Solar eclipse of July 13, 2075

Last updated
Solar eclipse of July 13, 2075
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Map
Type of eclipse
NatureAnnular
Gamma 0.6583
Magnitude 0.9467
Maximum eclipse
Duration285 s (4 min 45 s)
Coordinates 63°06′N95°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
Saros 147 (26 of 80)
Catalog # (SE5000) 9676

An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, July 13, 2075, with a magnitude of 0.9467. 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 kilometers wide.

Contents

An annular eclipse will cross Europe and Russia. Eight European capitals will observe annual eclipse: Monaco, San Marino, Ljubljana, Zagreb, Vienna, Bratislava, Budapest and Moscow. For Moscow it will be the first central eclipse since 1887. Other European large cities (non-capitals), in which the annular eclipse will be seen include Barcelona, Marseille, Genoa, Graz, Kraków, Lviv, Nizhny Novgorod, Kirov.

Eclipses in 2075

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 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]

122 February 7, 2073
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Partial
127 August 3, 2073
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Total
132 January 27, 2074
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Annular
137 July 24, 2074
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Annular
142 January 16, 2075
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Total
147 July 13, 2075
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Annular
152 January 6, 2076
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Total
157 July 1, 2076
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Partial

Saros 147

Solar saros 147, repeating every about 18 years and 11 days, contains 80 events. The series started with a partial solar eclipse on October 12, 1624. It has annular eclipses from May 31, 2003, to July 31, 2706. There are no total eclipses in this series. The series ends at member 80 as a partial eclipse on February 24, 3049. The longest annular eclipse will be on November 21, 2291, at 9 minutes and 41 seconds. [2]

Series members 17–27 occur between 1901 and 2100:
171819
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April 6, 1913
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April 18, 1931
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April 28, 1949
202122
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May 9, 1967
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May 19, 1985
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May 31, 2003
232425
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June 10, 2021
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June 21, 2039
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July 1, 2057
2627
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July 13, 2075
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July 23, 2093

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Metonic series

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.

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A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, May 1, 2079, with a magnitude of 1.0512. 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. The eclipse will be visible in Greenland, parts of eastern Canada and parts of the northeastern United States.

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. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.