Solar eclipse of July 13, 2075

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 at the Moon's ascending node of orbit on Saturday, July 13, 2075,[1] 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 kilometres wide. Occurring about 1.4 days after apogee (on July 11, 2075, at 20:20 UTC), the Moon's apparent diameter will be smaller.[2]

The path of annularity will be visible from parts of eastern Spain, southern France, Monaco, Italy, San Marino, Austria, Slovenia, Croatia, northwestern Bosnia and Herzegovina, Hungary, Slovakia, southwestern Czech Republic, extreme northwestern Romania, southeastern Poland, Ukraine, Belarus, and Russia. A partial solar eclipse will also be visible for parts of Europe, North Africa, Greenland, northern Canada, Alaska, and Asia.

The 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.

Eclipse details

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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]

July 13, 2075 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2075 July 13 at 03:17:41.4 UTC
First Umbral External Contact 2075 July 13 at 04:33:52.6 UTC
First Central Line 2075 July 13 at 04:36:49.8 UTC
First Umbral Internal Contact 2075 July 13 at 04:39:49.5 UTC
Equatorial Conjunction 2075 July 13 at 06:01:28.2 UTC
Greatest Duration 2075 July 13 at 06:03:23.0 UTC
Greatest Eclipse 2075 July 13 at 06:05:44.0 UTC
Ecliptic Conjunction 2075 July 13 at 06:13:31.4 UTC
Last Umbral Internal Contact 2075 July 13 at 07:31:42.1 UTC
Last Central Line 2075 July 13 at 07:34:41.0 UTC
Last Umbral External Contact 2075 July 13 at 07:37:37.2 UTC
Last Penumbral External Contact 2075 July 13 at 08:53:46.6 UTC
July 13, 2075 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.94668
Eclipse Obscuration 0.89620
Gamma 0.65829
Sun Right Ascension 07h30m57.3s
Sun Declination +21°47'03.5"
Sun Semi-Diameter 15'44.0"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 07h31m05.6s
Moon Declination +22°22'29.6"
Moon Semi-Diameter 14'43.7"
Moon Equatorial Horizontal Parallax 0°54'03.3"
ΔT 101.8 s

Eclipse season

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This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of June–July 2075
June 28
Descending node (full moon)
July 13
Ascending node (new moon)
Partial lunar eclipse
Lunar Saros 121
Annular solar eclipse
Solar Saros 147
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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.[4]

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.[5]

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

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

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)

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.

Series members between 1801 and 2200

January 10, 1815
(Saros 138)

December 21, 1843
(Saros 139)

November 30, 1872
(Saros 140)

November 11, 1901
(Saros 141)

October 21, 1930
(Saros 142)

October 2, 1959
(Saros 143)

September 11, 1988
(Saros 144)

August 21, 2017
(Saros 145)

August 2, 2046
(Saros 146)

July 13, 2075
(Saros 147)

June 22, 2104
(Saros 148)

June 3, 2133
(Saros 149)

May 14, 2162
(Saros 150)

April 23, 2191
(Saros 151)

References

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  1. ^ "July 13, 2075 Annular Solar Eclipse". timeanddate. Retrieved 21 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 21 August 2024.
  3. ^ "Annular Solar Eclipse of 2075 Jul 13". EclipseWise.com. Retrieved 21 August 2024.
  4. ^ 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.
  5. ^ "NASA - Catalog of Solar Eclipses of Saros 147". eclipse.gsfc.nasa.gov.
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