Solar 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).

Series members 30–46 occur between 1901 and 2200:
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	41
July 24, 2074	August 3, 2092	August 15, 2110
42	43	44
August 25, 2128	September 6, 2146	September 16, 2164
45	46
September 27, 2182	October 9, 2200

Solar Saros series 137, repeating every 18 years and 11 days, has a total of 70 solar eclipse events including 12 central solar eclipses with a penumbral internal contact, between 1948 and 2146. The penumbra northern limit started in 1948 and will end on 2633, while the penumbra southern limit started in 1389 and will end in 2146.

Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 137 appears in the following table.

Solar Saros 137 has 55 umbral eclipses between 1533 and 2507. The total duration is almost one millennium, or about within 974 years.

• Saros cycle 137 - Information and visualization

• http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros137.html