Solar eclipse of May 9, 1910 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.9437 |
Magnitude | 1.06 |
Maximum eclipse | |
Duration | 255 s (4 min 15 s) |
Coordinates | 48°12′S 125°12′E / 48.2°S 125.2°E |
Max. width of band | 594 km (369 mi) |
Times (UTC) | |
Greatest eclipse | 5:42:13 |
References | |
Saros | 117 (63 of 71) |
Catalog # (SE5000) | 9304 |
A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, May 9, 1910,[1][2][3][4] with a magnitude of 1.06. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring only about 10 hours after perigee (on May 8, 1910, at 19:20 UTC), the Moon's apparent diameter was larger.[5]
Totality was visible from part of Wilkes Land in Antarctica and Tasmania in Australia. A partial eclipse was visible for parts of Antarctica, Australia, and Southeast Asia.