The 72 eclipses in Saros 24 occur in the following order : 8P 15T 16H 26A 7P 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 24appears in the following table. Saros 24 is composed of 72 solar eclipses as follows: Solar Eclipses of Saros 24 The total duration of Saros series 24 is 1280.14 years.

The series ended with a partial eclipse in the northern hemisphere on -0854 May 14. The series began with a partial eclipse in the southern hemisphere on -2134 Apr 06. Solar eclipses of Saros 24all occur at the Moons descending node and the Moon moves northward with each eclipse. Statistics for Solar Eclipses of Saros 24 A description of each parameter in the catalog table can be found in Key to Saros Catalog of Solar Eclipses. The date and time of each eclipse is given for the instant of Greatest Eclipse.For eclipses between the years -1999 to 3000, the calendar date links to a web page containing additional details and a map showing the geographic region of eclipse visibility for that eclipse. The table below lists the concise characteristics of every solar eclipse belonging to Saros 24. For more information, see Periodicity of Solar Eclipses. The series will then produce several dozen central eclipses before ending with a group of partial eclipses near the opposite pole. The periodicity and recurrence of solar eclipses is governed by the Saros cycle, a period of approximately 6,585.3 days (18 years 11 days 8 hours).When two eclipses are separated by a period of one Saros, they share a very similar geometry.The two eclipses occur at the same node with the Moon at nearly the same distance from Earth and the same time of year due to a harmonic in three cycles of the Moon's orbit.Thus, the Saros is useful for organizing eclipses into families or series.Each series typically lasts 12 to 13 centuries and contains 70 or more eclipses.Every saros series begins with a number of partial eclipses near one of Earth's polar regions. A solar eclipse occurs whenever the Moon's shadow passes across Earth's surface.At least two solar eclipses and as many as five occur every year.

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