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Solar eclipse of July 13, 2075

From Wikipedia, the free encyclopedia

Solar eclipse of July 13, 2075
Map
Type of eclipse
NatureAnnular
Gamma0.6583
Magnitude0.9467
Maximum eclipse
Duration285 sec (4 m 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 Saturday, 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 kilometers wide.

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.

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Transcription

Related eclipses

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]

122 February 7, 2073

Partial
127 August 3, 2073

Total
132 January 27, 2074

Annular
137 July 24, 2074

Annular
142 January 16, 2075

Total
147 July 13, 2075

Annular
152 January 6, 2076

Total
157 July 1, 2076

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:
17 18 19

April 6, 1913

April 18, 1931

April 28, 1949
20 21 22

May 9, 1967

May 19, 1985

May 31, 2003
23 24 25

June 10, 2021

June 21, 2039

July 1, 2057
26 27

July 13, 2075

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.

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.

External links

This page was last edited on 18 December 2023, at 09:48
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