Solar eclipse of July 24, 2074

Solar eclipse of July 24, 2074
Map
Type of eclipse
Nature	Annular
Gamma	−0.1242
Magnitude	0.9838
Maximum eclipse
Duration	117 s (1 min 57 s)
Coordinates	12.8°N 133.7°E / 12.8; 133.7
Max. width of band	58 km (36 mi)
Times (UTC)
Greatest eclipse	3:10:32
References
Saros	137 (39 of 70)
Catalog # (SE5000)	9674

An annular solar eclipse will occur on July 24, 2074. 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.

Related eclipses

Solar eclipses 2073–2076

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.

The partial solar eclipses on June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2073 to 2076
Descending node				Ascending node
Saros	Map	Gamma		Saros	Map	Gamma
122	February 7, 2073 Partial	1.1651		127	August 3, 2073 Total	−0.8763
132	January 27, 2074 Annular	0.4251		137	July 24, 2074 Annular	−0.1242
142	January 16, 2075 Total	−0.2799		147	July 13, 2075 Annular	0.6583
152	January 6, 2076 Total	−0.9373		157	July 1, 2076 Partial	1.4005

Saros 137

It is a part of Saros cycle 137, repeating every 18 years, 11 days, containing 70 events. The series started with 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). That's almost 1 millennium!

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

External links

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