Solar eclipse of October 23, 1957
A total solar eclipse occurred on October 23, 1957. 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 total solar eclipse is non-central because gamma is between 0.9972 and 1.0260.
Solar eclipse of October 23, 1957 | |
---|---|
Map | |
Type of eclipse | |
Nature | Total |
Gamma | 1.0022 |
Magnitude | 1.0013 |
Maximum eclipse | |
Duration | - |
Coordinates | 71.2°S 23.1°W |
Max. width of band | - km |
Times (UTC) | |
Greatest eclipse | 4:54:02 |
References | |
Saros | 123 (50 of 70) |
Catalog # (SE5000) | 9415 |
Related eclipses
Solar eclipses of 1957–1960
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]
Solar eclipse series sets from 1957–1960 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
Saros | Map | Saros | Map | |
118 | 1957 April 30 Annular (non-central) |
123 | 1957 October 23 Total (non-central) | |
128 | 1958 April 19 Annular |
133 | 1958 October 12 Total | |
138 | 1959 April 8 Annular |
143 | 1959 October 2 Total | |
148 | 1960 March 27 Partial |
153 | 1960 September 20 Partial |
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.
22 eclipse events between January 5, 1935 and August 11, 2018 | ||||
---|---|---|---|---|
January 4-5 | October 23-24 | August 10-12 | May 30-31 | March 18-19 |
111 | 113 | 115 | 117 | 119 |
January 5, 1935 |
August 12, 1942 |
May 30, 1946 |
March 18, 1950 | |
121 | 123 | 125 | 127 | 129 |
January 5, 1954 |
October 23, 1957 |
August 11, 1961 |
May 30, 1965 |
March 18, 1969 |
131 | 133 | 135 | 137 | 139 |
January 4, 1973 |
October 23, 1976 |
August 10, 1980 |
May 30, 1984 |
March 18, 1988 |
141 | 143 | 145 | 147 | 149 |
January 4, 1992 |
October 24, 1995 |
August 11, 1999 |
May 31, 2003 |
March 19, 2007 |
151 | 153 | 155 | 157 | 159 |
January 4, 2011 |
October 23, 2014 |
August 11, 2018 |
Notes
- 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.
References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC