Solar eclipse of October 14, 2088 | |
---|---|
Map
|
|
Type of eclipse | |
Nature | Annular |
Gamma | -0.5349 |
Magnitude | 0.9727 |
Maximum eclipse | |
Duration | 2m 38s |
Coordinates | 39.7S 56W |
Max. width of band | 115 km |
Times (UTC) | |
Greatest eclipse | 14:48:05 |
References | |
Saros | 135 (43 of 71) |
Catalog # (SE5000) | 9707 |
An annular solar eclipse will occur on October 14, 2088. 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, causing the sun to look like an annulus (ring), blocking most of the Sun's light. An annular eclipse appears as a partial eclipse over a region thousands of kilometres wide.
Contents |
This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
120 | May 2, 2087 Partial |
125 | October 26, 2087 Partial |
130 | April 21, 2088 Total |
135 | October 14, 2088 Annular |
140 | April 10, 2089 Annular |
145 | October 4, 2089 Total |
150 | March 31, 2090 Partial |
155 | September 23, 2090 Total |