Solar eclipse of July 12, 2094

Last updated
Solar eclipse of July 12, 2094
SE2094Jul12P.png
Map
Type of eclipse
NaturePartial
Gamma 1.3150
Magnitude 0.4224
Maximum eclipse
Coordinates 68°00′N52°48′E / 68°N 52.8°E / 68; 52.8
Times (UTC)
Greatest eclipse13:24:35
References
Saros 157 (3 of 70)
Catalog # (SE5000) 9720

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, July 12, 2094, [1] with a magnitude of 0.4224. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

This will be the third of four solar eclipses in 2094, with the others occurring on January 16, June 13, and December 7.

The partial solar eclipse will be visible for parts of northern North America, Scandinavia, and Russia.

Eclipse details

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. [2]

July 12, 2094 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2094 July 12 at 11:46:47.0 UTC
Equatorial Conjunction2094 July 12 at 13:16:11.9 UTC
Greatest Eclipse2094 July 12 at 13:24:34.9 UTC
Ecliptic Conjunction2094 July 12 at 13:39:38.8 UTC
Last Penumbral External Contact2094 July 12 at 15:02:30.3 UTC
July 12, 2094 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.42247
Eclipse Obscuration0.30296
Gamma1.31495
Sun Right Ascension07h29m49.1s
Sun Declination+21°49'23.2"
Sun Semi-Diameter15'43.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension07h30m06.1s
Moon Declination+23°01'02.4"
Moon Semi-Diameter14'54.5"
Moon Equatorial Horizontal Parallax0°54'43.0"
ΔT118.3 s

Eclipse season

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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of June–July 2094
June 13
Ascending node (new moon)
June 28
Descending node (full moon)
July 12
Ascending node (new moon)
SE2094Jun13P.png Lunar eclipse chart close-2094Jun28.png SE2094Jul12P.png
Partial solar eclipse
Solar Saros 119
Total lunar eclipse
Lunar Saros 131
Partial solar eclipse
Solar Saros 157

Eclipses in 2094

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 157

Inex

Triad

Solar eclipses of 2091–2094

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. [3]

The partial solar eclipses on June 13, 2094 and December 7, 2094 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2091 to 2094
Descending node Ascending node
SarosMapGammaSarosMapGamma
122 February 18, 2091
SE2091Feb18P.png
Partial
1.1779127 August 15, 2091
SE2091Aug15T.png
Total
−0.949
132 February 7, 2092
SE2092Feb07A.png
Annular
0.4322137 August 3, 2092
SE2092Aug03A.png
Annular
−0.2044
142 January 27, 2093
SE2093Jan27T.png
Total
−0.2737147 July 23, 2093
SE2093Jul23A.png
Annular
0.5717
152 January 16, 2094
SE2094Jan16T.png
Total
−0.9333157 July 12, 2094
SE2094Jul12P.png
Partial
1.3150

Saros 157

This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. 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 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–8 occur between 2058 and 2200:
123
SE2058Jun21P.png
June 21, 2058
SE2076Jul01P.png
July 1, 2076
SE2094Jul12P.png
July 12, 2094
456
Saros157 04van70 SE2112Jul23P.jpg
July 23, 2112
Saros157 05van70 SE2130Aug04P.jpg
August 4, 2130
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
78
Saros157 07van70 SE2166Aug25A.jpg
August 25, 2166
Saros157 08van70 SE2184Sep04A.jpg
September 4, 2184

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.

21 eclipse events between July 13, 2018 and July 12, 2094
July 12–13April 30–May 1February 16–17December 5–6September 22–23
117119121123125
SE2018Jul13P.png
July 13, 2018
SE2022Apr30P.png
April 30, 2022
SE2026Feb17A.png
February 17, 2026
SE2029Dec05P.png
December 5, 2029
SE2033Sep23P.png
September 23, 2033
127129131133135
SE2037Jul13T.png
July 13, 2037
SE2041Apr30T.png
April 30, 2041
SE2045Feb16A.png
February 16, 2045
SE2048Dec05T.png
December 5, 2048
SE2052Sep22A.png
September 22, 2052
137139141143145
SE2056Jul12A.png
July 12, 2056
SE2060Apr30T.png
April 30, 2060
SE2064Feb17A.png
February 17, 2064
SE2067Dec06H.png
December 6, 2067
SE2071Sep23T.png
September 23, 2071
147149151153155
SE2075Jul13A.png
July 13, 2075
SE2079May01T.png
May 1, 2079
SE2083Feb16P.png
February 16, 2083
SE2086Dec06P.png
December 6, 2086
SE2090Sep23T.png
September 23, 2090
157
SE2094Jul12P.png
July 12, 2094

Tritos series

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.

The partial solar eclipses on December 7, 2170 (part of Saros 164) and November 7, 2181 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2105
SE1810Sep28A.gif
September 28, 1810
(Saros 131)
SE1821Aug27A.gif
August 27, 1821
(Saros 132)
SE1832Jul27T.gif
July 27, 1832
(Saros 133)
SE1843Jun27H.gif
June 27, 1843
(Saros 134)
SE1854May26A.png
May 26, 1854
(Saros 135)
SE1865Apr25T.png
April 25, 1865
(Saros 136)
SE1876Mar25A.gif
March 25, 1876
(Saros 137)
SE1887Feb22A.png
February 22, 1887
(Saros 138)
SE1898Jan22T.png
January 22, 1898
(Saros 139)
SE1908Dec23H.png
December 23, 1908
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1930Oct21T.png
October 21, 1930
(Saros 142)
SE1941Sep21T.png
September 21, 1941
(Saros 143)
SE1952Aug20A.png
August 20, 1952
(Saros 144)
SE1963Jul20T.png
July 20, 1963
(Saros 145)
SE1974Jun20T.png
June 20, 1974
(Saros 146)
SE1985May19P.png
May 19, 1985
(Saros 147)
SE1996Apr17P.png
April 17, 1996
(Saros 148)
SE2007Mar19P.png
March 19, 2007
(Saros 149)
SE2018Feb15P.png
February 15, 2018
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2039Dec15T.png
December 15, 2039
(Saros 152)
SE2050Nov14P.png
November 14, 2050
(Saros 153)
SE2061Oct13A.png
October 13, 2061
(Saros 154)
SE2072Sep12T.png
September 12, 2072
(Saros 155)
SE2083Aug13P.png
August 13, 2083
(Saros 156)
SE2094Jul12P.png
July 12, 2094
(Saros 157)
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105
(Saros 158)

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.

Series members between 1801 and 2200
SE1805Jan30P.gif
January 30, 1805
(Saros 147)
SE1834Jan09P.gif
January 9, 1834
(Saros 148)
SE1862Dec21P.gif
December 21, 1862
(Saros 149)
SE1891Dec01P.gif
December 1, 1891
(Saros 150)
SE1920Nov10P.png
November 10, 1920
(Saros 151)
SE1949Oct21P.png
October 21, 1949
(Saros 152)
SE1978Oct02P.png
October 2, 1978
(Saros 153)
SE2007Sep11P.png
September 11, 2007
(Saros 154)
SE2036Aug21P.png
August 21, 2036
(Saros 155)
SE2065Aug02P.png
August 2, 2065
(Saros 156)
SE2094Jul12P.png
July 12, 2094
(Saros 157)
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
(Saros 158)
Saros159 02van70 SE2152Jun03P.jpg
June 3, 2152
(Saros 159)
Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)

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References

  1. "July 12, 2094 Partial Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. "Partial Solar Eclipse of 2094 Jul 12". EclipseWise.com. Retrieved 24 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 157". eclipse.gsfc.nasa.gov.