Solar eclipse of April 30, 2060

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Solar eclipse of April 30, 2060
SE2060Apr30T.png
Map
Type of eclipse
NatureTotal
Gamma0.2422
Magnitude1.066
Maximum eclipse
Duration315 sec (5 m 15 s)
Coordinates28°00′N 20°54′E / 28°N 20.9°E / 28; 20.9
Max. width of band222 km (138 mi)
Times (UTC)
Greatest eclipse10:10:00
References
Saros139 (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.

Related eclipses[]

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 2059–2061
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[]

It is a part 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 entabulated in three columns; each one in the same column, every third eclipse, is one exeligmos apart so 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 each duration will decrease, until the series end. This date is the longest solar eclipse computed between 4000BC and 6000AD.[3] Saros series eclipses are 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
24 25 26
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February 3, 1916
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February 14, 1934
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February 25, 1952
27 28 29
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March 7, 1970
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March 18, 1988
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March 29, 2006
30 31 32
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April 8, 2024
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April 20, 2042
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April 30, 2060
33 34 35
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May 11, 2078
SE2096May22T.png
May 22, 2096
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June 3, 2114
36 37 38
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June 13, 2132
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June 25, 2150
SE2168Jul05T.png
July 5, 2168
39 40 41
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July 16, 2186
SE2204Jul27T.png
July 27, 2204
SE2222Aug08T.png
August 8, 2222
42 43 44
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August 18, 2240
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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.

References[]

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