Solar eclipse of November 5, 2059

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Solar eclipse of November 5, 2059
SE2059Nov05A.png
Map
Type of eclipse
NatureAnnular
Gamma0.4454
Magnitude0.9417
Maximum eclipse
Duration420 sec (7 m 0 s)
Coordinates8°42′N 47°06′E / 8.7°N 47.1°E / 8.7; 47.1
Max. width of band238 km (148 mi)
Times (UTC)
Greatest eclipse9:18:15
References
Saros134 (46 of 71)
Catalog # (SE5000)9641

An annular solar eclipse will occur on November 5, 2059. 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. The Sun will be 94% covered in a moderate annular eclipse, lasting 7 minutes exactly and covering a broad path up to 238 km 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
SE2059Nov05A.png
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 134[]

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428. All eclipses in this series occurs at the Moon’s descending node.[2]

Series members 32–48 occur between 1801 and 2100:
32 33 34
SE1807Jun06H.png
June 6, 1807
SE1825Jun16H.png
June 16, 1825
SE1843Jun27H.png
June 27, 1843
35 36 37
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July 8, 1861
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July 19, 1879
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July 29, 1897
38 39 40
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August 10, 1915
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August 21, 1933
SE1951Sep01A.png
September 1, 1951
41 42 43
SE1969Sep11A.png
September 11, 1969
SE1987Sep23A.png
September 23, 1987
SE2005Oct03A.png
October 3, 2005
44 45 46
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October 14, 2023
SE2041Oct25A.png
October 25, 2041
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November 5, 2059
47 48
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November 15, 2077
SE2095Nov27A.png
November 27, 2095

Metonic cycle[]

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).

References[]

  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. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros134.html

External links[]

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