Solar eclipse of October 14, 2023 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.3753 |
Magnitude | 0.952 |
Maximum eclipse | |
Duration | 317 s (5 min 17 s) |
Coordinates | 11°24′N83°06′W / 11.4°N 83.1°W |
Max. width of band | 187 km (116 mi) |
Times (UTC) | |
Greatest eclipse | 18:00:41 |
References | |
Saros | 134 (44 of 71) |
Catalog # (SE5000) | 9560 |
An annular solar eclipse occurred on October 14, 2023. [1] [2] [3] [4] [5] [ excessive citations ] 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 or miles wide. Occurring only 4.6 days after apogee (Apogee on October 10, 2023), the Moon's apparent diameter was small.
The path of the eclipse crossed the United States beginning in Oregon, entering at Dunes City, and passing over Newport, Crater Lake National Park, Eugene (passing over University of Oregon), and Medford. [6] After passing over the northeast corner of California (in Modoc National Forest), it traveled through Nevada (passing over Black Rock Desert, Winnemucca and Elko) and Utah (passing over Canyonlands National Park, Glen Canyon National Recreation Area, and Bluff). [6] After that, it covered the northeast corner of Arizona (including Kayenta) and the southwest corner of Colorado (including Cortez and the Ute Mountain Reservation). [6] In New Mexico, it passed over Farmington, Albuquerque, Santa Fe, Roswell, Hobbs, and Carlsbad. [6] Afterwards, it entered Texas, passing over Midland, Odessa, San Angelo, Kerrville, San Antonio and Corpus Christi before entering the Gulf of Mexico. [6] This was the second annular eclipse visible from Albuquerque in 11 years, where it crossed the path of the May 2012 eclipse. It also coincided with the last day of the Albuquerque International Balloon Fiesta.
A total solar eclipse crossed the United States in April 2024 (12 states) (Saros 139, Ascending Node), and a future solar eclipse will cross in August 2045 (10 states) (Saros 136, Descending Node). An annular solar eclipse will occur in June 2048 (9 states) (Saros 128, Descending Node).
In Mexico, the eclipse path passed over the Yucatan Peninsula, covering Campeche City in Campeche State, Oxkutzcab in Yucatan State (coming close to Mérida), and Chetumal in Quintana Roo. [6]
In Western Cuba, Cayman Islands, and Jamaica all saw a partial eclipse (50% and above). The greatest of the partial eclipse was seen over Western Cuba and the Cayman Islands.
In Belize, the eclipse passed over Belmopan and Belize City before leaving land again; when it entered in Honduras, it passed over La Ceiba and Catacamas, and in Nicaragua it passed over Bluefields. [6] The point of greatest eclipse occurred near the coast of Nicaragua. [6] After that, in Costa Rica it passed over Limon, and in Panama it passed over Santiago and came close to Panama City. Its point of greatest duration occurred just off the coast of Nata, Panama. [6]
In South America, the eclipse entered Colombia from the Pacific Ocean and passed over Pereira, Armenia, Cali, Ibagué and Neiva. [6] In Brazil, it passed over the states of Amazonas (covering Fonte Boa, Tefé and Coari), Pará (covering Parauapebas and Xinguara), Tocantins (Araguaína) Maranhão (Balsas), Piauí (Picos), Ceará (Juazeiro do Norte), Pernambuco (Araripina), Paraíba (João Pessoa) and Rio Grande do Norte (Natal) before ending in the Atlantic Ocean. [6]
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. [7]
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Map | Gamma | Saros | Map | Gamma | |
119 Partial from CTIO, Chile | 2022 April 30 Partial | −1.19008 | 124 Partial from Saratov, Russia | 2022 October 25 Partial | 1.07014 | |
129 Total from East Timor | 2023 April 20 Hybrid | −0.39515 | 134 Annular from Campeche, Mexico | 2023 October 14 Annular | 0.37534 | |
139 Total from Indianapolis, USA | 2024 April 8 Total | 0.34314 | 144 | 2024 October 2 Annular | −0.35087 | |
149 | 2025 March 29 Partial | 1.04053 | 154 | 2025 September 21 Partial | −1.06509 |
It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428. All eclipses in this series occur at the Moon’s descending node. [8]
Series members 32–48 occur between 1801 and 2100: | ||
---|---|---|
32 | 33 | 34 |
June 6, 1807 | June 16, 1825 | June 27, 1843 |
35 | 36 | 37 |
July 8, 1861 | July 19, 1879 | July 29, 1897 |
38 | 39 | 40 |
August 10, 1915 | August 21, 1933 | September 1, 1951 |
41 | 42 | 43 |
September 11, 1969 | September 23, 1987 | October 3, 2005 |
44 | 45 | 46 |
October 14, 2023 | October 25, 2041 | November 5, 2059 |
47 | 48 | |
November 15, 2077 | November 27, 2095 |
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: | ||
---|---|---|
January 3, 1908 (Saros 130) | December 13, 1936 (Saros 131) | November 23, 1965 (Saros 132) |
November 3, 1994 (Saros 133) | October 14, 2023 (Saros 134) | September 22, 2052 (Saros 135) |
September 3, 2081 (Saros 136) |
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 | |||
---|---|---|---|
September 21, 1903 (Saros 123) | August 21, 1914 (Saros 124) | July 20, 1925 (Saros 125) | |
June 19, 1936 (Saros 126) | May 20, 1947 (Saros 127) | April 19, 1958 (Saros 128) | |
March 18, 1969 (Saros 129) | February 16, 1980 (Saros 130) | January 15, 1991 (Saros 131) | |
December 14, 2001 (Saros 132) | November 13, 2012 (Saros 133) | October 14, 2023 (Saros 134) | |
September 12, 2034 (Saros 135) | August 12, 2045 (Saros 136) | July 12, 2056 (Saros 137) | |
June 11, 2067 (Saros 138) | May 11, 2078 (Saros 139) | April 10, 2089 (Saros 140) | |
March 10, 2100 (Saros 141) |
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. [9]
Octon series with 21 events between May 21, 1993 and August 2, 2065 | ||||
---|---|---|---|---|
May 20–21 | March 8–9 | December 25–26 | October 13–14 | August 1–2 |
98 | 100 | 102 | 104 | 106 |
May 21, 1955 | March 9, 1959 | December 26, 1962 | October 14, 1966 | August 2, 1970 |
108 | 110 | 112 | 114 | 116 |
May 21, 1974 | March 9, 1978 | December 26, 1981 | October 14, 1985 | August 1, 1989 |
118 | 120 | 122 | 124 | 126 |
May 21, 1993 | March 9, 1997 | December 25, 2000 | October 14, 2004 | August 1, 2008 |
128 | 130 | 132 | 134 | 136 |
May 20, 2012 | March 9, 2016 | December 26, 2019 | October 14, 2023 | August 2, 2027 |
138 | 140 | 142 | 144 | 146 |
May 21, 2031 | March 9, 2035 | December 26, 2038 | October 14, 2042 | August 2, 2046 |
148 | 150 | 152 | 154 | 156 |
May 20, 2050 | March 9, 2054 | December 26, 2057 | October 13, 2061 | August 2, 2065 |
158 | 160 | 162 | 164 | 166 |
May 20, 2069 | March 8, 2073 | December 26, 2076 | October 13, 2080 | August 1, 2084 |
During the annular and total eclipses of 2023 and 2024, the GLOBE Program (Global Learning and Observations to Benefit the Environment) through the GLOBE Observer app will seek to collect information on air temperature, clouds, and wind. During the 2017 eclipse, citizen scientists contributed with over 80,000 observations of air temperature and 20,000 cloud observations. [10] [11]
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