Solar eclipse of March 10, 2081
An annular solar eclipse will occur at the Moon's ascending node of orbit on Monday, March 10, 2081, with a magnitude of 0.9304. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus. An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 2.3 days after apogee, the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of Chile, Argentina, southeastern Liberia, southern Côte d'Ivoire, Ghana, Togo, Benin, Nigeria, Cameroon, and the western Central African Republic. A partial solar eclipse will also be visible for parts of South America, Antarctica, Africa, and Southern Europe.
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 | 2081 March 10 at 12:22:46.4 UTC |
| First Umbral External Contact | 2081 March 10 at 13:30:23.7 UTC |
| First Central Line | 2081 March 10 at 13:33:33.4 UTC |
| First Umbral Internal Contact | 2081 March 10 at 13:36:43.7 UTC |
| First Penumbral Internal Contact | 2081 March 10 at 14:57:39.7 UTC |
| Equatorial Conjunction | 2081 March 10 at 14:59:36.9 UTC |
| Greatest Duration | 2081 March 10 at 15:14:48.8 UTC |
| Ecliptic Conjunction | 2081 March 10 at 15:19:08.3 UTC |
| Greatest Eclipse | 2081 March 10 at 15:23:30.7 UTC |
| Last Penumbral Internal Contact | 2081 March 10 at 15:49:56.8 UTC |
| Last Umbral Internal Contact | 2081 March 10 at 17:10:33.8 UTC |
| Last Central Line | 2081 March 10 at 17:13:42.3 UTC |
| Last Umbral External Contact | 2081 March 10 at 17:16:50.1 UTC |
| Last Penumbral External Contact | 2081 March 10 at 18:24:21.0 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.93039 |
| Eclipse Obscuration | 0.86563 |
| Gamma | −0.36528 |
| Sun Right Ascension | 23h25m55.3s |
| Sun Declination | -03°40'25.8" |
| Sun Semi-Diameter | 16'06.3" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 23h26m33.6s |
| Moon Declination | -03°57'43.0" |
| Moon Semi-Diameter | 14'46.5" |
| Moon Equatorial Horizontal Parallax | 0°54'13.5" |
| ΔT | 106.4 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.| March 10 Ascending node | March 25 Descending node |
| Annular solar eclipse Solar Saros 131 | Partial lunar eclipse Lunar Saros 143 |
Related eclipses
Eclipses in 2081
An annular solar eclipse on March 10.- A partial lunar eclipse on March 25.
- A total solar eclipse on September 3.
- A penumbral lunar eclipse on September 18.
Metonic
- Preceded by: Solar eclipse of May 22, 2077
- Followed by: Solar eclipse of December 27, 2084
Tzolkinex
- Preceded by: Solar eclipse of January 27, 2074
- Followed by: Solar eclipse of April 21, 2088
Half-Saros
- Preceded by: Lunar eclipse of March 4, 2072
- Followed by: Lunar eclipse of March 15, 2090
Tritos
- Preceded by: Solar eclipse of April 11, 2070
- Followed by: Solar eclipse of February 7, 2092
Solar Saros 131
- Preceded by: Solar eclipse of February 28, 2063
- Followed by: Solar eclipse of March 21, 2099
Inex
- Preceded by: Solar eclipse of March 30, 2052
- Followed by: Solar eclipse of February 18, 2110
Triad
- Preceded by: Solar eclipse of May 10, 1994
- Followed by: Solar eclipse of January 10, 2168