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Solar eclipse of July 13, 2075

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Solar eclipse of July 13, 2075
Map
Type of eclipse
NatureAnnular
Gamma0.6583
Magnitude0.9467
Maximum eclipse
Duration285 s (4 min 45 s)
Coordinates63°06′N 95°12′E / 63.1°N 95.2°E / 63.1; 95.2
Max. width of band262 km (163 mi)
Times (UTC)
Greatest eclipse6:05:44
References
Saros147 (26 of 80)
Catalog # (SE5000)9676

An annular solar eclipse will occur on July 13, 2075. 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.

Eight european capitals will observe annual eclipse: Monaco, San Marino, Ljubljana, Zagreb, Vienna, Bratislava, Budapest and Moscow.

Solar eclipses 2073-2076

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]

The partial solar eclipses on June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2073 to 2076
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
122 February 7, 2073

Partial
1.1651 127 August 3, 2073

Total
−0.8763
132 January 27, 2074

Annular
0.4251 137 July 24, 2074

Annular
−0.1242
142 January 16, 2075

Total
−0.2799 147 July 13, 2075

Annular
0.6583
152 January 6, 2076

Total
−0.9373 157 July 1, 2076

Partial
1.4005

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.