Solar eclipse of January 16, 2094

Last updated
Solar eclipse of January 16, 2094
SE2094Jan16T.png
Map
Type of eclipse
NatureTotal
Gamma −0.9333
Magnitude 1.0342
Maximum eclipse
Duration111 s (1 min 51 s)
Coordinates 84°48′S10°36′W / 84.8°S 10.6°W / -84.8; -10.6
Max. width of band329 km (204 mi)
Times (UTC)
Greatest eclipse18:59:03
References
Saros 152 (17 of 70)
Catalog # (SE5000) 9718

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, January 16, 2094, [1] with a magnitude of 1.0342. 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. Occurring about 10.5 hours before perigee (on January 17, 2094, at 5:40 UTC), the Moon's apparent diameter will be larger. [2]

Contents

This will be the first of four solar eclipses in 2094, with the others occurring on June 13, July 12, and December 7.

The path of totality will be visible from parts of Antarctica. A partial solar eclipse will also be visible for parts of New Zealand, Antarctica, and southern South America. This total eclipse is notable in that the path of totality passes over the South Pole.

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. [3]

January 16, 2094 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2094 January 16 at 16:53:04.7 UTC
First Umbral External Contact2094 January 16 at 18:20:43.2 UTC
First Central Line2094 January 16 at 18:22:49.9 UTC
First Umbral Internal Contact2094 January 16 at 18:25:03.5 UTC
Equatorial Conjunction2094 January 16 at 18:49:35.7 UTC
Greatest Eclipse2094 January 16 at 18:59:03.4 UTC
Greatest Duration2094 January 16 at 18:59:14.4 UTC
Ecliptic Conjunction2094 January 16 at 19:08:26.0 UTC
Last Umbral Internal Contact2094 January 16 at 19:33:09.4 UTC
Last Central Line2094 January 16 at 19:35:23.5 UTC
Last Umbral External Contact2094 January 16 at 19:37:30.8 UTC
Last Penumbral External Contact2094 January 16 at 21:05:05.3 UTC
January 16, 2094 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.03423
Eclipse Obscuration1.06962
Gamma−0.93334
Sun Right Ascension19h56m48.4s
Sun Declination-20°43'02.8"
Sun Semi-Diameter16'15.5"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension19h57m12.4s
Moon Declination-21°39'54.3"
Moon Semi-Diameter16'43.2"
Moon Equatorial Horizontal Parallax1°01'21.9"
ΔT117.8 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.

Eclipse season of January 2094
January 1
Ascending node (full moon)
 January 16
Descending node (new moon)
SE2094Jan16T.png
Partial lunar eclipse
Lunar Saros 126		 Total solar eclipse
Solar Saros 152

Eclipses in 2094

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 152

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. [4]

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 152

This eclipse is a part of Saros series 152, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 26, 1805. It contains total eclipses from November 2, 1967 through September 14, 2490; hybrid eclipses from September 26, 2508 through October 17, 2544; and annular eclipses from October 29, 2562 through June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 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 totality will be produced by member 30 at 5 minutes, 16 seconds on June 9, 2328, and the longest duration of annularity will be produced by member 53 at 5 minutes, 20 seconds on February 16, 2743. All eclipses in this series occur at the Moon’s descending node of orbit. [5]

Series members 1–22 occur between 1805 and 2200:
123
SE1805Jul26Pb.gif
July 26, 1805		 SE1823Aug06P.gif
August 6, 1823		 SE1841Aug16P.gif
August 16, 1841
456
SE1859Aug28P.gif
August 28, 1859		 SE1877Sep07P.gif
September 7, 1877		 SE1895Sep18P.gif
September 18, 1895
789
SE1913Sep30P.png
September 30, 1913 		SE1931Oct11P.png
October 11, 1931 		SE1949Oct21P.png
October 21, 1949
101112
SE1967Nov02T.png
November 2, 1967 		SE1985Nov12T.png
November 12, 1985 		SE2003Nov23T.png
November 23, 2003
131415
SE2021Dec04T.png
December 4, 2021 		SE2039Dec15T.png
December 15, 2039 		SE2057Dec26T.png
December 26, 2057
161718
SE2076Jan06T.png
January 6, 2076 		SE2094Jan16T.png
January 16, 2094 		Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112
192021
Saros152 19van70 SE2130Feb08T.jpg
February 8, 2130		 Saros152 20van70 SE2148Feb19T.jpg
February 19, 2148		 Saros152 21van70 SE2166Mar02T.jpg
March 2, 2166
22
Saros152 22van70 SE2184Mar12T.jpg
March 12, 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 descending node.

22 eclipse events between June 12, 2029 and November 4, 2116
June 11–12March 30–31January 16November 4–5August 23–24
118120122124126
SE2029Jun12P.png
June 12, 2029 		SE2033Mar30T.png
March 30, 2033 		SE2037Jan16P.png
January 16, 2037 		SE2040Nov04P.png
November 4, 2040 		SE2044Aug23T.png
August 23, 2044
128130132134136
SE2048Jun11A.png
June 11, 2048 		SE2052Mar30T.png
March 30, 2052 		SE2056Jan16A.png
January 16, 2056 		SE2059Nov05A.png
November 5, 2059 		SE2063Aug24T.png
August 24, 2063
138140142144146
SE2067Jun11A.png
June 11, 2067 		SE2071Mar31A.png
March 31, 2071 		SE2075Jan16T.png
January 16, 2075 		SE2078Nov04A.png
November 4, 2078 		SE2082Aug24T.png
August 24, 2082
148150152154156
SE2086Jun11T.png
June 11, 2086 		SE2090Mar31P.png
March 31, 2090 		SE2094Jan16T.png
January 16, 2094 		SE2097Nov04A.png
November 4, 2097 		Saros156 06van69 SE2101Aug24P.jpg
August 24, 2101
158160162164
Saros158 03van70 SE2105Jun12P.jpg
June 12, 2105		 Saros164 02van80 SE2116Nov04P.jpg
November 4, 2116

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.

Series members between 1801 and 2200
SE1810Apr04A.gif
April 4, 1810
(Saros 126)		 SE1821Mar04T.gif
March 4, 1821
(Saros 127)		 SE1832Feb01A.gif
February 1, 1832
(Saros 128)		 SE1842Dec31A.gif
December 31, 1842
(Saros 129)		 SE1853Nov30T.png
November 30, 1853
(Saros 130)
SE1864Oct30A.gif
October 30, 1864
(Saros 131)		 SE1875Sep29A.gif
September 29, 1875
(Saros 132)		 SE1886Aug29T.png
August 29, 1886
(Saros 133)		 SE1897Jul29A.gif
July 29, 1897
(Saros 134)		 SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)		 SE1930Apr28H.png
April 28, 1930
(Saros 137)		 SE1941Mar27A.png
March 27, 1941
(Saros 138)		 SE1952Feb25T.png
February 25, 1952
(Saros 139)		 SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1973Dec24A.png
December 24, 1973
(Saros 141)		 SE1984Nov22T.png
November 22, 1984
(Saros 142)		 SE1995Oct24T.png
October 24, 1995
(Saros 143)		 SE2006Sep22A.png
September 22, 2006
(Saros 144)		 SE2017Aug21T.png
August 21, 2017
(Saros 145)
SE2028Jul22T.png
July 22, 2028
(Saros 146)		 SE2039Jun21A.png
June 21, 2039
(Saros 147)		 SE2050May20H.png
May 20, 2050
(Saros 148)		 SE2061Apr20T.png
April 20, 2061
(Saros 149)		 SE2072Mar19P.png
March 19, 2072
(Saros 150)
SE2083Feb16P.png
February 16, 2083
(Saros 151)		 SE2094Jan16T.png
January 16, 2094
(Saros 152)		 Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)		 SE2115Nov16A.png
November 16, 2115
(Saros 154)		 SE2126Oct16T.png
October 16, 2126
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)		 Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)		 Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
(Saros 158)		 Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)		 Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

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
SE1804Aug05T.gif
August 5, 1804
(Saros 142)		 SE1833Jul17T.gif
July 17, 1833
(Saros 143)		 SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1891Jun06A.gif
June 6, 1891
(Saros 145)		 SE1920May18P.png
May 18, 1920
(Saros 146)		 SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1978Apr07P.png
April 7, 1978
(Saros 148)		 SE2007Mar19P.png
March 19, 2007
(Saros 149)		 SE2036Feb27P.png
February 27, 2036
(Saros 150)
SE2065Feb05P.png
February 5, 2065
(Saros 151)		 SE2094Jan16T.png
January 16, 2094
(Saros 152)		 Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
(Saros 153)
Saros154 14van71 SE2151Dec08A.jpg
December 8, 2151
(Saros 154)		 Saros155 15van71 SE2180Nov17T.jpg
November 17, 2180
(Saros 155)

Notes

  1. ↑ "January 16, 2094 Total Solar Eclipse". timeanddate. Retrieved 24 August 2024.
  2. ↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 24 August 2024.
  3. ↑ "Total Solar Eclipse of 2094 Jan 16". EclipseWise.com. Retrieved 24 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 152". eclipse.gsfc.nasa.gov.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of September 11, 2007</span> Partial solar eclipse September 11, 2007

A partial solar eclipse occurred at the Moon’s descending node of orbit on Tuesday, September 11, 2007, with a magnitude of 0.7507. 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.

<span class="mw-page-title-main">Solar eclipse of May 22, 2096</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit between Monday, May 21 and Tuesday, May 22, 2096, with a magnitude of 1.0737. 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. Occurring about 13 hours after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of December 27, 2084</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, December 27, 2084, with a magnitude of 1.0396. 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. Occurring only about 21 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of September 23, 2090</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, September 23, 2090, with a magnitude of 1.0562. 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. Occurring only about 4 hours after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of September 25, 2098</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit between Wednesday, September 24 and Thursday, September 25, 2098, with a magnitude of 0.7871. 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.

<span class="mw-page-title-main">Solar eclipse of August 15, 2091</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit between Tuesday, August 14 and Wednesday, August 15, 2091, with a magnitude of 1.0216. 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. Occurring about 3.3 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of January 27, 2093</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, January 27, 2093, with a magnitude of 1.034. 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. Occurring about 1.3 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of November 27, 2095</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit between Saturday, November 26 and Sunday, November 27, 2095, with a magnitude of 0.933. 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 3.8 days after apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of May 2, 2087</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, May 2, 2087, with a magnitude of 0.8011. 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.

<span class="mw-page-title-main">Solar eclipse of February 5, 2065</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Thursday, February 5, 2065, with a magnitude of 0.9123. 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.

<span class="mw-page-title-main">Solar eclipse of July 3, 2065</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, July 3, 2065, with a magnitude of 0.1638. 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.

<span class="mw-page-title-main">Solar eclipse of January 6, 2076</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Monday, January 6, 2076, with a magnitude of 1.0342. 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. Occurring about 8.5 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of November 4, 2097</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, November 3 and Monday, November 4, 2097, with a magnitude of 0.9494. 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 5.4 days before apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of May 11, 2097</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, May 11, 2097, with a magnitude of 1.0538. 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. Occurring about 1.3 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of June 2, 2095</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, June 2, 2095, with a magnitude of 1.0332. 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. Occurring about 3 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of February 18, 2091</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, February 18, 2091, with a magnitude of 0.6558. 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.

<span class="mw-page-title-main">Solar eclipse of April 1, 2098</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, April 1, 2098, with a magnitude of 0.7984. 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.

<span class="mw-page-title-main">Solar eclipse of December 7, 2094</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, December 7, 2094, with a magnitude of 0.7046. 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.

<span class="mw-page-title-main">Solar eclipse of July 12, 2094</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, July 12, 2094, 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.

<span class="mw-page-title-main">Solar eclipse of October 26, 2087</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, October 26, 2087, with a magnitude of 0.4696. 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.

References

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.