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Solar eclipse of May 22, 2058
Future partial solar eclipse
Future partial solar eclipse
| Field | Value |
|---|---|
| previous | Solar eclipse of December 26, 2057 |
| next | Solar eclipse of June 21, 2058 |
A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, May 22, 2058, with a magnitude of 0.4141. 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.
The partial solar eclipse will be visible for parts of Antarctica, southern South Africa, and southern Madagascar.
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 (UTC) |
|---|---|
| First Penumbral External Contact | 2058 May 22 at 09:05:01.4 UTC |
| Equatorial Conjunction | 2058 May 22 at 09:52:44.5 UTC |
| Ecliptic Conjunction | 2058 May 22 at 10:24:51.8 UTC |
| Greatest Eclipse | 2058 May 22 at 10:39:25.5 UTC |
| Last Penumbral External Contact | 2058 May 22 at 12:14:13.5 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.41409 |
| Eclipse Obscuration | 0.29549 |
| Gamma | −1.31939 |
| Sun Right Ascension | 03h58m00.8s |
| Sun Declination | +20°28'40.9" |
| Sun Semi-Diameter | 15'48.1" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 03h59m32.2s |
| Moon Declination | +19°18'44.2" |
| Moon Semi-Diameter | 15'09.0" |
| Moon Equatorial Horizontal Parallax | 0°55'36.1" |
| ΔT | 89.3 s |
Eclipse season
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. The first and last eclipse in this sequence is separated by one synodic month.
| May 22 | |||||
|---|---|---|---|---|---|
| Ascending node (new moon) | |||||
| June 6 | |||||
| Descending node (full moon) | |||||
| June 21 | |||||
| Ascending node (new moon) | |||||
| [[File:SE2058May22P.png | 200px]] | [[File:Lunar eclipse chart close-2058Jun06.png | 200px]] | [[File:SE2058Jun21P.png | 200px]] |
| Partial solar eclipse | |||||
| Solar Saros 119 | Total lunar eclipse | ||||
| Lunar Saros 131 | Partial solar eclipse | ||||
| Solar Saros 157 |
References
References
- "May 22, 2058 Partial Solar Eclipse". timeanddate.
- "Partial Solar Eclipse of 2058 May 22". EclipseWise.com.
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