Solar eclipse of June 10, 2021

An annular solar eclipse occurred on Thursday, June 10, 2021, when the Moon passed between Earth and the Sun, thereby partly obscuring the image of the Sun for a viewer on Earth.[1][2][3] During the eclipse, the Moon's apparent diameter was smaller than the Sun's, so it caused the Sun to look like an annulus. 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]

Solar eclipse of June 10, 2021
Partial from Halifax, Canada
Map
Type of eclipse
NatureAnnular
Gamma0.9152
Magnitude0.9435
Maximum eclipse
Duration231 s (3 min 51 s)
Coordinates80°48′N 66°48′W / 80.8°N 66.8°W / 80.8; -66.8
Max. width of band527 km (327 mi)
Times (UTC)
Greatest eclipse10:43:07
References
Saros147 (23 of 80)
Catalog # (SE5000)9555

Path

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

Related eclipses

Other eclipses in 2021

Tzolkinex

Half-saros cycle

Tritos

Triad

Solar eclipses of 2018–2021

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
Ascending node Descending node
SarosMapGammaSarosMapGamma
117

Partial from Melbourne, Australia
2018 July 13

Partial
−1.35423122

Partial from Nakhodka, Russia
2019 January 6

Partial
1.14174
127

La Serena, Chile
2019 July 2

Total
−0.64656132

Jaffna, Sri Lanka
2019 December 26

Annular
0.41351
137

Beigang, Yunlin, Taiwan
2020 June 21

Annular
0.12090142

Gorbea, Chile
2020 December 14

Total
−0.29394
147

Partial from Halifax, Canada
2021 June 10

Annular
0.91516152

From HMS Protector off South Georgia
2021 December 4

Total
−0.95261

Saros 147

Solar saros 147, repeating every about 18 years and 11 days, contains 80 events. The series started with a partial solar eclipse on October 12, 1624. It has annular eclipses from May 31, 2003, to July 31, 2706. There are no total eclipses in this series. The series ends at member 80 as a partial eclipse on February 24, 3049. The longest annular eclipse will be on November 21, 2291, at 9 minutes and 41 seconds.[9]

Series members 17–27 occur between 1901 and 2100:
171819

April 6, 1913

April 18, 1931

April 28, 1949
202122

May 9, 1967

May 19, 1985

May 31, 2003
232425

June 10, 2021

June 21, 2039

July 1, 2057
2627

July 13, 2075

July 23, 2093

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.

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

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

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 10–11March 27–29January 15–16November 3August 21–22
117119121123125

June 10, 1964

March 28, 1968

January 16, 1972

November 3, 1975

August 22, 1979
127129131133135

June 11, 1983

March 29, 1987

January 15, 1991

November 3, 1994

August 22, 1998
137139141143145

June 10, 2002

March 29, 2006

January 15, 2010

November 3, 2013

August 21, 2017
147149151153155

June 10, 2021

March 29, 2025

January 14, 2029

November 3, 2032

August 21, 2036

References

External links