Solar eclipse of July 13, 2037 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.7246 |
Magnitude | 1.0413 |
Maximum eclipse | |
Duration | 238 s (3 min 58 s) |
Coordinates | 24°48′S 139°06′E / 24.8°S 139.1°E |
Max. width of band | 201 km (125 mi) |
Times (UTC) | |
Greatest eclipse | 2:40:36 |
References | |
Saros | 127 (59 of 82) |
Catalog # (SE5000) | 9591 |
A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, July 13, 2037, with a magnitude of 1.0413. 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. Totality will pass through the centre of Brisbane and the Gold Coast, as well as Geraldton, Western Australia.
Images
Related eclipses
Eclipses in 2037
- A partial solar eclipse on January 16, 2037.
- A total lunar eclipse on January 31, 2037.
- A total solar eclipse on July 13, 2037.
- A partial lunar eclipse on July 27, 2037.
Metonic
- Preceded by: Solar eclipse of September 23, 2033
- Followed by: Solar eclipse of April 30, 2041
Tzolkinex
- Preceded by: Solar eclipse of June 1, 2030
- Followed by: Solar eclipse of August 23, 2044
Half-Saros
- Preceded by: Lunar eclipse of July 6, 2028
- Followed by: Lunar eclipse of July 18, 2046
Tritos
- Preceded by: Solar eclipse of August 12, 2026
- Followed by: Solar eclipse of June 11, 2048
Solar Saros 127
- Preceded by: Solar eclipse of July 2, 2019
- Followed by: Solar eclipse of July 24, 2055
Inex
- Preceded by: Solar eclipse of August 1, 2008
- Followed by: Solar eclipse of June 22, 2066
Triad
- Preceded by: Solar eclipse of September 12, 1950
- Followed by: Solar eclipse of May 14, 2124
Solar eclipses of 2036–2039
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]
The partial solar eclipses on February 27, 2036 and August 21, 2036 occur in the previous lunar year eclipse set.
Solar eclipse series sets from 2036 to 2039 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
117 | July 23, 2036 Partial |
−1.425 | 122 | January 16, 2037 Partial |
1.1477 | |
127 | July 13, 2037 Total |
−0.7246 | 132 | January 5, 2038 Annular |
0.4169 | |
137 | July 2, 2038 Annular |
0.0398 | 142 | December 26, 2038 Total |
−0.2881 | |
147 | June 21, 2039 Annular |
0.8312 | 152 | December 15, 2039 Total |
−0.9458 |
Saros 127
This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. 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 totality was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]
Series members 46–68 occur between 1801 and 2200: | ||
---|---|---|
46 | 47 | 48 |
February 21, 1803 |
March 4, 1821 |
March 15, 1839 |
49 | 50 | 51 |
March 25, 1857 |
April 6, 1875 |
April 16, 1893 |
52 | 53 | 54 |
April 28, 1911 |
May 9, 1929 |
May 20, 1947 |
55 | 56 | 57 |
May 30, 1965 |
June 11, 1983 |
June 21, 2001 |
58 | 59 | 60 |
July 2, 2019 |
July 13, 2037 |
July 24, 2055 |
61 | 62 | 63 |
August 3, 2073 |
August 15, 2091 |
August 26, 2109 |
64 | 65 | 66 |
September 6, 2127 |
September 16, 2145 |
September 28, 2163 |
67 | 68 | |
October 8, 2181 |
October 19, 2199 |
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 13, 2018 and July 12, 2094 | ||||
---|---|---|---|---|
July 12–13 | April 30–May 1 | February 16–17 | December 5–6 | September 22–23 |
117 | 119 | 121 | 123 | 125 |
July 13, 2018 |
April 30, 2022 |
February 17, 2026 |
December 5, 2029 |
September 23, 2033 |
127 | 129 | 131 | 133 | 135 |
July 13, 2037 |
April 30, 2041 |
February 16, 2045 |
December 5, 2048 |
September 22, 2052 |
137 | 139 | 141 | 143 | 145 |
July 12, 2056 |
April 30, 2060 |
February 17, 2064 |
December 6, 2067 |
September 23, 2071 |
147 | 149 | 151 | 153 | 155 |
July 13, 2075 |
May 1, 2079 |
February 16, 2083 |
December 6, 2086 |
September 23, 2090 |
157 | ||||
July 12, 2094 |
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 127". eclipse.gsfc.nasa.gov.