Solar eclipse of September 21, 1903 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.8967 |
Magnitude | 1.0316 |
Maximum eclipse | |
Duration | 132 s (2 min 12 s) |
Coordinates | 58°00′S77°12′E / 58°S 77.2°E |
Max. width of band | 241 km (150 mi) |
Times (UTC) | |
Greatest eclipse | 4:39:52 |
References | |
Saros | 123 (47 of 70) |
Catalog # (SE5000) | 9289 |
A total solar eclipse occurred on September 21, 1903. [1] [2] [3] 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.
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. [4]
Solar eclipse series sets from 1902 to 1907 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
108 | April 8, 1902 Partial | 113 | October 1, 1902 | |
118 | March 29, 1903 Annular | 123 | September 21, 1903 Total | |
128 | March 17, 1904 Annular | 133 | September 9, 1904 Total | |
138 | March 6, 1905 Annular | 143 | August 30, 1905 Total | |
148 | February 23, 1906 Partial | 153 | August 20, 1906 Partial |
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.
In the 19th century:
Inex series members between 1901 and 2100: | ||
---|---|---|
September 21, 1903 (Saros 123) | August 31, 1932 (Saros 124) | August 11, 1961 (Saros 125) |
July 22, 1990 (Saros 126) | July 2, 2019 (Saros 127) | June 11, 2048 (Saros 128) |
May 22, 2077 (Saros 129) |
In the 22nd century:
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) |
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