Solar eclipse of July 13, 2075

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.

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 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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Eclipses in 2075

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 147

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Inex

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Triad

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Solar eclipses of 2073–2076

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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

Saros 147

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This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity will be produced by member 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]

Series members 11–32 occur between 1801 and 2200:
11 12 13
 
January 30, 1805
 
February 11, 1823
 
February 21, 1841
14 15 16
 
March 4, 1859
 
March 15, 1877
 
March 26, 1895
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 28
 
July 13, 2075
 
July 23, 2093
 
August 4, 2111
29 30 31
 
August 15, 2129
 
August 26, 2147
 
September 5, 2165
32
 
September 16, 2183

Inex series

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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.

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
 
August 28, 1802
(Saros 122)
 
July 27, 1813
(Saros 123)
 
June 26, 1824
(Saros 124)
 
May 27, 1835
(Saros 125)
 
April 25, 1846
(Saros 126)
 
March 25, 1857
(Saros 127)
 
February 23, 1868
(Saros 128)
 
January 22, 1879
(Saros 129)
 
December 22, 1889
(Saros 130)
 
November 22, 1900
(Saros 131)
 
October 22, 1911
(Saros 132)
 
September 21, 1922
(Saros 133)
 
August 21, 1933
(Saros 134)
 
July 20, 1944
(Saros 135)
 
June 20, 1955
(Saros 136)
 
May 20, 1966
(Saros 137)
 
April 18, 1977
(Saros 138)
 
March 18, 1988
(Saros 139)
 
February 16, 1999
(Saros 140)
 
January 15, 2010
(Saros 141)
 
December 14, 2020
(Saros 142)
 
November 14, 2031
(Saros 143)
 
October 14, 2042
(Saros 144)
 
September 12, 2053
(Saros 145)
 
August 12, 2064
(Saros 146)
 
July 13, 2075
(Saros 147)
 
June 11, 2086
(Saros 148)
 
May 11, 2097
(Saros 149)
 
April 11, 2108
(Saros 150)
 
March 11, 2119
(Saros 151)
 
February 8, 2130
(Saros 152)
 
January 8, 2141
(Saros 153)
 
December 8, 2151
(Saros 154)
 
November 7, 2162
(Saros 155)
 
October 7, 2173
(Saros 156)
 
September 4, 2184
(Saros 157)
 
August 5, 2195
(Saros 158)

Metonic series

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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.

21 eclipse events between July 13, 2018 and July 12, 2094
July 12–13 April 30–May 1 February 16–17 December 5–6 September 22–23
117 119 121 123 125
 
July 13, 2018
 
April 30, 2022
 
February 17, 2026
 
December 5, 2029
 
September 23, 2033
127 129 131 133 135
 
July 13, 2037
 
April 30, 2041
 
February 16, 2045
 
December 5, 2048
 
September 22, 2052
137 139 141 143 145
 
July 12, 2056
 
April 30, 2060
 
February 17, 2064
 
December 6, 2067
 
September 23, 2071
147 149 151 153 155
 
July 13, 2075
 
May 1, 2079
 
February 16, 2083
 
December 6, 2086
 
September 23, 2090
157
 
July 12, 2094

References

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  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. ^ "NASA - Catalog of Solar Eclipses of Saros 147". eclipse.gsfc.nasa.gov.
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