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Solar Saros 133

Saros cycle series 133 for solar eclipses From Wikipedia, the free encyclopedia

Solar Saros 133
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Saros cycle series 133 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 eclipses, 53 of which are umbral (6 annular, 1 hybrid, 46 total). The first eclipse in the series was on 13 July 1219 and the last will be on 5 September 2499. The most recent eclipse was a total eclipse on 13 November 2012 and the next will be a total eclipse on 25 November 2030.

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Historic saros cycle animation

The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850[1] and the longest annular was 1 minute 14 seconds on 30 November 1453. This solar saros is linked to Lunar Saros 126.

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June 24, 1778
Series member 32
August 18, 1868
Series member 37
August 29, 1886
Series member 38
November 13, 2012
Series member 45
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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 133 appears in the following table.

More information Classification, Number ...
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All eclipses

In the following list, the Julian calendar is used for the first 21 members of the series; the Gregorian calendar is used for all the rest,[2] starting with the solar eclipse of March 7, 1598.

More information Saros, Member ...
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References

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