Solar eclipse of November 22, 1984

Solar eclipse of November 22, 1984

Map
Type of eclipse
Nature Total
Gamma -0.3132
Magnitude 1.0237
Maximum eclipse
Duration 120 sec (2 m 0 s)
Coordinates 37°48′S 173°36′W / 37.8°S 173.6°W / -37.8; -173.6
Max. width of band 85 km (53 mi)
Times (UTC)
Greatest eclipse 22:54:17
References
Saros 142 (21 of 72)
Catalog # (SE5000) 9475

A total solar eclipse occurred on November 22, 1984. 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.

Solar eclipses of 1982-1985

Each member 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.

Note: Partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1982-1985
Ascending node   Descending node
SarosMap SarosMap
117
June 21, 1982
Partial
122
December 15, 1982
Partial
127
June 11, 1983
Total
132
December 4, 1983
Annular
137
May 30, 1984
Annular
142

Partial from Gisborne, NZ

November 22, 1984
Total
147
May 19, 1985
Partial
152
November 12, 1985
Total

Saros 142

It is a part of Saros cycle 142, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on April 17, 1624. It contains one hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. The series ends at member 72 as a partial eclipse on June 5, 2904. The longest duration of totality will be 6 minutes, 34 seconds on May 28, 2291.[1]

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

References

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