Solar eclipse of October 25, 2041
Solar eclipse of October 25, 2041 | |
---|---|
Map | |
Type of eclipse | |
Nature | Annular |
Gamma | 0.4133 |
Magnitude | 0.9467 |
Maximum eclipse | |
Duration | 367 sec (6 m 7 s) |
Coordinates | 9°54′N 162°54′E / 9.9°N 162.9°E |
Max. width of band | 213 km (132 mi) |
Times (UTC) | |
Greatest eclipse | 1:36:22 |
References | |
Saros | 134 (45 of 71) |
Catalog # (SE5000) | 9600 |
An annular solar eclipse will occur on October 25, 2041. 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.
Images
Animated path
Related eclipses
Solar eclipses of 2040-2043
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.
Ascending node | Descending node | |||
---|---|---|---|---|
119 | May 11, 2040 Partial |
124 | November 4, 2040 Annular | |
129 | April 30, 2041 Total |
134 | October 25, 2041 Annular | |
139 | April 20, 2042 Total |
144 | October 14, 2042 Annular | |
149 | April 9, 2043 Total |
154 | October 3, 2043 Annular |
Saros 134
It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428.[1]