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Solar eclipse of September 13, 2015

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Solar eclipse of September 13, 2015
From the Solar Dynamics Observatory
Map
Type of eclipse
NaturePartial
Gamma−1.1004
Magnitude0.7875
Maximum eclipse
Coordinates72°06′S 2°18′W / 72.1°S 2.3°W / -72.1; -2.3
Times (UTC)
Greatest eclipse6:55:19
References
Saros125 (54 of 73)
Catalog # (SE5000)9542

A partial solar eclipse occurred at the Moon's ascending node of orbit on Sunday, September 13, 2015,[1][2][3] with a magnitude of 0.7875. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Images

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Animated path

View from center of sun
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Eclipses in 2015

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 125

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Inex

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Triad

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Solar eclipses of 2015–2018

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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.[4]

The partial solar eclipse on July 13, 2018 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 2015 to 2018
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120

Totality in Longyearbyen, Svalbard
March 20, 2015

Total
0.94536 125

Solar Dynamics Observatory

September 13, 2015

Partial
−1.10039
130

Balikpapan, Indonesia
March 9, 2016

Total
0.26092 135

Annularity in L'Étang-Salé, Réunion
September 1, 2016

Annular
−0.33301
140

Partial from Buenos Aires, Argentina
February 26, 2017

Annular
−0.45780 145

Totality in Madras, OR, USA
August 21, 2017

Total
0.43671
150

Partial in Olivos, Buenos Aires, Argentina
February 15, 2018

Partial
−1.21163 155

Partial in Huittinen, Finland
August 11, 2018

Partial
1.14758

Saros 125

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This eclipse is a part of Saros series 125, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on February 4, 1060. It contains total eclipses from June 13, 1276 through July 16, 1330; hybrid eclipses on July 26, 1348 and August 7, 1366; and annular eclipses from August 17, 1384 through August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. 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 totality was produced by member 14 at 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was produced by member 48 at 7 minutes, 23 seconds on July 10, 1907. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]

Series members 43–64 occur between 1801 and 2200:
43 44 45

May 16, 1817

May 27, 1835

June 6, 1853
46 47 48

June 18, 1871

June 28, 1889

July 10, 1907
49 50 51

July 20, 1925

August 1, 1943

August 11, 1961
52 53 54

August 22, 1979

September 2, 1997

September 13, 2015
55 56 57

September 23, 2033

October 4, 2051

October 15, 2069
58 59 60

October 26, 2087

November 6, 2105

November 18, 2123
61 62 63

November 28, 2141

December 9, 2159

December 20, 2177
64

December 31, 2195

Metonic series

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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 July 1, 2000 and July 1, 2076
July 1–2 April 19–20 February 5–7 November 24–25 September 12–13
117 119 121 123 125

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157

July 1, 2076

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

March 25, 1819
(Saros 107)

February 23, 1830
(Saros 108)

January 22, 1841
(Saros 109)

November 21, 1862
(Saros 111)

August 20, 1895
(Saros 114)

July 21, 1906
(Saros 115)

June 19, 1917
(Saros 116)

May 19, 1928
(Saros 117)

April 19, 1939
(Saros 118)

March 18, 1950
(Saros 119)

February 15, 1961
(Saros 120)

January 16, 1972
(Saros 121)

December 15, 1982
(Saros 122)

November 13, 1993
(Saros 123)

October 14, 2004
(Saros 124)

September 13, 2015
(Saros 125)

August 12, 2026
(Saros 126)

July 13, 2037
(Saros 127)

June 11, 2048
(Saros 128)

May 11, 2059
(Saros 129)

April 11, 2070
(Saros 130)

March 10, 2081
(Saros 131)

February 7, 2092
(Saros 132)

January 8, 2103
(Saros 133)

December 8, 2113
(Saros 134)

November 6, 2124
(Saros 135)

October 7, 2135
(Saros 136)

September 6, 2146
(Saros 137)

August 5, 2157
(Saros 138)

July 5, 2168
(Saros 139)

June 5, 2179
(Saros 140)

May 4, 2190
(Saros 141)

Inex series

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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.

Series members between 1801 and 2200

February 1, 1813
(Saros 118)

January 11, 1842
(Saros 119)

December 22, 1870
(Saros 120)

December 3, 1899
(Saros 121)

November 12, 1928
(Saros 122)

October 23, 1957
(Saros 123)

October 3, 1986
(Saros 124)

September 13, 2015
(Saros 125)

August 23, 2044
(Saros 126)

August 3, 2073
(Saros 127)

July 15, 2102
(Saros 128)

June 25, 2131
(Saros 129)

June 4, 2160
(Saros 130)

May 15, 2189
(Saros 131)

References

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  1. ^ Orwig, Jessica. "A NASA video shows what a total lunar eclipse looks like from the moon, and it's mind-blowing". Business Insider.
  2. ^ European Space Agency. "Image: Proba-2 captures partial solar eclipse". phys.org.
  3. ^ Wall, Mike (September 12, 2015). "Watch Sunday's Partial Solar Eclipse Live in Slooh Webcast". Space.com.
  4. ^ 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.
  5. ^ "NASA - Catalog of Solar Eclipses of Saros 125". eclipse.gsfc.nasa.gov.
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