Solar eclipse of August 31, 1970
Solar eclipse of August 31, 1970 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.5364 |
Magnitude | 0.94 |
Maximum eclipse | |
Duration | 407 s (6 min 47 s) |
Coordinates | 20°18′S 164°00′W / 20.3°S 164°W |
Max. width of band | 258 km (160 mi) |
Times (UTC) | |
Greatest eclipse | 21:55:30 |
References | |
Saros | 144 (14 of 70) |
Catalog # (SE5000) | 9443 |
An annular solar eclipse occurred on August 31, 1970. 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 wide.
Related eclipses
Solar eclipses of 1968-1971
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 July 22, 1971 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1968 to 1971 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | March 28, 2968![]() Partial |
−1.037 | 124 | September 22, 1968![]() Total |
0.9451 | |
129 | March 18, 1969![]() Annular |
−0.2704 | 134 | September 11, 1969![]() Annular |
0.2201 | |
139![]() Totality in Williamston, NC USA |
March 7, 1970![]() Total |
0.4473 | 144 | August 31, 1970![]() Annular |
−0.5364 | |
149 | February 25, 1971![]() Partial |
1.1188 | 154 | August 20, 1971![]() Partial |
−1.2659 |
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
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