Solar eclipse of August 21, 2036

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Solar eclipse of August 21, 2036
SE2036Aug21P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0825
Magnitude 0.8622
Maximum eclipse
Coordinates 71°06′N47°00′E / 71.1°N 47°E / 71.1; 47
Times (UTC)
Greatest eclipse17:25:45
References
Saros 155 (7 of 71)
Catalog # (SE5000) 9589

A partial solar eclipse will occur on Thursday, August 21, 2036. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

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SE2036Aug21P.gif
Animated path

Solar eclipses of 2033–2036

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. [1]

Saros 155 series

It is a part of Saros cycle 155, repeating every 18 years, 11 days (223 synodic months), contains 71 events. The series started with a partial solar eclipse on June 17, 1928. It has total eclipses from September 12, 2072 to August 30, 2649. The series also has 3 hybrid eclipses from September 10, 2667 to October 3, 2703 and 20 annular eclipses from October 13, 2721 to May 8, 3064.

The series ends at member 71 as a partial eclipse on July 24, 3190. The longest total eclipses will be on October 26, 2144 and on November 7, 2162, at 4 minutes and 5 seconds. [2]

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.

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References

  1. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.