Solar eclipse of November 14, 2050
Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 14, 2050,[1] with a magnitude of 0.8874. 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 the Northeastern United States, eastern Canada, Greenland, Europe, West Africa, and North Africa.
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 | 2050 November 14 at 11:17:27.7 UTC |
| Equatorial Conjunction | 2050 November 14 at 13:11:24.1 UTC |
| Greatest Eclipse | 2050 November 14 at 13:30:52.8 UTC |
| Ecliptic Conjunction | 2050 November 14 at 13:42:38.5 UTC |
| Last Penumbral External Contact | 2050 November 14 at 15:44:21.5 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.88738 |
| Eclipse Obscuration | 0.83218 |
| Gamma | 1.04468 |
| Sun Right Ascension | 15h19m50.5s |
| Sun Declination | -18°21'19.2" |
| Sun Semi-Diameter | 16'09.8" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 15h20m29.5s |
| Moon Declination | -17°24'01.9" |
| Moon Semi-Diameter | 15'10.6" |
| Moon Equatorial Horizontal Parallax | 0°55'41.9" |
| ΔT | 84.6 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.
| October 30 Descending node (full moon) |
November 14 Ascending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-2050Oct30.png | File:SE2050Nov14P.png |
| Total lunar eclipse Lunar Saros 127 |
Partial solar eclipse Solar Saros 153 |
Related eclipses
Eclipses in 2050
- A total lunar eclipse on May 6.
- A hybrid solar eclipse on May 20.
- A total lunar eclipse on October 30.
- A partial solar eclipse on November 14.
Metonic
- Preceded by: Solar eclipse of January 26, 2047
- Followed by: Solar eclipse of September 2, 2054
Tzolkinex
- Preceded by: Solar eclipse of October 3, 2043
- Followed by: Solar eclipse of December 26, 2057
Half-Saros
- Preceded by: Lunar eclipse of November 8, 2041
- Followed by: Lunar eclipse of November 19, 2059
Tritos
- Preceded by: Solar eclipse of December 15, 2039
- Followed by: Solar eclipse of October 13, 2061
Solar Saros 153
- Preceded by: Solar eclipse of November 3, 2032
- Followed by: Solar eclipse of November 24, 2068
Inex
- Preceded by: Solar eclipse of December 4, 2021
- Followed by: Solar eclipse of October 24, 2079
Triad
- Preceded by: Solar eclipse of January 14, 1964
- Followed by: Solar eclipse of September 15, 2137
Solar eclipses of 2047–2050
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 26, 2047 and July 22, 2047 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2047 to 2050 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | June 23, 2047 File:SE2047Jun23P.png Partial |
1.3766 | 123 | December 16, 2047 File:SE2047Dec16P.png Partial |
−1.0661 | |
| 128 | June 11, 2048 File:SE2048Jun11A.png Annular |
0.6468 | 133 | December 5, 2048 File:SE2048Dec05T.png Total |
−0.3973 | |
| 138 | May 31, 2049 File:SE2049May31A.png Annular |
−0.1187 | 143 | November 25, 2049 File:SE2049Nov25H.png Hybrid |
0.2943 | |
| 148 | May 20, 2050 File:SE2050May20H.png Hybrid |
−0.8688 | 153 | November 14, 2050 File:SE2050Nov14P.png Partial |
1.0447 | |
Saros 153
Template:Solar Saros series 153
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 ascending node.
| 21 eclipse events between June 21, 1982 and June 21, 2058 | ||||
|---|---|---|---|---|
| June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
| 117 | 119 | 121 | 123 | 125 |
| File:SE1982Jun21P.png June 21, 1982 |
File:SE1986Apr09P.png April 9, 1986 |
File:SE1990Jan26A.png January 26, 1990 |
File:SE1993Nov13P.png November 13, 1993 |
File:SE1997Sep02P.png September 2, 1997 |
| 127 | 129 | 131 | 133 | 135 |
| File:SE2001Jun21T.png June 21, 2001 |
File:SE2005Apr08H.png April 8, 2005 |
File:SE2009Jan26A.png January 26, 2009 |
File:SE2012Nov13T.png November 13, 2012 |
File:SE2016Sep01A.png September 1, 2016 |
| 137 | 139 | 141 | 143 | 145 |
| File:SE2020Jun21A.png June 21, 2020 |
File:SE2024Apr08T.png April 8, 2024 |
File:SE2028Jan26A.png January 26, 2028 |
File:SE2031Nov14H.png November 14, 2031 |
File:SE2035Sep02T.png September 2, 2035 |
| 147 | 149 | 151 | 153 | 155 |
| File:SE2039Jun21A.png June 21, 2039 |
File:SE2043Apr09T.png April 9, 2043 |
File:SE2047Jan26P.png January 26, 2047 |
File:SE2050Nov14P.png November 14, 2050 |
File:SE2054Sep02P.png September 2, 2054 |
| 157 | ||||
| File:SE2058Jun21P.png June 21, 2058 | ||||
Tritos series
Template:Solar Tritos series 2007 March 19
Inex series
Template:Solar Inex series 2021 December 4
References
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External links
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