Solar eclipse of June 8, 1956
A total solar eclipse occurred at the Moon's descending node of orbit between Friday, June 8 and Saturday, June 9, 1956, with a magnitude of 1.0581. 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 1.3 days before perigee, the Moon's apparent diameter was larger.
It began near sunrise over New Zealand on June 9, and ended west of South America on June 8. A partial eclipse was visible for most of Oceania.
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 | 1956 June 8 at 19:11:21.5 UTC |
| First Umbral External Contact | 1956 June 8 at 20:31:34.6 UTC |
| First Central Line | 1956 June 8 at 20:34:31.6 UTC |
| First Umbral Internal Contact | 1956 June 8 at 20:37:38.2 UTC |
| Greatest Eclipse | 1956 June 8 at 21:20:39.3 UTC |
| Greatest Duration | 1956 June 8 at 21:20:59.3 UTC |
| Equatorial Conjunction | 1956 June 8 at 21:21:17.5 UTC |
| Ecliptic Conjunction | 1956 June 8 at 21:29:39.0 UTC |
| Last Umbral Internal Contact | 1956 June 8 at 22:03:38.5 UTC |
| Last Central Line | 1956 June 8 at 22:06:46.5 UTC |
| Last Umbral External Contact | 1956 June 8 at 22:09:44.9 UTC |
| Last Penumbral External Contact | 1956 June 8 at 23:29:54.1 UTC |
| Parameter | Value |
| Eclipse Magnitude | 1.05810 |
| Eclipse Obscuration | 1.11958 |
| Gamma | −0.89341 |
| Sun Right Ascension | 05h07m54.5s |
| Sun Declination | +22°54'13.6" |
| Sun Semi-Diameter | 15'45.2" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 05h07m52.9s |
| Moon Declination | +22°00'05.8" |
| Moon Semi-Diameter | 16'32.9" |
| Moon Equatorial Horizontal Parallax | 1°00'44.0" |
| ΔT | 31.5 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.| May 24 Ascending node | June 8 Descending node |
| Partial lunar eclipse Lunar Saros 120 | Total solar eclipse Solar Saros 146 |
Related eclipses
Eclipses in 1956
- A partial lunar eclipse on May 24.A total solar eclipse on June 8.
- A total lunar eclipse on November 18.
- A partial solar eclipse on December 2.
Metonic
- Preceded by: Solar eclipse of August 20, 1952
- Followed by: Solar eclipse of March 27, 1960
Tzolkinex
- Preceded by: Solar eclipse of April 28, 1949
- Followed by: Solar eclipse of July 20, 1963
Half-Saros
- Preceded by: Lunar eclipse of June 3, 1947
- Followed by: Lunar eclipse of June 14, 1965
Tritos
- Preceded by: Solar eclipse of July 9, 1945
- Followed by: Solar eclipse of May 9, 1967
Solar Saros 146
- Preceded by: Solar eclipse of May 29, 1938
- Followed by: Solar eclipse of June 20, 1974
Inex
- Preceded by: Solar eclipse of June 29, 1927
- Followed by: Solar eclipse of May 19, 1985
Triad
- Preceded by: Solar eclipse of August 7, 1869
- Followed by: Solar eclipse of April 9, 2043