Solar eclipse of April 8, 1902
Map
Type of eclipse
NaturePartial
Gamma1.5024
Magnitude0.0643
Maximum eclipse
Coordinates71°42′N 142°24′W / 71.7°N 142.4°W / 71.7; -142.4
Times (UTC)
Greatest eclipse14:05:06
References
Saros108 (76 of 76)
Catalog # (SE5000)9286

A partial solar eclipse occurred on April 8, 1902.[1][2] 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This was the 76th and final event from Solar Saros 108.

Solar eclipses 1902–1907

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.[3]

Solar eclipse series sets from 1902–1907
Descending node   Ascending node
108April 8, 1902

Partial
113October 1, 1902
118March 29, 1903

Annular
123September 21, 1903

Total
128March 17, 1904

Annular
133September 9, 1904

Total
138March 6, 1905

Annular
143August 30, 1905

Total
148February 23, 1906

Partial
153August 20, 1906

Partial

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).

Notes

  1. "There was an eclipse of the sun to-day". The Gazette. Cedar Rapids, Iowa. 1902-04-08. p. 3. Retrieved 2023-10-27 via Newspapers.com.
  2. "City items". The Dayton Herald. Dayton, Ohio. 1902-04-09. p. 10. Retrieved 2023-10-27 via Newspapers.com.
  3. 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

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