Solar eclipse of April 10, 2089
| Solar eclipse of April 10, 2089 | |
|---|---|
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| Type of eclipse | |
| Nature | Annular |
| Gamma | -0.3319 |
| Magnitude | 0.9919 |
| Maximum eclipse | |
| Duration | 53 sec (0 m 53 s) |
| Coordinates | Lua error in package.lua at line 80: module 'strict' not found. |
| Max. width of band | 30 km (19 mi) |
| Times (UTC) | |
| Greatest eclipse | 22:44:42 |
| References | |
| Saros | 140 (33 of 71) |
| Catalog # (SE5000) | 9708 |
An annular solar eclipse will occur on April 10, 2089. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, 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 of the Earth thousands of kilometres wide.
Related eclipses
Solar eclipses 2087-2090
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 | May 2, 2087 Partial |
125 | October 26, 2087 150px Partial |
| 130 | April 21, 2088 Total |
135 | October 14, 2088 150px Annular |
| 140 | April 10, 2089 150px Annular |
145 | October 4, 2089 Total |
| 150 | March 31, 2090 150px Partial |
155 | September 23, 2090 150px Total |
Notes
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- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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