Solar eclipse of May 9, 1910
Solar eclipse of May 9, 1910 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.9437 |
Magnitude | 1.06 |
Maximum eclipse | |
Duration | 255 s (4 min 15 s) |
Coordinates | 48°12′S 125°12′E / 48.2°S 125.2°E |
Max. width of band | 594 km (369 mi) |
Times (UTC) | |
Greatest eclipse | 5:42:13 |
References | |
Saros | 117 (63 of 71) |
Catalog # (SE5000) | 9304 |
A total solar eclipse occurred on May 9, 1910. 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 was visible from part of Wilkes Land in Antarctica and Tasmania in Australia.
Related eclipses
Solar eclipses of 1910–1913
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 eclipse on August 31, 1913 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1910 to 1913 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
117 | May 9, 1910 Total |
−0.9437 | 122 | November 2, 1910 Partial |
1.0603 | |
127 | April 28, 1911 Total |
−0.2294 | 132 | October 22, 1911 Annular |
0.3224 | |
137 | April 17, 1912 Hybrid |
0.528 | 142 | October 10, 1912 Total |
−0.4149 | |
147 | April 6, 1913 Partial |
1.3147 | 152 | September 30, 1913 Partial |
−1.1005 |
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).
22 eclipse events between December 13, 1898 and July 20, 1982 | ||||
---|---|---|---|---|
December 13–14 | October 1–2 | July 20–21 | May 9 | February 24–25 |
111 | 113 | 115 | 117 | 119 |
December 13, 1898 |
July 21, 1906 |
May 9, 1910 |
February 25, 1914 | |
121 | 123 | 125 | 127 | 129 |
December 14, 1917 |
October 1, 1921 |
July 20, 1925 |
May 9, 1929 |
February 24, 1933 |
131 | 133 | 135 | 137 | 139 |
December 13, 1936 |
October 1, 1940 |
July 20, 1944 |
May 9, 1948 |
February 25, 1952 |
141 | 143 | 145 | 147 | 149 |
December 14, 1955 |
October 2, 1959 |
July 20, 1963 |
May 9, 1967 |
February 25, 1971 |
151 | 153 | 155 | ||
December 13, 1974 |
October 2, 1978 |
July 20, 1982 |
References
- ^ 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.
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC