Solar eclipse of May 19, 1985
Template:Short description Script error: No such module "Solar eclipse". A partial solar eclipse occurred at the Moon's ascending node of orbit between Sunday, May 19 and Monday, May 20, 1985,[1] with a magnitude of 0.8406. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial eclipse was visible near sunrise on May 20 over Japan and northeast Russia and ended on May 19 over Alaska and near sunset over northern Canada and Greenland.
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.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1985 May 19 at 19:15:42.2 UTC |
| Greatest Eclipse | 1985 May 19 at 21:29:37.8 UTC |
| Ecliptic Conjunction | 1985 May 19 at 21:42:01.7 UTC |
| Equatorial Conjunction | 1985 May 19 at 22:11:12.4 UTC |
| Last Penumbral External Contact | 1985 May 19 at 23:43:13.0 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.84064 |
| Eclipse Obscuration | 0.77714 |
| Gamma | 1.07197 |
| Sun Right Ascension | 03h46m23.8s |
| Sun Declination | +19°54'02.6" |
| Sun Semi-Diameter | 15'48.3" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 03h45m05.8s |
| Moon Declination | +20°49'15.8" |
| Moon Semi-Diameter | 14'49.5" |
| Moon Equatorial Horizontal Parallax | 0°54'24.6" |
| ΔT | 54.5 s |
Eclipse season
Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) 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 4 Descending node (full moon) |
May 19 Ascending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-1985May04.png | File:SE1985May19P.png |
| Total lunar eclipse Lunar Saros 121 |
Partial solar eclipse Solar Saros 147 |
Related eclipses
Eclipses in 1985
- A total lunar eclipse on May 4.
- A partial solar eclipse on May 19.
- A total lunar eclipse on October 28.
- A total solar eclipse on November 12.
Metonic
- Preceded by: Solar eclipse of July 31, 1981
- Followed by: Solar eclipse of March 7, 1989
Tzolkinex
- Preceded by: Solar eclipse of April 7, 1978
- Followed by: Solar eclipse of June 30, 1992
Half-Saros
- Preceded by: Lunar eclipse of May 13, 1976
- Followed by: Lunar eclipse of May 25, 1994
Tritos
- Preceded by: Solar eclipse of June 20, 1974
- Followed by: Solar eclipse of April 17, 1996
Solar Saros 147
- Preceded by: Solar eclipse of May 9, 1967
- Followed by: Solar eclipse of May 31, 2003
Inex
- Preceded by: Solar eclipse of June 8, 1956
- Followed by: Solar eclipse of April 29, 2014
Triad
- Preceded by: Solar eclipse of July 18, 1898
- Followed by: Solar eclipse of March 19, 2072
Solar eclipses of 1982–1985
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[3]
The partial solar eclipses on January 25, 1982 and July 20, 1982 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 1982 to 1985 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | June 21, 1982 File:SE1982Jun21P.png Partial |
−1.2102 | 122 | December 15, 1982 File:SE1982Dec15P.png Partial |
1.1293 | |
| 127 | June 11, 1983 File:SE1983Jun11T.png Total |
−0.4947 | 132 | December 4, 1983 File:SE1983Dec04A.png Annular |
0.4015 | |
| 137 | May 30, 1984 File:SE1984May30A.png Annular |
0.2755 | 142 File:Solar eclipse of 22 November 1984.JPG Partial in Gisborne, New Zealand |
November 22, 1984 File:SE1984Nov22T.png Total |
−0.3132 | |
| 147 | May 19, 1985 File:SE1985May19P.png Partial |
1.072 | 152 | November 12, 1985 File:SE1985Nov12T.png Total |
−0.9795 | |
Saros 147
Template:Solar Saros series 147
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
Tritos series
Template:Solar Tritos series 2007 March 19
Inex series
Template:Solar Inex series 2014 April 29
References
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External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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