Solar eclipse of April 30, 2060

Last updated
Solar eclipse of April 30, 2060
SE2060Apr30T.png
Map
Type of eclipse
NatureTotal
Gamma 0.2422
Magnitude 1.066
Maximum eclipse
Duration315 s (5 min 15 s)
Coordinates 28°00′N20°54′E / 28°N 20.9°E / 28; 20.9
Max. width of band222 km (138 mi)
Times (UTC)
Greatest eclipse10:10:00
References
Saros 139 (32 of 71)
Catalog # (SE5000) 9642

A total solar eclipse will occur on Friday, April 30, 2060. 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.

Contents

Solar eclipses 2059–2061

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]

Solar eclipses 2059 to 2061
119 May 22, 2058
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Partial
124 November 16, 2058
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Partial
129 May 11, 2059
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Total
134 November 5, 2059
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Annular
139 April 30, 2060
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Total
144 October 24, 2060
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Annular
149 April 20, 2061
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Total
154 October 13, 2061
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Annular

Saros 139

This eclipse is a member of saros series 139, repeating every 18 years, 11 days, 8 hours, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627, through to December 9, 1825; and total eclipses from December 21, 1843, through to March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763. 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 solar eclipse of June 13, 2132, will be the longest total solar eclipse since July 11, 1991, at 6 minutes, 55.02 seconds.

The longest duration of totality will be produced by member 39 at 7 minutes, 29.22 seconds on July 16, 2186. [2] After that date, the durations of totality will decrease until the series ends. This date is the longest solar eclipse computed between 4000 BC and AD 6000. [3] Saros series eclipses occur during the Moon's ascending node (a term related to our equator and polar-naming conventions).

Series members 24–45 occur between 1901 and 2300
242526
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February 3, 1916
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February 14, 1934
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February 25, 1952
272829
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March 7, 1970
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March 18, 1988
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March 29, 2006
303132
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April 8, 2024
SE2042Apr20T.png
April 20, 2042
SE2060Apr30T.png
April 30, 2060
333435
SE2078May11T.png
May 11, 2078
SE2096May22T.png
May 22, 2096
SE2114Jun03T.png
June 3, 2114
363738
SE2132Jun13T.png
June 13, 2132
SE2150Jun25T.png
June 25, 2150
SE2168Jul05T.png
July 5, 2168
394041
SE2186Jul16T.png
July 16, 2186
SE2204Jul27T.png
July 27, 2204
SE2222Aug08T.png
August 8, 2222
424344
SE2240Aug18T.png
August 18, 2240
SE2258Aug29T.png
August 29, 2258
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September 9, 2276
45
SE2294Sep20T.png
September 20, 2294

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.

Notes

  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. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
  3. Ten Millennium Catalog of Long Solar Eclipses, −3999 to +6000 (4000 BCE to 6000 CE) Fred Espenak.

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References