Solar eclipse of July 11, 2029
Solar eclipse of July 11, 2029 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | −1.4191 |
Magnitude | 0.2303 |
Maximum eclipse | |
Coordinates | 64°18′S 85°36′W / 64.3°S 85.6°W |
Times (UTC) | |
Greatest eclipse | 15:37:19 |
References | |
Saros | 156 (2 of 69) |
Catalog # (SE5000) | 9573 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Wednesday, July 11, 2029,[1] with a magnitude of 0.2303. 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.
This will be the third of four partial solar eclipses in 2029, with the others occurring on January 14, June 12, and December 5.
A partial eclipse will be visible for parts of southern Chile and Argentina.
Images
[edit]Eclipse details
[edit]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]
Event | Time (UTC) |
---|---|
First Penumbral External Contact | 2029 July 11 at 14:28:56.7 UTC |
Greatest Eclipse | 2029 July 11 at 15:37:18.9 UTC |
Ecliptic Conjunction | 2029 July 11 at 15:52:13.6 UTC |
Equatorial Conjunction | 2029 July 11 at 16:15:41.3 UTC |
Last Penumbral External Contact | 2029 July 11 at 16:45:20.1 UTC |
Parameter | Value |
---|---|
Eclipse Magnitude | 0.23033 |
Eclipse Obscuration | 0.12768 |
Gamma | −1.41908 |
Sun Right Ascension | 07h24m55.6s |
Sun Declination | +22°00'04.3" |
Sun Semi-Diameter | 15'43.9" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 07h23m33.7s |
Moon Declination | +20°41'22.0" |
Moon Semi-Diameter | 15'35.3" |
Moon Equatorial Horizontal Parallax | 0°57'12.6" |
ΔT | 73.6 s |
Eclipse season
[edit]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.
June 12 Descending node (new moon) |
June 26 Ascending node (full moon) |
July 11 Descending node (new moon) |
---|---|---|
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Partial solar eclipse Solar Saros 118 |
Total lunar eclipse Lunar Saros 130 |
Partial solar eclipse Solar Saros 156 |
Related eclipses
[edit]Eclipses in 2029
[edit]- 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
[edit]- Preceded by: Solar eclipse of September 21, 2025
Tzolkinex
[edit]- Followed by: Solar eclipse of August 21, 2036
Half-Saros
[edit]- Preceded by: Lunar eclipse of July 5, 2020
- Followed by: Lunar eclipse of July 16, 2038
Tritos
[edit]- Preceded by: Solar eclipse of August 11, 2018
Solar Saros 156
[edit]- Preceded by: Solar eclipse of July 1, 2011
- Followed by: Solar eclipse of July 22, 2047
Inex
[edit]- Preceded by: Solar eclipse of July 31, 2000
- Followed by: Solar eclipse of June 21, 2058
Triad
[edit]- Preceded by: Solar eclipse of September 10, 1942
Solar eclipses of 2026–2029
[edit]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 12, 2029 and December 5, 2029 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2026 to 2029 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | February 17, 2026![]() Annular |
−0.97427 | 126 | August 12, 2026![]() Total |
0.89774 | |
131 | February 6, 2027![]() Annular |
−0.29515 | 136 | August 2, 2027![]() Total |
0.14209 | |
141 | January 26, 2028![]() Annular |
0.39014 | 146 | July 22, 2008![]() Total |
−0.60557 | |
151 | January 14, 2029![]() Partial |
1.05532 | 156 | July 11, 2029![]() Partial |
−1.41908 |
Saros 156
[edit]This eclipse is a part of Saros series 156, repeating every 18 years, 11 days, and containing 69 events. The series started with a partial solar eclipse on July 1, 2011. It contains annular eclipses from September 26, 2155 through April 7, 3075. There are no hybrid or total eclipses in this set. The series ends at member 69 as a partial eclipse on July 14, 3237. 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 29 at 8 minutes, 28 seconds on May 3, 2516. All eclipses in this series occur at the Moon’s descending node of orbit.[4]
Series members 1–11 occur between 2011 and 2200: | ||
---|---|---|
1 | 2 | 3 |
![]() July 1, 2011 |
![]() July 11, 2029 |
![]() July 22, 2047 |
4 | 5 | 6 |
![]() August 2, 2065 |
![]() August 13, 2083 |
![]() August 24, 2101 |
7 | 8 | 9 |
![]() September 5, 2119 |
![]() September 15, 2137 |
![]() September 26, 2155 |
10 | 11 | |
![]() October 7, 2173 |
![]() October 18, 2191 |
Metonic series
[edit]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.
21 eclipse events between July 11, 1953 and July 11, 2029 | ||||
---|---|---|---|---|
July 10–11 | April 29–30 | February 15–16 | December 4 | September 21–23 |
116 | 118 | 120 | 122 | 124 |
![]() July 11, 1953 |
![]() April 30, 1957 |
![]() February 15, 1961 |
![]() December 4, 1964 |
![]() September 22, 1968 |
126 | 128 | 130 | 132 | 134 |
![]() July 10, 1972 |
![]() April 29, 1976 |
![]() February 16, 1980 |
![]() December 4, 1983 |
![]() September 23, 1987 |
136 | 138 | 140 | 142 | 144 |
![]() July 11, 1991 |
![]() April 29, 1995 |
![]() February 16, 1999 |
![]() December 4, 2002 |
![]() September 22, 2006 |
146 | 148 | 150 | 152 | 154 |
![]() July 11, 2010 |
![]() April 29, 2014 |
![]() February 15, 2018 |
![]() December 4, 2021 |
![]() September 21, 2025 |
156 | ||||
![]() July 11, 2029 |
Tritos series
[edit]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 eclipse on November 4, 2116 (part of Saros 164) is also a part of this series but is not included in the table below.
Series members between 1801 and 2029 | ||||
---|---|---|---|---|
![]() March 24, 1811 (Saros 136) |
![]() February 21, 1822 (Saros 137) |
![]() January 20, 1833 (Saros 138) |
![]() December 21, 1843 (Saros 139) |
![]() November 20, 1854 (Saros 140) |
![]() October 19, 1865 (Saros 141) |
![]() September 17, 1876 (Saros 142) |
![]() August 19, 1887 (Saros 143) |
![]() July 18, 1898 (Saros 144) |
![]() June 17, 1909 (Saros 145) |
![]() May 18, 1920 (Saros 146) |
![]() April 18, 1931 (Saros 147) |
![]() March 16, 1942 (Saros 148) |
![]() February 14, 1953 (Saros 149) |
![]() January 14, 1964 (Saros 150) |
![]() December 13, 1974 (Saros 151) |
![]() November 12, 1985 (Saros 152) |
![]() October 12, 1996 (Saros 153) |
![]() September 11, 2007 (Saros 154) |
![]() August 11, 2018 (Saros 155) |
![]() July 11, 2029 (Saros 156) |
Inex series
[edit]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 | ||
---|---|---|
![]() November 29, 1826 (Saros 149) |
![]() November 9, 1855 (Saros 150) |
![]() October 19, 1884 (Saros 151) |
![]() September 30, 1913 (Saros 152) |
![]() September 10, 1942 (Saros 153) |
![]() August 20, 1971 (Saros 154) |
![]() July 31, 2000 (Saros 155) |
![]() July 11, 2029 (Saros 156) |
![]() June 21, 2058 (Saros 157) |
![]() June 1, 2087 (Saros 158) |
||
![]() April 1, 2174 (Saros 161) |
References
[edit]- ^ "July 11, 2029 Partial Solar Eclipse". timeanddate. Retrieved 13 August 2024.
- ^ "Partial Solar Eclipse of 2029 Jul 11". EclipseWise.com. Retrieved 13 August 2024.
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 156". eclipse.gsfc.nasa.gov.
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External links
[edit]- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC