Solar eclipse of July 13, 2037

Total eclipse
24°48′S 139°06′E / 24.8°S 139.1°E / -24.8; 139.1Max. width of band201 km (125 mi)Times (UTC)Greatest eclipse2:40:36ReferencesSaros127 (59 of 82)Catalog # (SE5000)9591

A total solar eclipse will occur on July 13, 2037. 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. Totality will pass through the centre of Brisbane and the Gold Coast, as well as Geraldton, Western Australia

Images


Animated path

Related eclipses

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
117 July 23, 2036

Partial
122 January 16, 2037

Partial
127 July 13, 2037

Total
132 January 5, 2038

Annular
137 July 2, 2038

Annular
142 December 26, 2038

Total
147 June 21, 2039

Annular
152 December 15, 2039

Total

Saros 127

It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular eclipses in this series. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occurs at the Moon’s ascending node.[2]

Series members 52–68 occur between 1901 and 2200
52 53 54

April 28, 1911

May 9, 1929

May 20, 1947
55 56 57

May 30, 1965

June 11, 1983

June 21, 2001
58 59 60

July 2, 2019

July 13, 2037

July 24, 2055
61 62 63

August 3, 2073

August 15, 2091
August 26, 2109 (Partial)
64 65 66
September 6, 2127 (Partial September 16, 2145 (Partial) September 28, 2163 (Partial)
67 68
October 8, 2181 (Partial) October 19, 2199 (Partial)

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 July 13, 2018 and July 12, 2094
July 12–13 April 30-May 1 February 16–17 December 5–6 September 22–23
117 119 121 123 125

July 13, 2018

April 30, 2022

February 17, 2026

December 5, 2029

September 23, 2033
127 129 131 133 135

July 13, 2037

April 30, 2041

February 16, 2045

December 5, 2048

September 22, 2052
137 139 141 143 145

July 12, 2056

April 30, 2060

February 17, 2064

December 6, 2067

September 23, 2071
147 149 151 153 155

July 13, 2075

May 1, 2079

February 16, 2083

December 6, 2086

September 23, 2090
157

July 12, 2094

References

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements
  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. ^ "Solar Saros series 127". NASA Goddard Space Flight Center. NASA. Retrieved 2 November 2017.
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External links

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