Solar eclipse of April 11, 2070

Solar eclipse of April 11, 2070
Map
Type of eclipse
Nature	Total
Gamma	0.3652
Magnitude	1.0472
Maximum eclipse
Duration	244 s (4 min 4 s)
Coordinates	29.1°N 135.1°E / 29.1; 135.1
Max. width of band	168 km (104 mi)
Times (UTC)
Greatest eclipse	2:36:09
References
Saros	130 (55 of 73)
Catalog # (SE5000)	9665

A total solar eclipse will occur on April 11, 2070. 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.

Related eclipses

Solar eclipses 2069–2072

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 eclipse on May 20, 2069 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 2069 to 2072
Descending node				Ascending node
Saros	Map	Gamma		Saros	Map	Gamma
120	April 21, 2069 Partial	1.0624		125	October 15, 2069 Partial	−1.2524
130	April 11, 2070 Total	0.3652		135	October 4, 2070 Annular	−0.495
140	March 31, 2071 Annular	−0.3739		145	September 23, 2071 Total	0.262
150	March 19, 2072 Partial	−1.1405		155	September 12, 2072 Total	0.9655

Saros 130

This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of totality was produced by member 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’s descending node of orbit.

Series members 41–62 occur between 1801 and 2200:
41	42	43
November 9, 1817	November 20, 1835	November 30, 1853
44	45	46
December 12, 1871	December 22, 1889	January 3, 1908
47	48	49
January 14, 1926	January 25, 1944	February 5, 1962
50	51	52
February 16, 1980	February 26, 1998	March 9, 2016
53	54	55
March 20, 2034	March 30, 2052	April 11, 2070
56	57	58
April 21, 2088	May 3, 2106	May 14, 2124
59	60	61
May 25, 2142	June 4, 2160	June 16, 2178
62
June 26, 2196

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Inex series members between 1901 and 2100:
July 20, 1925 (Saros 125)	June 30, 1954 (Saros 126)	June 11, 1983 (Saros 127)
May 20, 2012 (Saros 128)	April 30, 2041 (Saros 129)	April 11, 2070 (Saros 130)
March 21, 2099 (Saros 131)

References

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