Solar eclipse of May 18, 1901

A total solar eclipse occurred on May 18, 1901.[1][2][3][4] 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. The path of totality crossed French Madagascar (the part now belonging to Madagascar), Réunion, British Mauritius (now Mauritius), Dutch East Indies (now Indonesia), and British New Guinea (now belonging to Papua New Guinea).

Solar eclipse of May 18, 1901
Map
Type of eclipse
NatureTotal
Gamma−0.3626
Magnitude1.068
Maximum eclipse
Duration389 sec (6 m 29 s)
Coordinates1.7°S 98.4°E / -1.7; 98.4
Max. width of band238 km (148 mi)
Times (UTC)
Greatest eclipse5:33:48
References
Saros136 (31 of 71)
Catalog # (SE5000)9283

Solar eclipses 1901–1902

This eclipse is a member of the 1898–1902 solar eclipse semester series. An eclipse 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.

Solar eclipse series sets from 1898–1902
Ascending node   Descending node
111December 13, 1898

Partial		 116June 8, 1899

Partial
121December 3, 1899

Annular		 126May 28, 1900

Total
131November 22, 1900

Annular		 136May 18, 1901

Total
141November 11, 1901

Annular		 146May 7, 1902

Partial
151October 31, 1902

Partial

Saros 136

Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node.[5]

Series members 29–43 occur between 1865 and 2117
29 30 31

Apr 25, 1865
May 6, 1883
May 18, 1901
32 33 34

May 29, 1919
Jun 8, 1937
Jun 20, 1955
35 36 37

Jun 30, 1973
Jul 11, 1991
Jul 22, 2009
38 39 40

Aug 2, 2027
Aug 12, 2045
Aug 24, 2063
41 42 43

Sep 3, 2081
Sep 14, 2099
Sep 26, 2117

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Notes
  1. "Viewing the solar eclipse: Many of America's astronomers now on the other side of the globe". The Atchison Daily Globe. Atchison, Kansas. 1901-05-17. p. 7. Retrieved 2023-10-27 – via Newspapers.com.
  2. "The sun eclipsed: On the whole astronomers have been disappointed". The Fresno Morning Republican. Fresno, California. 1901-05-19. p. 8. Retrieved 2023-10-27 – via Newspapers.com.
  3. "The Eclipse of the Sun". Daily News Advertiser. Vancouver, British Columbia, Canada. 1901-05-19. p. 4. Retrieved 2023-10-27 – via Newspapers.com.
  4. "What is the solar corona?". San Francisco Chronicle. San Francisco, California. 1901-11-10. p. 6. Retrieved 2023-10-27 – via Newspapers.com.
  5. SEsaros136 at NASA.gov

References
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.