Solar eclipse of September 2, 2035

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Solar eclipse of September 2, 2035
SE2035Sep02T.png
Map
Type of eclipse
NatureTotal
Gamma0.3727
Magnitude1.032
Maximum eclipse
Duration174 sec (2 m 54 s)
Coordinates29°06′N 158°00′E / 29.1°N 158°E / 29.1; 158
Max. width of band116 km (72 mi)
Times (UTC)
Greatest eclipse1:56:46
References
Saros145 (23 of 77)
Catalog # (SE5000)9586

A total solar eclipse will occur on September 2, 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Visibility[edit]

Animation of the eclipse shadow. The dot in the center represents the path of totality.

The path of totality will cross two Asian capital cities, Beijing, China and Pyongyang, North Korea, and will pass north of a third, Tokyo, Japan.[1]

Related eclipses[edit]

Solar eclipses of 2033-2036[edit]

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.[2]

Saros 145[edit]

This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon’s ascending node.

Metonic series[edit]

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.

References[edit]

  1. ^ Kennedy, Kelsey (August 21, 2017). "If You Missed This Year's Eclipse, Chase Another". Atlas Obscura. Retrieved December 12, 2017.
  2. ^ 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.

External links[edit]