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Solar eclipse of October 2, 2024

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Solar eclipse of October 2, 2024
Map
Type of eclipse
NatureAnnular
Gamma−0.3509
Magnitude0.9326
Maximum eclipse
Duration445 s (7 min 25 s)
Coordinates22°00′S 114°30′W / 22°S 114.5°W / -22; -114.5
Max. width of band266 km (165 mi)
Times (UTC)
Greatest eclipse18:46:13
References
Saros144 (17 of 70)
Catalog # (SE5000)9562

An annular solar eclipse will occur at the Moon’s descending node of orbit on Wednesday, October 2, 2024, with a magnitude of 0.9326. 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.

Other than Easter Island and a small portion near the southern tips of Argentina and Chile and the north of the Falkland Islands,[1] the path of the eclipse's antumbra will be entirely over the Pacific Ocean. The penumbra will be visible from southern South America, Hawaii, the southwesternmost parts of Mexico (more specifically, Baja California del Sur and Jalisco), and portions of Antarctica. Approximately 175,000 people live in the path of annularity.[2][3] The eclipse’s magnitude will be 0.93261, occurring only 56 minutes before apogee.

The next solar eclipse occurs on March 29, 2025.

Images[edit]


Animated path

Details of the antumbra in some places or cities[edit]

Solar Eclipse of October 2, 2024
Country or Territory Place or City Start

of
partial
eclipse
(Local Time)

Start of
annular
eclipse (Local Time)
End of
annular
eclipse (Local Time)
Duration of
annular
eclipse
End of
partial
eclipse (Local Time)
Maximum darkness Magnitude
 Chile Hanga Roa, Easter Island, Valparaíso Region 12:23:49 14:04:05 14:10:24 6 min 19 s 15:52:23 86,9% 0,932
 Chile Tortel, Aysén Region 15:56:48 17:20:04 17:26:24 6 min 20 s 18:41:50 85,6% 0,925
 Chile Villa O'Higgins, Aysén Region 15:58:12 17:21:05 17:26:37 5 min 32 s 18:41:49 85,6% 0,925
 Chile Cochrane, Aysén Region 15:57:55 17:21:15 17:27:09 5 min 54 s 18:42:30 85,6% 0,925
 Argentina Gobernador Gregores, Santa Cruz Province 16:01:02 17:22:40 17:28:28 5 min 48 s 18:42:27 85,5% 0,925
 Argentina Puerto San Julián, Santa Cruz Province 16:03:57 17:24:27 17:29:49 5 min 22 s 18:42:48 85,4% 0,924
 Argentina Puerto Deseado, Santa Cruz Province 16:06:06 17:27:12 17:30:58 3 min 45 s 18:44:14 85,4% 0,924

Related eclipses[edit]

The 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.[4] It is also part of Saros cycle 144, repeating every 18 years, 11 days, containing 70 events.

Eclipses of 2024[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 144[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 2022–2025[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.[5]

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 144[edit]

This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 will be produced by member 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[6]

Series members 5–26 occur between 1801 and 2200:
5 6 7

May 25, 1808

June 5, 1826

June 16, 1844
8 9 10

June 27, 1862

July 7, 1880

July 18, 1898
11 12 13

July 30, 1916

August 10, 1934

August 20, 1952
14 15 16

August 31, 1970

September 11, 1988

September 22, 2006
17 18 19

October 2, 2024

October 14, 2042

October 24, 2060
20 21 22

November 4, 2078

November 15, 2096

November 27, 2114
23 24 25

December 7, 2132

December 19, 2150

December 29, 2168
26

January 9, 2187

Tritos series[edit]

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[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 descending node.

21 events between July 22, 1971 and July 22, 2047
July 21–22 May 9–11 February 26–27 December 14–15 October 2–3
116 118 120 122 124

July 22, 1971

May 11, 1975

February 26, 1979

December 15, 1982

October 3, 1986
126 128 130 132 134

July 22, 1990

May 10, 1994

February 26, 1998

December 14, 2001

October 3, 2005
136 138 140 142 144

July 22, 2009

May 10, 2013

February 26, 2017

December 14, 2020

October 2, 2024
146 148 150 152 154

July 22, 2028

May 9, 2032

February 27, 2036

December 15, 2039

October 3, 2043
156

July 22, 2047

See also[edit]

References[edit]

  1. ^ "An annular solar eclipse on October 2, 2024". earthsky.org. October 1, 2024. Retrieved April 9, 2024.
  2. ^ "What the Eclipse Will Look Like near the Maximum Point". Time and Date. Retrieved May 12, 2024.
  3. ^ Carter, Jamie (April 9, 2024). "Annular solar eclipse 2024: Everything you need to know about the next solar eclipse". Space.com. Retrieved May 12, 2024.
  4. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Archived from the original on September 7, 2019. Retrieved October 6, 2018.
  5. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.
  6. ^ "NASA - Catalog of Solar Eclipses of Saros 144". eclipse.gsfc.nasa.gov.

External links[edit]