Jump to content

Solar eclipse of August 31, 1989

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by 191.178.53.96 (talk) at 15:22, 14 June 2020 (→‎Related eclipses). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Solar eclipse of August 31, 1989
Map
Type of eclipse
NaturePartial
Gamma−1.1928
Magnitude0.6344
Maximum eclipse
Coordinates61°18′S 23°36′E / 61.3°S 23.6°E / -61.3; 23.6
Times (UTC)
Greatest eclipse5:31:47
References
Saros154 (5 of 71)
Catalog # (SE5000)9485

A partial solar eclipse occurred on August 31, 1989. 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.

Eclipses of 1989

Solar eclipses of 1986–1989

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 1986 to 1989
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
119 April 9, 1986

Partial
−1.0822 124 October 3, 1986

Hybrid
0.9931
129 March 29, 1987

Hybrid
−0.3053 134 September 23, 1987

Annular
0.2787
139 March 18, 1988

Total
0.4188 144 September 11, 1988

Annular
−0.4681
149 March 7, 1989

Partial
1.0981 154 August 31, 1989

Partial
−1.1928

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).

References

  1. ^ 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.