Solar eclipse of February 26, 2017

Last updated
Solar eclipse of February 26, 2017
26-feb-2017 solar ecipse.jpg
SE2017Feb26A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.4578
Magnitude 0.9922
Maximum eclipse
Duration44 s (0 min 44 s)
Coordinates 34°42′S31°12′W / 34.7°S 31.2°W / -34.7; -31.2
Max. width of band31 km (19 mi)
Times (UTC)
Greatest eclipse14:54:33
References
Saros 140 (29 of 71)
Catalog # (SE5000) 9545

An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, February 26, 2017, [1] [2] [3] [4] with a magnitude of 0.9922. 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. Occurring about 4.9 days before perigee (on March 3, 2017, at 13:30 UTC), the Moon's apparent diameter was larger. [5]

Contents

The eclipse was visible across southern Chile and Argentina in the morning and ended in Angola and southwestern Katanga, Democratic Republic of the Congo at sunset. In Argentina, the best places to see the eclipse were located in the south of the Chubut Province, in the towns of Facundo, Sarmiento and Camarones. A partial eclipse was visible for parts of southern South America, southern and western Africa, and Antarctica.

Images

SE2017Feb26A.GIF
The Solar Ring of Fire.gif
Animation assembled from 3 images acquired by NASA’s Earth Polychromatic Imaging Camera.

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. [6]

February 26, 2017 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2017 February 26 at 12:11:56.1 UTC
First Umbral External Contact2017 February 26 at 13:16:26.6 UTC
First Central Line2017 February 26 at 13:17:14.6 UTC
Greatest Duration2017 February 26 at 13:17:14.6 UTC
First Umbral Internal Contact2017 February 26 at 13:18:02.7 UTC
Equatorial Conjunction2017 February 26 at 14:39:54.4 UTC
Greatest Eclipse2017 February 26 at 14:54:32.8 UTC
Ecliptic Conjunction2017 February 26 at 14:59:31.7 UTC
Last Umbral Internal Contact2017 February 26 at 16:31:16.0 UTC
Last Central Line2017 February 26 at 16:32:01.1 UTC
Last Umbral External Contact2017 February 26 at 16:32:46.1 UTC
Last Penumbral External Contact2017 February 26 at 17:37:10.0 UTC
February 26, 2017 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.99223
Eclipse Obscuration0.98451
Gamma−0.45780
Sun Right Ascension22h39m23.1s
Sun Declination-08°29'38.8"
Sun Semi-Diameter16'09.0"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension22h39m53.2s
Moon Declination-08°55'03.6"
Moon Semi-Diameter15'47.8"
Moon Equatorial Horizontal Parallax0°57'58.6"
ΔT68.6 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 February 2017
February 11
Ascending node (full moon)
February 26
Descending node (new moon)
Lunar eclipse chart close-2017Feb11.png SE2017Feb26A.png
Penumbral lunar eclipse
Lunar Saros 114
Annular solar eclipse
Solar Saros 140

Eclipses in 2017

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 140

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. [7]

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 140

This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit. [8]

Series members 18–39 occur between 1801 and 2200:
181920
SE1818Oct29T.png
October 29, 1818
SE1836Nov09T.png
November 9, 1836
SE1854Nov20H.png
November 20, 1854
212223
SE1872Nov30H.png
November 30, 1872
SE1890Dec12H.png
December 12, 1890
SE1908Dec23H.png
December 23, 1908
242526
SE1927Jan03A.png
January 3, 1927
SE1945Jan14A.png
January 14, 1945
SE1963Jan25A.png
January 25, 1963
272829
SE1981Feb04A.png
February 4, 1981
SE1999Feb16A.png
February 16, 1999
SE2017Feb26A.png
February 26, 2017
303132
SE2035Mar09A.png
March 9, 2035
SE2053Mar20A.png
March 20, 2053
SE2071Mar31A.png
March 31, 2071
333435
SE2089Apr10A.png
April 10, 2089
SE2107Apr23A.png
April 23, 2107
SE2125May03A.png
May 3, 2125
363738
SE2143May14A.png
May 14, 2143
SE2161May25A.png
May 25, 2161
SE2179Jun05A.png
June 5, 2179
39
SE2197Jun15A.png
June 15, 2197

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 July 22, 1971 and July 22, 2047
July 22May 9–11February 26–27December 14–15October 2–3
116118120122124
SE1971Jul22P.png
July 22, 1971
SE1975May11P.png
May 11, 1975
SE1979Feb26T.png
February 26, 1979
SE1982Dec15P.png
December 15, 1982
SE1986Oct03H.png
October 3, 1986
126128130132134
SE1990Jul22T.png
July 22, 1990
SE1994May10A.png
May 10, 1994
SE1998Feb26T.png
February 26, 1998
SE2001Dec14A.png
December 14, 2001
SE2005Oct03A.png
October 3, 2005
136138140142144
SE2009Jul22T.png
July 22, 2009
SE2013May10A.png
May 10, 2013
SE2017Feb26A.png
February 26, 2017
SE2020Dec14T.png
December 14, 2020
SE2024Oct02A.png
October 2, 2024
146148150152154
SE2028Jul22T.png
July 22, 2028
SE2032May09A.png
May 9, 2032
SE2036Feb27P.png
February 27, 2036
SE2039Dec15T.png
December 15, 2039
SE2043Oct03A.png
October 3, 2043
156
SE2047Jul22P.png
July 22, 2047

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.

Series members between 1801 and 2200
SE1809Oct09T.gif
October 9, 1809
(Saros 121)
SE1820Sep07A.png
September 7, 1820
(Saros 122)
SE1831Aug07T.gif
August 7, 1831
(Saros 123)
SE1842Jul08T.png
July 8, 1842
(Saros 124)
SE1853Jun06A.gif
June 6, 1853
(Saros 125)
SE1864May06H.gif
May 6, 1864
(Saros 126)
SE1875Apr06T.png
April 6, 1875
(Saros 127)
SE1886Mar05A.gif
March 5, 1886
(Saros 128)
SE1897Feb01A.gif
February 1, 1897
(Saros 129)
SE1908Jan03T.png
January 3, 1908
(Saros 130)
SE1918Dec03A.png
December 3, 1918
(Saros 131)
SE1929Nov01A.png
November 1, 1929
(Saros 132)
SE1940Oct01T.png
October 1, 1940
(Saros 133)
SE1951Sep01A.png
September 1, 1951
(Saros 134)
SE1962Jul31A.png
July 31, 1962
(Saros 135)
SE1973Jun30T.png
June 30, 1973
(Saros 136)
SE1984May30A.png
May 30, 1984
(Saros 137)
SE1995Apr29A.png
April 29, 1995
(Saros 138)
SE2006Mar29T.png
March 29, 2006
(Saros 139)
SE2017Feb26A.png
February 26, 2017
(Saros 140)
SE2028Jan26A.png
January 26, 2028
(Saros 141)
SE2038Dec26T.png
December 26, 2038
(Saros 142)
SE2049Nov25H.png
November 25, 2049
(Saros 143)
SE2060Oct24A.png
October 24, 2060
(Saros 144)
SE2071Sep23T.png
September 23, 2071
(Saros 145)
SE2082Aug24T.png
August 24, 2082
(Saros 146)
SE2093Jul23A.png
July 23, 2093
(Saros 147)
SE2104Jun22T.png
June 22, 2104
(Saros 148)
SE2115May24T.png
May 24, 2115
(Saros 149)
Saros150 23van71 SE2126Apr22A.jpg
April 22, 2126
(Saros 150)
Saros151 21van72 SE2137Mar21A.jpg
March 21, 2137
(Saros 151)
Saros152 20van70 SE2148Feb19T.jpg
February 19, 2148
(Saros 152)
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
(Saros 153)
Saros154 15van71 SE2169Dec18A.jpg
December 18, 2169
(Saros 154)
Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
(Saros 155)
Saros156 11van69 SE2191Oct18A.jpg
October 18, 2191
(Saros 156)

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
SE1814Jul17T.png
July 17, 1814
(Saros 133)
SE1843Jun27H.png
June 27, 1843
(Saros 134)
SE1872Jun06A.gif
June 6, 1872
(Saros 135)
SE1901May18T.png
May 18, 1901
(Saros 136)
SE1930Apr28H.png
April 28, 1930
(Saros 137)
SE1959Apr08A.png
April 8, 1959
(Saros 138)
SE1988Mar18T.png
March 18, 1988
(Saros 139)
SE2017Feb26A.png
February 26, 2017
(Saros 140)
SE2046Feb05A.png
February 5, 2046
(Saros 141)
SE2075Jan16T.png
January 16, 2075
(Saros 142)
SE2103Dec29A.png
December 29, 2103
(Saros 143)
SE2132Dec07A.png
December 7, 2132
(Saros 144)
SE2161Nov17T.png
November 17, 2161
(Saros 145)
SE2190Oct29H.png
October 29, 2190
(Saros 146)

Notes and references

  1. "February 26, 2017 Annular Solar Eclipse". timeanddate. Retrieved 12 August 2024.
  2. Cofield, Calla (February 26, 2017). "Moon Blocks (Most of) the Sun in 'Ring of Fire' Solar Eclipse". Space.com.
  3. Dwyer, Colin (February 25, 2017). "'Ring Of Fire' Eclipse Set To Blaze In Southern Skies". NPR.
  4. ""Ring of fire" annular eclipse: Stunning views of first solar eclipse of 2017". www.cbsnews.com. February 27, 2017.
  5. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 August 2024.
  6. "Annular Solar Eclipse of 2017 Feb 26". EclipseWise.com. Retrieved 12 August 2024.
  7. 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.
  8. "NASA - Catalog of Solar Eclipses of Saros 140". eclipse.gsfc.nasa.gov.

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References