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Solar eclipse of March 20, 2015

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Solar eclipse of March 20, 2015
From Longyearbyen, Svalbard
Map
Type of eclipse
NatureTotal
Gamma0.9454
Magnitude1.0445
Maximum eclipse
Duration167 s (2 min 47 s)
Coordinates64°24′N 6°36′W / 64.4°N 6.6°W / 64.4; -6.6
Max. width of band463 km (288 mi)
Times (UTC)
Greatest eclipse9:46:47
References
Saros120 (61 of 71)
Catalog # (SE5000)9541

A total solar eclipse will occur on Friday March 20, 2015. Template:Total solar eclipse summary

It will have a magnitude of 1.045. The longest duration of totality will be 2 minutes 47 seconds off the coast of the Faroe Islands. It is the last total solar eclipse visible in Europe until the eclipse of August 12, 2026. [1]

At the end of its path, the shadow of the Moon rises from the Earth's surface to space at the north pole. As March 20 is the Northward equinox, the eclipse occurs as the Sun rises at the north pole for the first time in six months.

Images

Closeup animation of shadow in 30 second frames:

Related eclipses

Lunar eclipses

A total lunar eclipse will follow on April 4, 2015, visible over Australia, and the Pacific coast of Asia and North America.

Solar eclipses 2015-2018

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.[2]

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

Longyearbyen, Svalbard
2015 March 20

Total
0.94536 125

Solar Dynamics Observatory

2015 September 13

Partial (south)
−1.10039
130

Balikpapan, Indonesia
2016 March 9

Total
0.26092 135

L'Étang-Salé, Réunion
2016 September 1

Annular
−0.33301
140

Partial from Buenos Aires
2017 February 26

Annular
−0.45780 145

Casper, Wyoming
2017 August 21

Total
0.43671
150

Partial from Olivos, Buenos Aires
2018 February 15

Partial (south)
−1.21163 155

Partial from Huittinen, Finland
2018 August 11

Partial (north)
1.14758

Partial solar eclipses on July 13, 2018, and January 6, 2019, occur during the next semester series.

Saros series

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending node.

Series members 55–65 occur between 1901 and 2100
55 56 57

January 14, 1907

January 24, 1925

February 4, 1943
58 59 60

February 15, 1961

February 26, 1979

March 9, 1997
61 62 63

March 20, 2015

March 30, 2033

April 11, 2051
64 65

April 21, 2069

May 2, 2087

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 descending node.

21 eclipse events between June 1, 2011 and June 1, 2087
May 31 – June 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128 130 132 134 136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138 140 142 144 146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148 150 152 154 156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158 160 162 164 166

June 1, 2087

October 24, 2098

Notes

  1. ^ http://eclipse.gsfc.nasa.gov/SEsearch/SEsearchmap.php?Ecl=20260812[dead link]
  2. ^ 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.

References