Solar eclipse of May 11, 2097

A total solar eclipse will occur on May 11, 2097. 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.

Solar eclipse of May 11, 2097
Map
Type of eclipse
NatureTotal
Gamma0.8516
Magnitude1.0538
Maximum eclipse
Duration190 sec (3 m 10 s)
Coordinates67.4°N 149.5°W / 67.4; -149.5
Max. width of band339 km (211 mi)
Times (UTC)
Greatest eclipse
34:31
References
Saros149 (25 of 71)
Catalog # (SE5000)9726

Solar eclipses 2094–2098

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]

119June 13, 2094

Partial
124December 7, 2094

Partial
129June 2, 2095

Total
134November 27, 2095

Annular
139May 22, 2096

Total
144November 15, 2096

Annular
149May 11, 2097

Total
154November 4, 2097

Annular
  164October 24, 2098

Partial

Saros 149

Solar saros 149, repeating every about 18 years and 11 days, contains 71 events. The series started with a partial solar eclipse on August 21, 1664. It has total eclipses from April 9, 2043, to October 2, 2331. The series ends at member 71 as a partial eclipse on September 28, 2926. The longest total eclipse will be on July 17, 2205, at 4 minutes and 10 seconds.[2]

Notes

  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.

References

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