Solar eclipse of August 22, 1998

Solar eclipse of August 22, 1998
Map
Type of eclipse
Nature Annular
Gamma -0.2644
Magnitude 0.9734
Maximum eclipse
Duration 194 sec (3 m 14 s)
Coordinates 3°00′S 145°24′E / 3°S 145.4°E / -3; 145.4
Max. width of band 99 km (62 mi)
Times (UTC)
Greatest eclipse 2:07:11
References
Saros 135 (38 of 71)
Catalog # (SE5000) 9504

An annular solar eclipse occurred on August 22, 1998. 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 kilometres wide.

Images

Related eclipses

Solar eclipses 1997-2000

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.

Solar eclipse series sets from 1997 to 2000
Ascending node   Descending node
SarosMap SarosMap
120

Chita, Russia
March 9, 1997

Total
125September 2, 1997

Partial
130February 26, 1998

Total
135August 22, 1998

Annular
140February 16, 1999

Annular
145

Totality Cornwall, United Kingdom
August 11, 1999

Total
150February 5, 2000

Partial
155July 31, 2000

Partial
Partial solar eclipses on July 1, 2000 and December 25, 2000 occur in the next lunar year eclipse set.

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

    Photos:

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