Solar eclipse of May 9, 2032

Last updated
Solar eclipse of May 9, 2032
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Map
Type of eclipse
NatureAnnular
Gamma -0.9375
Magnitude 0.9957
Maximum eclipse
Duration22 sec (0 m 22 s)
Coordinates 51°18′S7°06′W / 51.3°S 7.1°W / -51.3; -7.1
Max. width of band44 km (27 mi)
Times (UTC)
Greatest eclipse13:26:42
References
Saros 148 (22 of 75)
Catalog # (SE5000) 9579

An annular solar eclipse will occur on May 9, 2032. 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.

Contents

Images

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Animated path

Solar eclipses 2029–2032

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]

Note: Partial solar eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2029–2032
Descending node Ascending node
118 June 12, 2029
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Partial
123 December 5, 2029
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Partial
128 June 1, 2030
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Annular
133 November 25, 2030
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Total
138 May 21, 2031
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Annular
143 November 14, 2031
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Hybrid
148 May 9, 2032
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Annular
153 November 3, 2032
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Partial

Saros 148

Solar saros 148, repeating every about 18 years and 11 days, contains 75 events. The series started with a partial solar eclipse on September 21, 1653. It has annular eclipses on April 29, 2014, and May 9, 2032, and a hybrid eclipse on May 20, 2050. It has total eclipses from May 31, 2068, to August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. The longest total eclipse will be on April 26, 2609, at 5 minutes and 23 seconds. [2]

Series members 15–25 occur between 1901 and 2100:
151617
SE1906Feb23P.png
February 23, 1906
SE1924Mar05P.png
March 5, 1924
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March 16, 1942
181920
SE1960Mar27P.png
March 27, 1960
SE1978Apr07P.png
April 7, 1978
SE1996Apr17P.png
April 17, 1996
212223
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April 29, 2014
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May 9, 2032
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May 20, 2050
2425
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May 31, 2068
SE2086Jun11T.png
June 11, 2086

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). All eclipses in this table occur at the Moon's descending node.

21 events between July 22, 1971 and July 22, 2047
July 21–22May 9–11February 26–27December 14–15October 2–3
106108110112114
July 21, 1952May 10, 1956February 26, 1960December 16, 1963October 3, 1967
116118120122124
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July 22, 1971
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May 11, 1975
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February 26, 1979
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December 15, 1982
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October 3, 1986
126128130132134
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July 22, 1990
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May 10, 1994
SE1998Feb26T.png
February 26, 1998
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December 14, 2001
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October 3, 2005
136138140142144
SE2009Jul22T.png
July 22, 2009
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May 10, 2013
SE2017Feb26A.png
February 26, 2017
SE2020Dec14T.png
December 14, 2020
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October 2, 2024
146148150152154
SE2028Jul22T.png
July 22, 2028
SE2032May09A.png
May 9, 2032
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February 27, 2036
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December 15, 2039
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October 3, 2043
156
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July 22, 2047

See also

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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. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.