Solar eclipse of June 8, 1937

Solar eclipse of June 8, 1937
Map
Type of eclipse
Nature	Total
Gamma	−0.2253
Magnitude	1.0751
Maximum eclipse
Duration	424 s (7 min 4 s)
Coordinates	9.9°N 130.5°W / 9.9; -130.5
Max. width of band	250 km (160 mi)
Times (UTC)
Greatest eclipse	20:41:02
References
Saros	136 (33 of 71)
Catalog # (SE5000)	9369

A total solar eclipse occurred on June 8, 1937. Template:Total solar eclipse summary

The path of totality crossed the pacific ocean starting in Micronesia, and ending at sunset in western South America.

Related eclipses

Solar eclipses 1935-1938

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 February 3, 1935 and July 30, 1935 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1935 to 1938
Ascending node				Descending node
Saros	Map	Gamma		Saros	Map	Gamma
111	January 5, 1935 Partial	−1.5381		116	June 30, 1935 Partial	1.3623
121	December 25, 1935 Annular	−0.9228		126	June 19, 1936 Total	0.5389
131	December 13, 1936 Annular	−0.2493		136 Totality in Kanton Island, Kiribati	June 8, 1937 Total	−0.2253
141	December 2, 1937 Annular	0.4389		146	May 29, 1938 Total	−0.9607
151	November 21, 1938 Partial	1.1077

Saros 136

This eclipse is a part of Saros series 136, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 14, 1360. It contains annular eclipses from September 8, 1504 through November 12, 1594; hybrid eclipses from November 22, 1612 through January 17, 1703; and total eclipses from January 27, 1721 through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622. 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 annularity was produced by member 9 at 32 seconds on September 8, 1504, and the longest duration of totality was produced by member 34 at 7 minutes, 7.74 seconds on June 20, 1955. All eclipses in this series occur at the Moon’s descending node of orbit.

Series members 26–47 occur between 1801 and 2200:
26	27	28
March 24, 1811	April 3, 1829	April 15, 1847
29	30	31
April 25, 1865	May 6, 1883	May 18, 1901
32	33	34
May 29, 1919	June 8, 1937	June 20, 1955
35	36	37
June 30, 1973	July 11, 1991	July 22, 2009
38	39	40
August 2, 2027	August 12, 2045	August 24, 2063
41	42	43
September 3, 2081	September 14, 2099	September 26, 2117
44	45	46
October 7, 2135	October 17, 2153	October 29, 2171
47
November 8, 2189

References

• Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
  • Google interactive map
  • Besselian elements
• Fotos of Solar Corona June 8, 1937