Solar eclipse of September 12, 2053

Summary

A total solar eclipse will take place at the Moon's ascending node of the orbit on Friday, September 12, 2053 with a magnitude of 1.0328. 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.

Solar eclipse of September 12, 2053
Map
Type of eclipse
NatureTotal
Gamma0.314
Magnitude1.0328
Maximum eclipse
Duration184 s (3 min 4 s)
Coordinates21°30′N 41°42′E / 21.5°N 41.7°E / 21.5; 41.7
Max. width of band116 km (72 mi)
Times (UTC)
Greatest eclipse9:34:09
References
Saros145 (24 of 77)
Catalog # (SE5000)9626

Related eclipses edit

Solar eclipses 2051–2054 edit

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 eclipse series sets from 2051 to 2054
Descending node   Ascending node
Saros Map Saros Map
120 April 11, 2051
 
Partial
125 October 4, 2051
 
Partial
130 March 30, 2052
 
Total
135 September 22, 2052
 
Annular
140 March 20, 2053
 
Annular
145 September 12, 2053
 
Total
150 March 9, 2054
 
Partial
155 September 2, 2054
 
Partial

Saros 145 edit

This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon's ascending node.

Series members 10–32 occur between 1801 and 2359
10 11 12
 
April 13, 1801
 
April 24, 1819
 
May 4, 1837
13 14 15
 
May 16, 1855
 
May 26, 1873
 
June 6, 1891
16 17 18
 
June 17, 1909
 
June 29, 1927
 
July 9, 1945
19 20 21
 
July 20, 1963
 
July 31, 1981
 
August 11, 1999
22 23 24
 
August 21, 2017
 
September 2, 2035
 
September 12, 2053 25 26 27  
September 23, 2071
 
October 4, 2089
 
October 16, 2107
28 29 30
 
October 26, 2125
 
November 7, 2143
 
November 17, 2161
31 32 33
 
November 28, 2179
 
December 9, 2197
 
December 21, 2215
34 35 36
 
December 31, 2233
 
January 12, 2252
 
January 22, 2270
37 38 39
 
February 2, 2288
 
February 14, 2306
 
February 25, 2324
40
 
March 8, 2342

Metonic series edit

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 edit

  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.
  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements