July 1982 lunar eclipse
A total lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, July 6, 1982, with an umbral magnitude of 1.7180. It was a central lunar eclipse, in which part of the Moon passed through the center of the Earth's shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.2 days after apogee, the Moon's apparent diameter was smaller. It was the longest total lunar eclipse since the 1859 eclipse.
Visibility
The eclipse was completely visible over western and central North America, western South America, and Antarctica, seen rising over northwestern North America, Australia, and the western Pacific Ocean and setting over northeastern North America, eastern South America, and west and southern Africa.Eclipse details
Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.| Parameter | Value |
| Penumbral Magnitude | 2.78600 |
| Umbral Magnitude | 1.71795 |
| Gamma | −0.05792 |
| Sun Right Ascension | 07h00m26.1s |
| Sun Declination | +22°42'50.6" |
| Sun Semi-Diameter | 15'43.9" |
| Sun Equatorial Horizontal Parallax | 08.6" |
| Moon Right Ascension | 19h00m26.1s |
| Moon Declination | -22°45'58.4" |
| Moon Semi-Diameter | 14'43.7" |
| Moon Equatorial Horizontal Parallax | 0°54'03.4" |
| ΔT | 52.6 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. The first and last eclipse in this sequence is separated by one synodic month.| June 21 Ascending node | July 6 Descending node | July 20 Ascending node |
| Partial solar eclipse Solar Saros 117 | Total lunar eclipse Lunar Saros 129 | Partial solar eclipse Solar Saros 155 |
Related eclipses
Eclipses in 1982
- A total lunar eclipse on January 9.
- A partial solar eclipse on January 25.
- A partial solar eclipse on June 21.A total lunar eclipse on July 6.
- A partial solar eclipse on July 20.
- A partial solar eclipse on December 15.
- A total lunar eclipse on December 30.
Metonic
- Preceded by: Lunar eclipse of September 16, 1978
- Followed by: Lunar eclipse of April 24, 1986
Tzolkinex
- Preceded by: Lunar eclipse of May 25, 1975
- Followed by: Lunar eclipse of August 17, 1989
Half-Saros
- Preceded by: Solar eclipse of June 30, 1973
- Followed by: Solar eclipse of July 11, 1991
Tritos
- Preceded by: Lunar eclipse of August 6, 1971
- Followed by: Lunar eclipse of June 4, 1993
Lunar Saros 129
- Preceded by: Lunar eclipse of June 25, 1964
- Followed by: Lunar eclipse of July 16, 2000
Inex
- Preceded by: Lunar eclipse of July 26, 1953
- Followed by: Lunar eclipse of June 15, 2011
Triad
- Preceded by: Lunar eclipse of September 4, 1895
- Followed by: Lunar eclipse of May 6, 2069
Half-Saros cycle
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days. This lunar eclipse is related to two total solar eclipses of Solar Saros 136.| June 30, 1973 | July 11, 1991 |