7]

Gallery[edit]

Eclipse over the Statue of Liberty in New York City
Montpelier, Vermont, 9:33 UTC
Killingly, Connecticut, 9:35 UTC
Lewes, Delaware, 9:42 UTC
Arlington, Virginia, 9:56 UTC
Logroño, Spain, 10:10 UTC
Projection from Prague, Czechia, 10:24 UTC
Haut-Doubs [fr], France, 10:26 UTC
Projection through leaves in Woerden, Netherlands, 10:30 UTC
Brastad, Sweden, 10:32 UTC
Lino Lakes, Minnesota, 10:33 UTC
Berlin, Germany, 10:38 UTC
Beccles, England, 10:48 UTC
Huittinen, Finland, 11:00 UTC
Sumburgh, Shetland, 11:04 UTC
Saint Petersburg, Russia, 11:09 UTC
Partial from Tõrva, Estonia
Petrozavodsk, Russia, 11:27 UTC, Coronado telescope
Timelapse-video from Akademgorodok, Novosibirsk, Russia
Timelapse-video from Kharbalakh, Yakutia, Russia

Related eclipses[edit]

Solar eclipses of 2018–2021[edit]

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.^[8]

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

Solar eclipse series sets from 2018 to 2021
Saros	Map	Gamma	Saros	Map	Gamma
Ascending node			Descending node
117 Partial from Melbourne, Australia	2018 July 13 Partial	−1.35423	122 Partial from Nakhodka, Russia	2019 January 6 Partial	1.14174
127 La Serena, Chile	2019 July 2 Total	−0.64656	132 Jaffna, Sri Lanka	2019 December 26 Annular	0.41351
137 Beigang, Yunlin, Taiwan	2020 June 21 Annular	0.12090	142 Gorbea, Chile	2020 December 14 Total	−0.29394
147 Partial from Halifax, Canada	2021 June 10 Annular	0.91516	152 From HMS Protector off South Georgia	2021 December 4 Total	−0.95261

Saros 147[edit]

This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit.^[9]

Series members 11–32 occur between 1801 and 2200:
11	12	13
January 30, 1805	February 11, 1823	February 21, 1841
14	15	16
March 4, 1859	March 15, 1877	March 26, 1895
17	18	19
April 6, 1913	April 18, 1931	April 28, 1949
20	21	22
May 9, 1967	May 19, 1985	May 31, 2003
23	24	25
June 10, 2021	June 21, 2039	July 1, 2057
26	27	28
July 13, 2075	July 23, 2093	August 4, 2111
29	30	31
August 15, 2129	August 26, 2147	September 5, 2165
32
September 16, 2183

Inex series[edit]

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. In the 19th century:

Solar saros 140: total solar eclipse of October 29, 1818
Solar saros 141: annular solar eclipse of October 9, 1847
Solar saros 142: total solar eclipse of September 17, 1876

Inex series members between 1901 and 2100:
August 30, 1905 (Saros 143)	August 10, 1934 (Saros 144)	July 20, 1963 (Saros 145)
June 30, 1992 (Saros 146)	June 10, 2021 (Saros 147)	May 20, 2050 (Saros 148)
May 1, 2079 (Saros 149)		1

In the 22nd century:

Solar Saros 150: Partial solar eclipse of April 11, 2108
Solar Saros 151: Annular solar eclwssipse of March 21, 2137

Solar Saros 152: Total solar eclipse of March 2, 2166
Solar Saros 153: Annular solar eclipse of February 10, 2195

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Metonic series[edit]

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 ascending node.

21 eclipse events, progressing from south to north 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
June 10, 1964	March 28, 1968	January 16, 1972	November 3, 1975	August 22, 1979
127	129	131	133	135
June 11, 1983	March 29, 1987	January 15, 1991	November 3, 1994	August 22, 1998
137	139	141	143	145
June 10, 2002	March 29, 2006	January 15, 2010	November 3, 2013	August 21, 2017
147	149	151	153	155
June 10, 2021	March 29, 2025	January 14, 2029	November 3, 2032	August 21, 2036