Solar eclipse of November 25, 2030
Map
Type of eclipse
NatureTotal
Gamma−0.3867
Magnitude1.0468
Maximum eclipse
Duration224 sec (3 m 44 s)
Coordinates43°36′S 71°12′E / 43.6°S 71.2°E / -43.6; 71.2
Max. width of band169 km (105 mi)
Times (UTC)
Greatest eclipse6:51:37
References
Saros133 (46 of 72)
Catalog # (SE5000)9576

A total solar eclipse will occur on Monday, November 25, 2030. 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.

Images


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
118June 12, 2029

Partial
123December 5, 2029

Partial
128June 1, 2030

Annular
133November 25, 2030

Total
138May 21, 2031

Annular
143November 14, 2031

Hybrid
148May 9, 2032

Annular
153November 3, 2032

Partial

Saros 133

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[2] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.

Series members 30–56 occur between 1742 and 2211
30 31 32
June 3, 1742 June 13, 1760
June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850
August 18, 1868

August 29, 1886
39 40 41

September 9, 1904

September 21, 1922

October 1, 1940
42 43 44

October 12, 1958

October 23, 1976

November 3, 1994
45 46 47

November 13, 2012

November 25, 2030

December 5, 2048
48 49 50

December 17, 2066

December 27, 2084

January 8, 2103
51 52 53

January 19, 2121

January 30, 2139

February 9, 2157
54 55 56

February 21, 2175

March 3, 2193

March 15, 2211

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.

21 eclipse events, progressing from south to north between July 1, 2000 and July 1, 2076
July 1–2 April 19–20 February 5–7 November 24–25 September 12–13
117 119 121 123 125

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157 159 161 163 165

July 1, 2076

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/SEsaros133.html
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