Solar eclipse of March 9, 2035

Solar eclipse of March 9, 2035
Map
Type of eclipse
Nature Annular
Gamma -0.4368
Magnitude 0.9919
Maximum eclipse
Duration 48 sec (0 m 48 s)
Coordinates 29°00′S 154°54′W / 29°S 154.9°W / -29; -154.9
Max. width of band 31 km (19 mi)
Times (UTC)
Greatest eclipse 23:05:54
References
Saros 140 (30 of 71)
Catalog # (SE5000) 9585

An annular solar eclipse will occur on March 9, 2035. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

Images


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]

Metonic series

This eclipse is a member of the Octon eclipse series, which includes 21 eclipses occurring in approximately 4 year intervals from May 21, 1993 to August 2, 2065.[2]

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

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. ↑ Freeth, Tony. "Note S1: Eclipses & Predictions". plos.org. Retrieved 6 October 2018.


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