Solar eclipse of June 21, 2039

An annular solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, June 21, 2039, with a magnitude of 0.9454. 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 start only a few hours after the northern solstice and most of the path will go across areas with midnight sun. For mainland Norway, Sweden and Belarus, it will be the first central solar eclipse since June 1954.

Solar eclipse of June 21, 2039
Map
Type of eclipse
NatureAnnular
Gamma0.8312
Magnitude0.9454
Maximum eclipse
Duration245 s (4 min 5 s)
Coordinates78.9°N 102.1°W / 78.9; -102.1
Max. width of band365 km (227 mi)
Times (UTC)
Greatest eclipse17:12:54
References
Saros147 (24 of 80)
Catalog # (SE5000)9595

Images


Animated path

Eclipses of 2039

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 2036–2039

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]

Note: Partial solar eclipses on February 27, 2036 and August 21, 2036 occur on the previod lunar year eclipse set.

Solar eclipse series sets from 2036 to 2039
Ascending node   Descending node
117July 23, 2036

Partial		 122January 16, 2037

Partial
127July 13, 2037

Total		 132January 5, 2038

Annular
137July 2, 2038

Annular		 142December 26, 2038

Total
147June 21, 2039

Annular		 152December 15, 2039

Total

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.[2]

Series members 17–27 occur between 1901 and 2100:
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

July 13, 2075
July 23, 2093

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 between June 21, 1982, and June 21, 2058
June 21 April 8–9 January 26 November 13–14 September 1–2
107 109 111 113 115
June 21, 1963 April 9, 1967 January 26, 1971 November 14, 1974 September 2, 1978
117 119 121 123 125

June 21, 1982
April 9, 1986
January 26, 1990
November 13, 1993
September 2, 1997
127 129 131 133 135

June 21, 2001
April 8, 2005
January 26, 2009
November 13, 2012
September 1, 2016
137 139 141 143 145

June 21, 2020
April 8, 2024
January 26, 2028
November 14, 2031
September 2, 2035
147 149 151 153 155

June 21, 2039
April 9, 2043
January 26, 2047
November 14, 2050
September 2, 2054
157

June 21, 2058

References
  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
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