Solar eclipse of May 11, 2097

Last updated
Solar eclipse of May 11, 2097
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Map
Type of eclipse
NatureTotal
Gamma 0.8516
Magnitude 1.0538
Maximum eclipse
Duration190 sec (3 m 10 s)
Coordinates 67°24′N149°30′W / 67.4°N 149.5°W / 67.4; -149.5
Max. width of band339 km (211 mi)
Times (UTC)
Greatest eclipse
34:31
References
Saros 149 (25 of 71)
Catalog # (SE5000) 9726

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.

Contents

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]

119 June 13, 2094
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Partial
124 December 7, 2094
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Partial
129 June 2, 2095
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Total
134 November 27, 2095
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Annular
139 May 22, 2096
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Total
144 November 15, 2096
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Annular
149 May 11, 2097
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Total
154 November 4, 2097
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Annular
 164 October 24, 2098
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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.

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References