Solar eclipse of September 22, 2052
From Wikipedia, the free encyclopedia
| Solar eclipse of September 22, 2052 | |
|---|---|
| Type of eclipse | |
| Nature | Annular |
| Gamma | -0.448 |
| Magnitude | 0.9734 |
| Maximum eclipse | |
| Duration | 2m 51s |
| Coordinates | 25.7S 175E |
| Max. width of band | 106 km |
| Times (UTC) | |
| Greatest eclipse | 23:39:10 |
| References | |
| Saros | 135 (41 of 71) |
| Catalog # (SE5000) | 9624 |
An annular solar eclipse will occur on September 22, 2052. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region thousands of kilometres wide.
Contents |
Related eclipses[edit]
Solar eclipses 2051-2054[edit]
Each member 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.
| 120 | April 11, 2051 Partial |
125 | October 4, 2051 Partial |
| 130 | March 30, 2052 Total |
135 | September 22, 2052 Annular |
| 140 | March 20, 2053 Annular |
145 | September 12, 2053 Total |
| 150 | March 9, 2054 Partial |
155 | September 2, 2054 Partial |
References[edit]
| Wikimedia Commons has media related to: Solar eclipse of 2052 September 22 |
External links[edit]
| This Solar eclipse-related article is a stub. You can help Wikipedia by expanding it. |