Solar eclipse of April 20, 2023

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Solar eclipse of April 20, 2023
SE2023Apr20H.png
Map
Type of eclipse
NatureHybrid
Gamma-0.3952
Magnitude1.0132
Maximum eclipse
Duration76 sec (1 m 16 s)
Coordinates9°36′S 125°48′E / 9.6°S 125.8°E / -9.6; 125.8
Max. width of band49 km (30 mi)
Times (UTC)
Greatest eclipse4:17:56
References
Saros129 (52 of 80)
Catalog # (SE5000)9559

A total solar eclipse will occur on Thursday, April 20, 2023. 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 the surface of the Earth, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Totality for this eclipse will be visible in the North West Cape peninsula and Barrow Island in Western Australia, eastern parts of East Timor, as well as Damar Island and parts of the province of Papua in Indonesia.[1]

It is a hybrid eclipse, with portions of its path near sunrise and sunset as annular.

Images[]

SE2023Apr20H.gif
Animated path

Related eclipses[]

Eclipses of 2023[]

Solar eclipses of 2022–2025[]

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.[2]

Solar eclipse series sets from 2022–2025
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 2022 April 30
SE2022Apr30P.png
Partial
-1.19008 124 2022 October 25
SE2022Oct25P.png
Partial
1.07014
129 2023 April 20
SE2023Apr20H.png
Hybrid
-0.39515 134 2023 October 14
SE2023Oct14A.png
Annular
0.37534
139 2024 April 8
SE2024Apr08T.png
Total
0.34314 144 2024 October 2
SE2024Oct02A.png
Annular
-0.35087
149 2025 March 29
SE2025Mar29P.png
Partial
1.04053 154 2025 September 21
SE2025Sep21P.png
Partial
-1.06509

Saros 129[]

It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses from March 29, 1987 through April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 . All eclipses in this series occurs at the Moon’s ascending node.[3]

Series members 46–56 occur between 1901 and 2100:
46 47 48
SE1915Feb14A.png
February 14, 1915
SE1933Feb24A.png
February 24, 1933
SE1951Mar07A.png
March 7, 1951
49 50 51
SE1969Mar18A.png
March 18, 1969
SE1987Mar29H.png
March 29, 1987
SE2005Apr08H.png
April 8, 2005
52 53 54
SE2023Apr20H.png
April 20, 2023
SE2041Apr30T.png
April 30, 2041
SE2059May11T.png
May 11, 2059
55 56
SE2077May22T.png
May 22, 2077
SE2095Jun02T.png
June 2, 2095

Inex series[]

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Tritos series[]

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

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
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127 129 131 133 135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137 139 141 143 145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147 149 151 153 155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157 159 161 163 165
SE2076Jul01P.png
July 1, 2076

References[]

  1. ^ Hybrid Solar Eclipse of 2023 Apr 20, National Aeronautics and Space Administration
  2. ^ 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.
  3. ^ Espenak, F. "NASA Catalog of Solar Eclipses of Saros 129". eclipse.gsfc.nasa.gov.

External links[]

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