Solar Saros 137
Saros cycle series 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 events. 55 of these are umbral eclipses and other 15 of these are partial solar eclipses. All eclipses in this series occurs at the Moon's ascending node. This solar saros is linked to Lunar Saros 130. 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). Summary. 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. 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. List of umbral eclipses. Solar Saros 137 has 55 umbral eclipses between 1533 and 2507. The total duration is almost one millennium, or about within 974 years.