Solar eclipse of September 11, 2007

A partial solar eclipse occurred on September 11, 2007. 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.

Solar eclipse of September 11, 2007
Map
Type of eclipse
NaturePartial
Gamma-1.1255
Magnitude0.7507
Maximum eclipse
Coordinates61°S 90.2°W / -61; -90.2
Times (UTC)
Greatest eclipse12:32:24
References
Saros154 (6 of 71)
Catalog # (SE5000)9524

Images

Eclipses of 2007

Solar eclipses 2004–2007

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]

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 descending node.

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.
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