Solar eclipse of June 12, 2029

Last updated
Solar eclipse of June 12, 2029
SE2029Jun12P.png
Map
Type of eclipse
NaturePartial
Gamma 1.2943
Magnitude 0.4576
Maximum eclipse
Coordinates 66°48′N66°12′W / 66.8°N 66.2°W / 66.8; -66.2
Times (UTC)
Greatest eclipse4:06:13
References
Saros 118 (69 of 72)
Catalog # (SE5000) 9572

A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 12, 2029, [1] with a magnitude of 0.4576. 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 second of four partial solar eclipses in 2029, with the others occurring on January 14, July 11, and December 5.

A partial eclipse will be visible for parts of Northern and Central Europe, northern Russia, Greenland, Alaska, and northwestern Canada.

Images

SE2029Jun12P.gif
Animated path

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]

June 12, 2029 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2029 June 12 at 02:27:40.7 UTC
Ecliptic Conjunction2029 June 12 at 03:51:42.6 UTC
Equatorial Conjunction2029 June 12 at 04:01:14.1 UTC
Greatest Eclipse2029 June 12 at 04:06:13.0 UTC
Last Penumbral External Contact2029 June 12 at 05:44:42.8 UTC
June 12, 2029 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.45761
Eclipse Obscuration0.34111
Gamma1.29431
Sun Right Ascension05h22m58.2s
Sun Declination+23°09'45.7"
Sun Semi-Diameter15'45.0"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension05h23m08.9s
Moon Declination+24°21'37.7"
Moon Semi-Diameter15'10.6"
Moon Equatorial Horizontal Parallax0°55'42.0"
ΔT73.6 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 2029
June 12
Descending node (new moon)
June 26
Ascending node (full moon)
July 11
Descending node (new moon)
SE2029Jun12P.png Lunar eclipse chart close-29jun26.png SE2029Jul11P.png
Partial solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130
Partial solar eclipse
Solar Saros 156

Eclipses in 2029

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 118

Inex

Triad

Solar eclipses of 2029–2032

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 January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 June 12, 2029
SE2029Jun12P.png
Partial
1.29431123 December 5, 2029
SE2029Dec05P.png
Partial
−1.06090
128 June 1, 2030
SE2030Jun01A.png
Annular
0.56265133 November 25, 2030
SE2030Nov25T.png
Total
−0.38669
138 May 21, 2031
SE2031May21A.png
Annular
−0.19699143 November 14, 2031
SE2031Nov14H.png
Hybrid
0.30776
148 May 9, 2032
SE2032May09A.png
Annular
−0.93748153 November 3, 2032
SE2032Nov03P.png
Partial
1.06431

Saros 118

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

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 2018 and 2200
SE2018Jul13P.png
July 13, 2018
(Saros 117)
SE2029Jun12P.png
June 12, 2029
(Saros 118)
SE2040May11P.png
May 11, 2040
(Saros 119)
SE2051Apr11P.png
April 11, 2051
(Saros 120)
SE2062Mar11P.png
March 11, 2062
(Saros 121)
SE2073Feb07P.png
February 7, 2073
(Saros 122)
SE2084Jan07P.png
January 7, 2084
(Saros 123)
SE2094Dec07P.png
December 7, 2094
(Saros 124)
Saros125 59van73 SE2105Nov06P.jpg
November 6, 2105
(Saros 125)
Saros126 53van72 SE2116Oct06P.jpg
October 6, 2116
(Saros 126)
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
(Saros 127)
Saros128 65van73 SE2138Aug05P.jpg
August 5, 2138
(Saros 128)
Saros129 59van80 SE2149Jul05T.jpg
July 5, 2149
(Saros 129)
SE2160Jun04T.png
June 4, 2160
(Saros 130)
SE2171May05A.png
May 5, 2171
(Saros 131)
SE2182Apr03H.png
April 3, 2182
(Saros 132)
SE2193Mar03T.png
March 3, 2193
(Saros 133)

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
SE1826Oct31P.gif
October 31, 1826
(Saros 111)
SE1913Aug31P.png
August 31, 1913
(Saros 114)
SE1942Aug12P.png
August 12, 1942
(Saros 115)
SE1971Jul22P.png
July 22, 1971
(Saros 116)
SE2000Jul01P.png
July 1, 2000
(Saros 117)
SE2029Jun12P.png
June 12, 2029
(Saros 118)
SE2058May22P.png
May 22, 2058
(Saros 119)
SE2087May02P.png
May 2, 2087
(Saros 120)
Saros121 66van71 SE2116Apr13P.jpg
April 13, 2116
(Saros 121)
Saros122 65van70 SE2145Mar23P.jpg
March 23, 2145
(Saros 122)
Saros123 62van70 SE2174Mar03P.jpg
March 3, 2174
(Saros 123)

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References

  1. "June 12, 2029 Partial Solar Eclipse". timeanddate. Retrieved 13 August 2024.
  2. "Partial Solar Eclipse of 2029 Jun 12". EclipseWise.com. Retrieved 13 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 118". eclipse.gsfc.nasa.gov.