Solar eclipse of March 20, 2015

Last updated
Solar eclipse of March 20, 2015
20th March 2015 total solar eclipse cropped.jpg
From Longyearbyen, Svalbard
SE2015Mar20T.png
Map
Type of eclipse
NatureTotal
Gamma 0.9454
Magnitude 1.0445
Maximum eclipse
Duration167 s (2 min 47 s)
Coordinates 64°24′N6°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
Saros 120 (61 of 71)
Catalog # (SE5000) 9541

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, March 20, 2015, [1] with a magnitude of 1.0445. 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 a partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 14 hours after perigee (on March 19, 2015, at 19:40 UTC), the Moon's apparent diameter was larger. [2]

Contents

Totality was visible in the Faroe Islands and Svalbard. A partial eclipse was visible for parts of Greenland, Europe, North Africa, Central Asia, and western Russia. This total solar eclipse is notable in that the path of totality passed over the North Pole.

The longest duration of totality was 2 minutes and 47 seconds off the coast of the Faroe Islands. It was the last total solar eclipse visible in Europe until the eclipse of August 12, 2026. [3]

Event

The solar eclipse began at 08:30 GMT in northwest Europe, and moved towards the northeast, but was still in northern Europe. It was most visible from the North Atlantic and Arctic Oceans, Greenland, Iceland, Ireland, the United Kingdom, Faroe Islands, northern Norway and Murmansk Oblast. The shadow began its pass off the south coast of Greenland. It then moved to the northeast, passing between Iceland and the United Kingdom before moving over the Faroe Islands and the northernmost islands of Norway. The shadow of the eclipse was visible in varying degrees all over Europe. [4] For example, London experienced an 86.8% partial solar eclipse while points north of the Faroe Islands in the Norwegian Sea saw a complete solar eclipse. [5] Three chartered airliners flew above the clouds, giving passengers a slightly prolonged view. [6]

The eclipse was observed at radio frequencies at the Metsähovi Radio Observatory, Finland, where a partial eclipse was seen. [7] The eclipse was also observed by meteorological satellite Meteosat-10. [8] [9]

Impact

The European Union has a solar power output of about 90 gigawatts and production could have been temporarily decreased by up to 34 GW of that dependent on the clarity of the sky. In actuality the dip was less than expected, with a 13 GW drop in Germany happening due to overcast skies. [10] [11] This was the first time that an eclipse had a significant impact on the power system, and the electricity sector took measures to mitigate the impact. The power gradient (change in power) may be −400 MW/minute and +700 MW/minute. Places in Netherlands, Belgium and Denmark were 80-85% obscured. [12] [13] [14] The temperature drops varied greatly across Europe, with most areas having an insignificant drop in temperature due to the overcast weather, while others, like Scotland, Wales, and Iceland received a drop of 2-4°C. These areas were not obscured by cloud cover during the eclipse which may have led to the drop in temperature. Wind speed in the UK dropped by ~9%. [15]

Coincidence of events

In addition to the eclipse, 20 March 2015 was also the day of the March equinox (also known as the spring or vernal equinox in the Northern Hemisphere). In addition, six supermoons were expected for 2015. The supermoon on 20 March 2015 was the third of the year; however, it was a new moon (near side facing away from the sun), and only its shadow was visible. [16]

At greatest eclipse, the Sun was at its zenith less than 24 kilometres (15 mi) south of the Equator. Greatest eclipse occurred at 09:45:39 UTC of Friday, March 20, 2015, while March Equinox occurred at 22:45:09 UTC, just under 13 hours after the greatest eclipse (Greatest eclipse occurred in winter, 13 hours before spring).

Religious Significance

Proponents of the Blood Moon Prophecy, such as Bob O'Dell [17] also pointed out that 20 March 2015 was also a significant day on the Jewish and Biblical calendar. That evening was the onset of the Hebrew month of Nisan, the first month in the Biblical calendar year. Furthermore, the path of the total eclipse over the North Pole [18] was a highly symbolic location infusing the day with both great natural significance and profound religious meaning according to O'Dell. Due to the significance of the eclipse, a global prayer event in Jerusalem was organized that day. [19]

Eclipse visibility

The event was visible as a partial eclipse all across Europe including: Norway, Sweden, Denmark, the United Kingdom, [20] Ireland, [21] Portugal, France, [22] Germany, [23] Poland, [24] Czech Republic, Slovakia, Hungary, Austria, Italy, Montenegro, Finland, Western Russia, and Ukraine.

Simulation

SE2015Mar20T.gif Animation solar eclipse of March 20, 2015.gif

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [25]

March 20, 2015 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2015 March 20 at 07:41:59.5 UTC
First Umbral External Contact2015 March 20 at 09:10:40.3 UTC
First Central Line2015 March 20 at 09:13:50.9 UTC
First Umbral Internal Contact2015 March 20 at 09:17:19.8 UTC
Ecliptic Conjunction2015 March 20 at 09:37:18.1 UTC
Greatest Duration2015 March 20 at 09:46:24.2 UTC
Greatest Eclipse2015 March 20 at 09:46:46.8 UTC
Equatorial Conjunction2015 March 20 at 10:18:14.1 UTC
Last Umbral Internal Contact2015 March 20 at 10:15:51.3 UTC
Last Central Line2015 March 20 at 10:19:19.7 UTC
Last Umbral External Contact2015 March 20 at 10:22:29.9 UTC
Last Penumbral External Contact2015 March 20 at 11:51:20.4 UTC
March 20, 2015 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04455
Eclipse Obscuration1.09109
Gamma0.94536
Sun Right Ascension23h58m01.5s
Sun Declination-00°12'50.4"
Sun Semi-Diameter16'03.7"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension23h56m50.5s
Moon Declination+00°42'08.7"
Moon Semi-Diameter16'41.6"
Moon Equatorial Horizontal Parallax1°01'15.8"
ΔT67.7 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of March–April 2015
March 20
Descending node (new moon)
April 4
Ascending node (full moon)
SE2015Mar20T.png Lunar eclipse chart close-2015Apr04.png
Total solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132

Eclipses in 2015

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 120

Inex

Triad

Solar eclipses of 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. [26]

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
SarosMapGammaSarosMapGamma
120
Total solar eclipse of March 20, 2015 by Damien Deltenre (licensed for free use). (32844461616).jpg
Totality in Longyearbyen, Svalbard
March 20, 2015
SE2015Mar20T.png
Total
0.94536125
Double Photobomb (21389400576).jpg
Solar Dynamics Observatory

September 13, 2015
SE2015Sep13P.png
Partial
−1.10039
130
Total Solar Eclipse, 9 March 2016, from Balikpapan, East Kalimantan, Indonesia.JPG
Balikpapan, Indonesia
March 9, 2016
SE2016Mar09T.png
Total
0.26092135
Eclipse 20160901 center.jpg
Annularity in L'Étang-Salé, Réunion
September 1, 2016
SE2016Sep01A.png
Annular
−0.33301
140
26-feb-2017 solar ecipse.jpg
Partial from Buenos Aires, Argentina
February 26, 2017
SE2017Feb26A.png
Annular
−0.45780145
2017 Total Solar Eclipse (NHQ201708210100) - square crop.jpg
Totality in Madras, OR, USA
August 21, 2017
Solar eclipse global visibility 2017Aug21T.png
Total
0.43671
150
Eclipse Solar Parcial - 15.02.2018 - Olivos, GBA (Argentina).jpg
Partial in Olivos, Buenos Aires, Argentina
February 15, 2018
SE2018Feb15P.png
Partial
−1.21163155
2018.08.11 1214Z C8F6 Solar Eclipse (43976490201).jpg
Partial in Huittinen, Finland
August 11, 2018
SE2018Aug11P.png
Partial
1.14758

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit. [27]

Series members 50–71 occur between 1801 and 2195:
505152
SE1816Nov19T.gif
November 19, 1816
SE1834Nov30T.gif
November 30, 1834
SE1852Dec11T.gif
December 11, 1852
535455
SE1870Dec22T.gif
December 22, 1870
SE1889Jan01T.png
January 1, 1889
SE1907Jan14T.png
January 14, 1907
565758
SE1925Jan24T.png
January 24, 1925
SE1943Feb04T.png
February 4, 1943
SE1961Feb15T.png
February 15, 1961
596061
SE1979Feb26T.png
February 26, 1979
SE1997Mar09T.png
March 9, 1997
SE2015Mar20T.png
March 20, 2015
626364
SE2033Mar30T.png
March 30, 2033
SE2051Apr11P.png
April 11, 2051
SE2069Apr21P.png
April 21, 2069
656667
SE2087May02P.png
May 2, 2087
Saros120 66van71 SE2105May14P.jpg
May 14, 2105
Saros120 67van71 SE2123May25P.jpg
May 25, 2123
686970
Saros120 68van71 SE2141Jun04P.jpg
June 4, 2141
Saros120 69van71 SE2159Jun16P.jpg
June 16, 2159
Saros120 70van71 SE2177Jun26P.jpg
June 26, 2177
71
Saros120 71van71 SE2195Jul07P.jpg
July 7, 2195

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.

22 eclipse events between June 1, 2011 and October 24, 2098
May 31–June 1March 19–20January 5–6October 24–25August 12–13
118120122124126
SE2011Jun01P.png
June 1, 2011
SE2015Mar20T.png
March 20, 2015
SE2019Jan06P.png
January 6, 2019
SE2022Oct25P.png
October 25, 2022
SE2026Aug12T.png
August 12, 2026
128130132134136
SE2030Jun01A.png
June 1, 2030
SE2034Mar20T.png
March 20, 2034
SE2038Jan05A.png
January 5, 2038
SE2041Oct25A.png
October 25, 2041
SE2045Aug12T.png
August 12, 2045
138140142144146
SE2049May31A.png
May 31, 2049
SE2053Mar20A.png
March 20, 2053
SE2057Jan05T.png
January 5, 2057
SE2060Oct24A.png
October 24, 2060
SE2064Aug12T.png
August 12, 2064
148150152154156
SE2068May31T.png
May 31, 2068
SE2072Mar19P.png
March 19, 2072
SE2076Jan06T.png
January 6, 2076
SE2079Oct24A.png
October 24, 2079
SE2083Aug13P.png
August 13, 2083
158160162164
SE2087Jun01P.png
June 1, 2087
SE2098Oct24P.png
October 24, 2098

Tritos series

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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 1971 and 2200
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE1982Jun21P.png
June 21, 1982
(Saros 117)
SE1993May21P.png
May 21, 1993
(Saros 118)
SE2004Apr19P.png
April 19, 2004
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2026Feb17A.png
February 17, 2026
(Saros 121)
SE2037Jan16P.png
January 16, 2037
(Saros 122)
SE2047Dec16P.png
December 16, 2047
(Saros 123)
SE2058Nov16P.png
November 16, 2058
(Saros 124)
SE2069Oct15P.png
October 15, 2069
(Saros 125)
SE2080Sep13P.png
September 13, 2080
(Saros 126)
SE2091Aug15T.png
August 15, 2091
(Saros 127)
SE2102Jul15A.png
July 15, 2102
(Saros 128)
SE2113Jun13T.png
June 13, 2113
(Saros 129)
SE2124May14T.png
May 14, 2124
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2168Jan10A.png
January 10, 2168
(Saros 134)
SE2178Dec09A.png
December 9, 2178
(Saros 135)
SE2189Nov08T.png
November 8, 2189
(Saros 136)
SE2200Oct09A.png
October 9, 2200
(Saros 137)

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.

Series members between 1801 and 2200
SE1812Aug07P.gif
August 7, 1812
(Saros 113)
SE1841Jul18P.gif
July 18, 1841
(Saros 114)
SE1870Jun28P.gif
June 28, 1870
(Saros 115)
SE1899Jun08P.gif
June 8, 1899
(Saros 116)
SE1928May19T.png
May 19, 1928
(Saros 117)
SE1957Apr30A.png
April 30, 1957
(Saros 118)
SE1986Apr09P.png
April 9, 1986
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2073Feb07P.png
February 7, 2073
(Saros 122)
Saros123 58van70 SE2102Jan19P.jpg
January 19, 2102
(Saros 123)
Saros124 61van73 SE2130Dec30P.jpg
December 30, 2130
(Saros 124)
Saros125 62van73 SE2159Dec09P.jpg
December 9, 2159
(Saros 125)
Saros126 57van72 SE2188Nov18P.jpg
November 18, 2188
(Saros 126)

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A total solar eclipse occurred at the Moon's descending node of orbit between Monday, September 11, 1950 and Tuesday, September 12, 1950, with a magnitude of 1.0182. 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. Occurring about 3.2 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of May 1, 2079</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, May 1, 2079, with a magnitude of 1.0512. 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. Occurring about 1.2 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of April 16, 1893</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, April 16, 1893, with a magnitude of 1.0556. 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. Occurring about 1.3 days before perigee, the Moon's apparent diameter was larger.

References

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Bibliography