Solar eclipse of March 21, 2099
An annular solar eclipse will occur at the Moon's ascending node of orbit between Saturday, March 21 and Sunday, March 22, 2099, with a magnitude of 0.93. 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 2.1 days after apogee, the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of the Auckland Islands, Chatham Island, and French Polynesia. A partial solar eclipse will also be visible for parts of eastern Australia, Oceania, Antarctica, Hawaii, Mexico, Central America, and the southwestern United States.
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 | 2099 March 21 at 19:54:47.9 UTC |
| First Umbral External Contact | 2099 March 21 at 21:03:08.8 UTC |
| First Central Line | 2099 March 21 at 21:06:17.6 UTC |
| First Umbral Internal Contact | 2099 March 21 at 21:09:27.2 UTC |
| First Penumbral Internal Contact | 2099 March 21 at 22:37:38.5 UTC |
| Equatorial Conjunction | 2099 March 21 at 22:27:57.2 UTC |
| Ecliptic Conjunction | 2099 March 21 at 22:49:43.7 UTC |
| Greatest Duration | 2099 March 21 at 22:54:15.0 UTC |
| Greatest Eclipse | 2099 March 21 at 22:54:32.0 UTC |
| Last Penumbral Internal Contact | 2099 March 21 at 23:12:04.5 UTC |
| Last Umbral Internal Contact | 2099 March 22 at 00:39:54.6 UTC |
| Last Central Line | 2099 March 22 at 00:43:02.6 UTC |
| Last Umbral External Contact | 2099 March 22 at 00:46:09.5 UTC |
| Last Penumbral External Contact | 2099 March 22 at 01:54:23.7 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.93180 |
| Eclipse Obscuration | 0.86826 |
| Gamma | −0.40163 |
| Sun Right Ascension | 00h06m00.9s |
| Sun Declination | +00°39'05.5" |
| Sun Semi-Diameter | 16'03.5" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 00h06m43.3s |
| Moon Declination | +00°20'09.1" |
| Moon Semi-Diameter | 14'45.5" |
| Moon Equatorial Horizontal Parallax | 0°54'09.7" |
| ΔT | 122.8 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 21 Ascending node | April 5 Descending node |
| Annular solar eclipse Solar Saros 131 | Partial lunar eclipse Lunar Saros 143 |
Related eclipses
Eclipses in 2099
An annular solar eclipse on March 21.- A partial lunar eclipse on April 5.
- A total solar eclipse on September 14.
- A penumbral lunar eclipse on September 29.
Metonic
- Preceded by: Solar eclipse of June 2, 2095
- Followed by: Solar eclipse of January 8, 2103
Tzolkinex
- Preceded by: Solar eclipse of February 7, 2092
- Followed by: Solar eclipse of May 3, 2106
Half-Saros
- Preceded by: Lunar eclipse of March 15, 2090
- Followed by: Lunar eclipse of March 27, 2108
Tritos
- Preceded by: Solar eclipse of April 21, 2088
- Followed by: Solar eclipse of February 18, 2110
Solar Saros 131
- Preceded by: Solar eclipse of March 10, 2081
- Followed by: Solar eclipse of April 2, 2117
Inex
- Preceded by: Solar eclipse of April 11, 2070
- Followed by: Solar eclipse of March 1, 2128
Triad
- Preceded by: Solar eclipse of May 20, 2012
- Followed by: Solar eclipse of January 20, 2186