Solar eclipse of September 3, 2062
Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, September 3, 2062,[1] with a magnitude of 0.9749. 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 partial solar eclipse will be visible for parts of Greenland, Northern Europe, and Asia.
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]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2062 September 3 at 06:53:47.7 UTC |
| Equatorial Conjunction | 2062 September 3 at 07:57:56.6 UTC |
| Ecliptic Conjunction | 2062 September 3 at 08:44:07.4 UTC |
| Greatest Eclipse | 2062 September 3 at 08:54:27.4 UTC |
| Last Penumbral External Contact | 2062 September 3 at 10:55:33.6 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.97489 |
| Eclipse Obscuration | 0.97526 |
| Gamma | 1.01915 |
| Sun Right Ascension | 10h50m30.3s |
| Sun Declination | +07°22'28.5" |
| Sun Semi-Diameter | 15'51.2" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 10h52m25.5s |
| Moon Declination | +08°16'29.0" |
| Moon Semi-Diameter | 16'22.2" |
| Moon Equatorial Horizontal Parallax | 1°00'04.6" |
| ΔT | 92.2 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| September 3 Descending node (new moon) |
September 18 Ascending node (full moon) |
|---|---|
| File:SE2062Sep03P.png | |
| Partial solar eclipse Solar Saros 126 |
Total lunar eclipse Lunar Saros 138 |
Related eclipses
Eclipses in 2062
- A partial solar eclipse on March 11.
- A total lunar eclipse on March 25.
- A partial solar eclipse on September 3.
- A total lunar eclipse on September 18.
Metonic
- Preceded by: Solar eclipse of November 16, 2058
- Followed by: Solar eclipse of June 22, 2066
Tzolkinex
- Preceded by: Solar eclipse of July 24, 2055
- Followed by: Solar eclipse of October 15, 2069
Half-Saros
- Preceded by: Lunar eclipse of August 29, 2053
- Followed by: Lunar eclipse of September 9, 2071
Tritos
- Preceded by: Solar eclipse of October 4, 2051
- Followed by: Solar eclipse of August 3, 2073
Solar Saros 126
- Preceded by: Solar eclipse of August 23, 2044
- Followed by: Solar eclipse of September 13, 2080
Inex
- Preceded by: Solar eclipse of September 23, 2033
- Followed by: Solar eclipse of August 15, 2091
Triad
- Preceded by: Solar eclipse of November 3, 1975
- Followed by: Solar eclipse of July 5, 2149
Solar eclipses of 2062–2065
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 July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2062 to 2065 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | March 11, 2062 File:SE2062Mar11P.png Partial |
−1.0238 | 126 | September 3, 2062 File:SE2062Sep03P.png Partial |
1.0191 | |
| 131 | February 28, 2063 File:SE2063Feb28A.png Annular |
−0.336 | 136 | August 24, 2063 File:SE2063Aug24T.png Total |
0.2771 | |
| 141 | February 17, 2064 File:SE2064Feb17A.png Annular |
0.3597 | 146 | August 12, 2064 File:SE2064Aug12T.png Total |
−0.4652 | |
| 151 | February 5, 2065 File:SE2065Feb05P.png Partial |
1.0336 | 156 | August 2, 2065 File:SE2065Aug02P.png Partial |
−1.2759 | |
Saros 126
This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. 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 was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.[4]
Metonic series
Template:Solar Metonic series 2047–2134
Tritos series
Template:Solar Tritos series 2008 February 7
Inex series
Template:Solar Inex series 2004 October 14
References
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External links
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