Solar eclipse of April 20, 2023

Solar eclipse of April 20, 2023
Partial from Magetan, Indonesia
Map
Type of eclipse
Nature	Hybrid
Gamma	−0.3952
Magnitude	1.0132
Maximum eclipse
Duration	76 s (1 min 16 s)
Coordinates	9.6°S 125.8°E / -9.6; 125.8
Max. width of band	49 km (30 mi)
Times (UTC)
Greatest eclipse	4:17:56
References
Saros	129 (52 of 80)
Catalog # (SE5000)	9559

A hybrid solar eclipse occurred on Thursday, April 20, 2023. A solar eclipse occurs when the Moon passes between Earth and the Sun thereby totally or partly obscuring the Sun for a viewer on Earth. A hybrid solar eclipse is a rare type of solar eclipse that changes its appearance from annular to total and back as the Moon's shadow moves across the Earth's surface. Totality occurs in a narrow path across the surface of the Earth, with the partial solar eclipse visible over a surrounding region thousands of kilometers wide. Hybrid solar eclipses are extremely rare, occurring in only 3.1% of solar eclipses in the 21st century.

Totality for this eclipse was 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. More than 20,000 people watched the eclipse from Exmouth, on Western Australia's North West Cape. This event cost the State Government of Western Australia $20 million AUD ($13.5 million USD) in planning and logistics fees. The date marked a significant moment of astrotourism and tourism in Western Australia, in addition to the beginning of the 2023 Margaret River Pro.

Portions of the eclipse's path near sunrise and sunset were annular. Occurring only 4.1 days after perigee (Perigee on Sunday, April 16, 2023), the Moon's apparent diameter was 1.02% larger than average.

Images

Animated path

Gallery

East Timor

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Indonesia

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  Partial from Jakarta, 03:47 UTC
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  Partial from Palangka Raya, Central Kalimantan, 04:02 UTC
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  Totality observed from Biak, Indonesia, 04:57 UTC - Zoomed out & the sun was barely visible
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  Partial viewed from Biak, Indonesia, 05:25 UTC - Post Totality

Philippines

• 
  Partial from San Fernando, Pampanga, 04:50 UTC
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  Partial from San Jose del Monte, Bulacan, 04:55 UTC
• Partial from Quezon City, 05:32 UTC
  Partial from Quezon City, 05:32 UTC

Related eclipses

Tzolkinex

• Preceded by: Solar eclipse of March 8–9, 2016
• Followed by: Solar eclipse of June 1, 2030

Half-Saros cycle

• Preceded by: Lunar eclipse of April 15, 2014
• Followed by: Lunar eclipse of April 25, 2032

Tritos

• Preceded by: Solar eclipse of May 20–21, 2012
• Followed by: Solar eclipse of March 20, 2034

Solar Saros 129

• Preceded by: Solar eclipse of April 8, 2005
• Followed by: Solar eclipse of April 30, 2041

Inex

• Preceded by: Solar eclipse of May 10, 1994
• Followed by: Solar eclipse of March 30, 2052

Triad

• Preceded by: Solar eclipse of June 19, 1936
• Followed by: Solar eclipse of February 18–19, 2110

Eclipses of 2023

• A hybrid solar eclipse on April 20.
• A penumbral lunar eclipse on May 5.
• An annular solar eclipse on October 14.
• A partial lunar eclipse on October 28.

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.

Solar eclipse series sets from 2022 to 2025
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
119 Partial in CTIO, Chile	April 30, 2022 Partial	−1.19008		124 Partial from Saratov, Russia	October 25, 2022 Partial	1.07014
129 Partial in Magetan, Indonesia	April 20, 2023 Hybrid	−0.39515		134 Annularity in Hobbs, NM, USA	October 14, 2023 Annular	0.37534
139 Totality in Dallas, TX, USA	April 8, 2024 Total	0.34314		144	October 2, 2024 Annular	−0.35087
149	March 29, 2025 Partial	1.04053		154	September 21, 2025 Partial	−1.06509

Saros 129

This eclipse is a part of Saros series 129, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 3, 1103. It contains annular eclipses from 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. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 34 at 5 minutes, 10 seconds on October 4, 1698, and the longest duration of totality will be produced by member 58 at 3 minutes, 43 seconds on June 25, 2131. All eclipses in this series occur at the Moon’s ascending node of orbit.

Series members 40–61 occur between 1801 and 2200:
40	41	42
December 10, 1806	December 20, 1824	December 31, 1842
43	44	45
January 11, 1861	January 22, 1879	February 1, 1897
46	47	48
February 14, 1915	February 24, 1933	March 7, 1951
49	50	51
March 18, 1969	March 29, 1987	April 8, 2005
52	53	54
April 20, 2023	April 30, 2041	May 11, 2059
55	56	57
May 22, 2077	June 2, 2095	June 13, 2113
58	59	60
June 25, 2131	July 5, 2149	July 16, 2167
61
July 26, 2185

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.

Inex series members between 1901 and 2100:
July 10, 1907 (Saros 125)	June 19, 1936 (Saros 126)	May 30, 1965 (Saros 127)
May 10, 1994 (Saros 128)	April 20, 2023 (Saros 129)	March 30, 2052 (Saros 130)
March 10, 2081 (Saros 131)

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.

Series members between 1901 and 2100
March 29, 1903 (Saros 118)	February 25, 1914 (Saros 119)	January 24, 1925 (Saros 120)
December 25, 1935 (Saros 121)	November 23, 1946 (Saros 122)	October 23, 1957 (Saros 123)
September 22, 1968 (Saros 124)	August 22, 1979 (Saros 125)	July 22, 1990 (Saros 126)
June 21, 2001 (Saros 127)	May 20, 2012 (Saros 128)	April 20, 2023 (Saros 129)
March 20, 2034 (Saros 130)	February 16, 2045 (Saros 131)	January 16, 2056 (Saros 132)
December 17, 2066 (Saros 133)	November 15, 2077 (Saros 134)	October 14, 2088 (Saros 135)
September 14, 2099 (Saros 136)

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 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
July 1, 2076

External links

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