Solar eclipse of January 16, 2075
A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.5 days after perigee, the Moon's apparent diameter will be larger.
The path of totality will be visible from parts of Chile, Argentina, Paraguay, and Brazil. A partial solar eclipse will also be visible for parts of Oceania, Antarctica, and South America.
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.| Event | Time |
| First Penumbral External Contact | 2075 January 16 at 15:57:25.0 UTC |
| First Umbral External Contact | 2075 January 16 at 16:55:14.7 UTC |
| First Central Line | 2075 January 16 at 16:55:40.1 UTC |
| First Umbral Internal Contact | 2075 January 16 at 16:56:05.5 UTC |
| First Penumbral Internal Contact | 2075 January 16 at 17:58:22.3 UTC |
| Equatorial Conjunction | 2075 January 16 at 18:33:19.8 UTC |
| Greatest Duration | 2075 January 16 at 18:33:39.8 UTC |
| Greatest Eclipse | 2075 January 16 at 18:36:04.3 UTC |
| Ecliptic Conjunction | 2075 January 16 at 18:38:59.2 UTC |
| Last Penumbral Internal Contact | 2075 January 16 at 19:13:49.8 UTC |
| Last Umbral Internal Contact | 2075 January 16 at 20:16:07.2 UTC |
| Last Central Line | 2075 January 16 at 20:16:30.9 UTC |
| Last Umbral External Contact | 2075 January 16 at 20:16:54.6 UTC |
| Last Penumbral External Contact | 2075 January 16 at 21:14:48.6 UTC |
| Parameter | Value |
| Eclipse Magnitude | 1.03115 |
| Eclipse Obscuration | 1.06327 |
| Gamma | −0.27987 |
| Sun Right Ascension | 19h55m06.1s |
| Sun Declination | -20°47'51.3" |
| Sun Semi-Diameter | 16'15.5" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 19h55m12.8s |
| Moon Declination | -21°04'40.9" |
| Moon Semi-Diameter | 16'29.7" |
| Moon Equatorial Horizontal Parallax | 1°00'32.2" |
| ΔT | 101.4 s |
Eclipse season
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months 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.| January 2 Ascending node | January 16 Descending node |
| Penumbral lunar eclipse Lunar Saros 116 | Total solar eclipse Solar Saros 142 |
Related eclipses
Eclipses in 2075
- A penumbral lunar eclipse on January 2.A total solar eclipse on January 16.
- A partial lunar eclipse on June 28.
- An annular solar eclipse on July 13.
- A partial lunar eclipse on December 22.
Metonic
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of November 4, 2078
Tzolkinex
- Preceded by: Solar eclipse of December 6, 2067
- Followed by: Solar eclipse of February 27, 2082
Half-Saros
- Preceded by: Lunar eclipse of January 11, 2066
- Followed by: Lunar eclipse of January 22, 2084
Tritos
- Preceded by: Solar eclipse of February 17, 2064
- Followed by: Solar eclipse of December 16, 2085
Solar Saros 142
- Preceded by: Solar eclipse of January 5, 2057
- Followed by: Solar eclipse of January 27, 2093
Inex
- Preceded by: Solar eclipse of February 5, 2046
- Followed by: Solar eclipse of December 29, 2103
Triad
- Preceded by: Solar eclipse of March 18, 1988
- Followed by: Solar eclipse of November 17, 2161