Solar eclipse of May 9, 1910

Solar eclipse of May 9, 1910
Map
Type of eclipse
NatureTotal
Gamma−0.9437
Magnitude1.06
Maximum eclipse
Duration255 s (4 min 15 s)
Coordinates48°12′S 125°12′E / 48.2°S 125.2°E / -48.2; 125.2
Max. width of band594 km (369 mi)
Times (UTC)
Greatest eclipse5:42:13
References
Saros117 (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.

  1. ^ "May 9, 1910 Total Solar Eclipse". timeanddate. Retrieved 31 July 2024.
  2. ^ "PARTIAL ECLIPSE OF THE SUN. IMPERFECT OBSERVATION IN SYDNEY". The Sun. Sydney, New South Wales, Australia. 1910-05-09. p. 5. Retrieved 2023-11-03 – via Newspapers.com.
  3. ^ "ECLIPSE OF THE SUN. VISIBLE AT BROKEN HILL TO-DAY". The Barrier Miner. Broken Hill, New South Wales, Australia. 1910-05-09. p. 5. Retrieved 2023-11-03 – via Newspapers.com.
  4. ^ "The solar eclipse". The Daily Telegraph. Sydney, New South Wales, Australia. 1910-05-10. p. 10. Retrieved 2023-11-03 – via Newspapers.com.
  5. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 31 July 2024.