Solar eclipse of August 3, 2092

Solar eclipse of August 3, 2092
Map
Type of eclipse
Nature	Annular
Gamma	−0.2044
Magnitude	0.9794
Maximum eclipse
Duration	151 sec (2 m 31 s)
Coordinates	5°36′N 30°18′E / 5.6°N 30.3°E / 5.6; 30.3
Max. width of band	75 km (47 mi)
Times (UTC)
Greatest eclipse	9:59:33
References
Saros	137 (40 of 70)
Catalog # (SE5000)	9715

An annular solar eclipse will occur on August 3, 2092. 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 kilometers wide.

Related eclipses

Solar eclipses 2091–2094

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 eclipses 2091–2094
122	February 18, 2091 Partial	127	August 15, 2091 Total
132	February 7, 2092 Annular	137	August 3, 2092 Annular
142	January 27, 2093 Total	147	July 23, 2093 Annular
152	January 16, 2094 Total	157	July 12, 2094 Partial

Saros 137

It is a part of Saros cycle 137, repeating every 18 years, 11 days, containing 70 events. The series started with a partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533, through December 6, 1695, first set of hybrid eclipses from December 17, 1713, through February 11, 1804, first set of annular eclipses from February 21, 1822, through March 25, 1876, second set of hybrid eclipses from April 6, 1894, through April 28, 1930, and second set of annular eclipses from May 9, 1948, through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569. Solar Saros 137 has 55 umbral eclipses from August 20, 1533, through April 13, 2507 (973.62 years).

Series members 30–40 occur between 1901 and 2100:
30	31	32
April 17, 1912	April 28, 1930	May 9, 1948
33	34	35
May 20, 1966	May 30, 1984	June 10, 2002
36	37	38
June 21, 2020	July 2, 2038	July 12, 2056
39	40
July 24, 2074	August 3, 2092

Notes

References

• Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
  • Google interactive map
  • Besselian elements

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This page was last edited on 19 June 2023, at 06:24