Solar eclipse of June 12, 2029
A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 12, 2029, 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. The eclipse will be visible from Northern and Central Europe, northern Russia, Arctic, Greenland, and northern North America.
This will be the second of four partial solar eclipses in 2029, with the others occurring on January 14, July 11, and December 5.
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Related eclipses
Eclipses in 2029
- A partial solar eclipse on January 14.
- A partial solar eclipse on June 12.
- A total lunar eclipse on June 26.
- A partial solar eclipse on July 11.
- A partial solar eclipse on December 5.
- A total lunar eclipse on December 20.
Metonic
- Followed by: Solar eclipse of March 30, 2033
Tzolkinex
- Preceded by: Solar eclipse of April 30, 2022
- Followed by: Solar eclipse of July 23, 2036
Half-Saros
- Preceded by: Lunar eclipse of June 5, 2020
- Followed by: Lunar eclipse of June 17, 2038
Tritos
- Preceded by: Solar eclipse of July 13, 2018
- Followed by: Solar eclipse of May 11, 2040
Solar Saros 118
- Preceded by: Solar eclipse of June 1, 2011
- Followed by: Solar eclipse of June 23, 2047
Inex
- Preceded by: Solar eclipse of July 1, 2000
- Followed by: Solar eclipse of May 22, 2058
Triad
- Preceded by: Solar eclipse of August 12, 1942
- Followed by: Solar eclipse of April 13, 2116
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.[1]
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 | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118 | June 12, 2029![]() Partial | 1.29431 | 123 | December 5, 2029![]() Partial | −1.06090 | |
128 | June 1, 2030![]() Annular | 0.56265 | 133 | November 25, 2030![]() Total | −0.38669 | |
138 | May 21, 2031![]() Annular | −0.19699 | 143 | November 14, 2031![]() Hybrid | 0.30776 | |
148 | May 9, 2032![]() Annular | −0.93748 | 153 | November 3, 2032![]() 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.[2]
Series members 57–72 occur between 1801 and 2083: | ||
---|---|---|
57 | 58 | 59 |
![]() February 1, 1813 | ![]() February 12, 1831 | ![]() February 23, 1849 |
60 | 61 | 62 |
![]() March 6, 1867 | ![]() March 16, 1885 | ![]() March 29, 1903 |
63 | 64 | 65 |
![]() April 8, 1921 | ![]() April 19, 1939 | ![]() April 30, 1957 |
66 | 67 | 68 |
![]() May 11, 1975 | ![]() May 21, 1993 | ![]() June 1, 2011 |
69 | 70 | 71 |
![]() June 12, 2029 | ![]() June 23, 2047 | ![]() July 3, 2065 |
72 | ||
![]() July 15, 2083 |
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 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
118 | 120 | 122 | 124 | 126 |
![]() June 12, 2029 | ![]() March 30, 2033 | ![]() January 16, 2037 | ![]() November 4, 2040 | ![]() August 23, 2044 |
128 | 130 | 132 | 134 | 136 |
![]() June 11, 2048 | ![]() March 30, 2052 | ![]() January 16, 2056 | ![]() November 5, 2059 | ![]() August 24, 2063 |
138 | 140 | 142 | 144 | 146 |
![]() June 11, 2067 | ![]() March 31, 2071 | ![]() January 16, 2075 | ![]() November 4, 2078 | ![]() August 24, 2082 |
148 | 150 | 152 | 154 | 156 |
![]() June 11, 2086 | ![]() March 31, 2090 | ![]() January 16, 2094 | ![]() November 4, 2097 | ![]() August 24, 2101 |
158 | 160 | 162 | 164 | |
![]() June 12, 2105 | ![]() 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 | ||||
---|---|---|---|---|
![]() July 13, 2018 (Saros 117) | ![]() June 12, 2029 (Saros 118) | ![]() May 11, 2040 (Saros 119) | ![]() April 11, 2051 (Saros 120) | ![]() March 11, 2062 (Saros 121) |
![]() February 7, 2073 (Saros 122) | ![]() January 7, 2084 (Saros 123) | ![]() December 7, 2094 (Saros 124) | ![]() November 6, 2105 (Saros 125) | ![]() October 6, 2116 (Saros 126) |
![]() September 6, 2127 (Saros 127) | ![]() August 5, 2138 (Saros 128) | ![]() July 5, 2149 (Saros 129) | ![]() June 4, 2160 (Saros 130) | ![]() May 5, 2171 (Saros 131) |
![]() April 3, 2182 (Saros 132) | ![]() 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 | ||
---|---|---|
![]() October 31, 1826 (Saros 111) | ||
![]() August 31, 1913 (Saros 114) | ![]() August 12, 1942 (Saros 115) | ![]() July 22, 1971 (Saros 116) |
![]() July 1, 2000 (Saros 117) | ![]() June 12, 2029 (Saros 118) | ![]() May 22, 2058 (Saros 119) |
![]() May 2, 2087 (Saros 120) | ![]() April 13, 2116 (Saros 121) | ![]() March 23, 2145 (Saros 122) |
![]() March 3, 2174 (Saros 123) |
References
![](http://upload.wikimedia.org/wikipedia/en/thumb/4/4a/Commons-logo.svg/30px-Commons-logo.svg.png)
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements
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![21 August 2017 total solar eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/4/42/Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg/80px-Solar_eclipse%2C_Miles_Landing_8-21-17_%2836842678271%29.jpg)
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![23 October 2014 partial eclipse](http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png/80px-Partial_solar_eclipse_Oct_23_2014_Minneapolis_5-36pm_Ruen1.png)
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