Jump to content

Solar eclipse of April 8, 1902

From Wikipedia, the free encyclopedia
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 at the Moon's descending node of orbit on Tuesday, April 8, 1902,[1][2] with a magnitude of 0.0643. 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.

Related eclipses[edit]

Eclipses in 1902[edit]

Solar Saros 108[edit]

Solar eclipses of 1902–1906[edit]

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]

The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1902 to 1906
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
108 April 8, 1902

Partial
1.5024 113 October 1, 1902
118 March 29, 1903

Annular
0.8413 123 September 21, 1903

Total
−0.8967
128 March 17, 1904

Annular
0.1299 133 September 9, 1904

Total
−0.1625
138 March 6, 1905

Annular
−0.5768 143
August 30, 1905

Total
0.5708
148 February 23, 1906

Partial
−1.2479 153 August 20, 1906

Partial
1.3731

Saros 108[edit]

This eclipse is a part of Saros series 108, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on January 4, 550 AD. It contains annular eclipses from May 13, 766 AD through December 4, 1108; hybrid eclipses from December 15, 1126 through January 28, 1199; and total eclipses from February 7, 1217 through August 11, 1523. The series ends at member 76 as a partial eclipse on April 8, 1902. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 13 at 3 minutes, 35 seconds on May 13, 766 AD, and the longest duration of totality was produced by member 46 at 5 minutes, 7 seconds on May 5, 1361. All eclipses in this series occur at the Moon’s descending node of orbit.[4]

Metonic series[edit]

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[edit]

  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.
  4. ^ "NASA - Catalog of Solar Eclipses of Saros 108". eclipse.gsfc.nasa.gov.

References[edit]


External links[edit]