Solar eclipse of August 22, 1979
An annular solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, August 22, 1979, with a magnitude of 0.9329. 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 15 hours before apogee, the Moon's apparent diameter was smaller.
Annularity was visible for a part of Antarctica. A partial eclipse was visible for parts of southern South America and Antarctica. This was the last of 40 umbral eclipses in Solar Saros 125.
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 | 1979 August 22 at 14:55:55.6 UTC |
| First Umbral External Contact | 1979 August 22 at 16:43:17.2 UTC |
| First Central Line | 1979 August 22 at 16:51:47.8 UTC |
| First Umbral Internal Contact | 1979 August 22 at 17:03:32.7 UTC |
| Ecliptic Conjunction | 1979 August 22 at 17:11:15.7 UTC |
| Greatest Duration | 1979 August 22 at 17:22:05.7 UTC |
| Greatest Eclipse | 1979 August 22 at 17:22:38.0 UTC |
| Equatorial Conjunction | 1979 August 22 at 17:52:40.4 UTC |
| Last Umbral Internal Contact | 1979 August 22 at 17:41:20.6 UTC |
| Last Central Line | 1979 August 22 at 17:53:06.4 UTC |
| Last Umbral External Contact | 1979 August 22 at 18:01:37.8 UTC |
| Last Penumbral External Contact | 1979 August 22 at 19:49:07.3 UTC |
| Parameter | Value |
| Eclipse Magnitude | 0.93295 |
| Eclipse Obscuration | 0.87039 |
| Gamma | −0.96319 |
| Sun Right Ascension | 10h04m36.4s |
| Sun Declination | +11°48'55.0" |
| Sun Semi-Diameter | 15'48.8" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 10h03m42.7s |
| Moon Declination | +10°58'46.8" |
| Moon Semi-Diameter | 14'42.1" |
| Moon Equatorial Horizontal Parallax | 0°53'57.5" |
| ΔT | 50.2 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.| August 22 Ascending node | September 6 Descending node |
| Annular solar eclipse Solar Saros 125 | Total lunar eclipse Lunar Saros 137 |
Related eclipses
Eclipses in 1979
- A total solar eclipse on February 26.
- A partial lunar eclipse on March 13.An annular solar eclipse on August 22.
- A total lunar eclipse on September 6.
Metonic
- Preceded by: Solar eclipse of November 3, 1975
- Followed by: Solar eclipse of June 11, 1983
Tzolkinex
- Preceded by: Solar eclipse of July 10, 1972
- Followed by: Solar eclipse of October 3, 1986
Half-Saros
- Preceded by: Lunar eclipse of August 17, 1970
- Followed by: Lunar eclipse of August 27, 1988
Tritos
- Preceded by: Solar eclipse of September 22, 1968
- Followed by: Solar eclipse of July 22, 1990
Solar Saros 125
- Preceded by: Solar eclipse of August 11, 1961
- Followed by: Solar eclipse of September 2, 1997
Inex
- Preceded by: Solar eclipse of September 12, 1950
- Followed by: Solar eclipse of August 1, 2008
Triad
- Preceded by: Solar eclipse of October 20, 1892
- Followed by: Solar eclipse of June 22, 2066