Solar eclipse of August 10, 1915

Summary

An annular solar eclipse occurred on August 10, 1915.[1][2][3] 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. Annularity was visible from the Pacific Ocean, with the only land being Haha-jima Group in Japan, where the eclipse occurred on August 11 because it is west of International Date Line.

Solar eclipse of August 10, 1915
Map
Type of eclipse
NatureAnnular
Gamma0.0124
Magnitude0.9853
Maximum eclipse
Duration93 s (1 min 33 s)
Coordinates16°24′N 161°24′W / 16.4°N 161.4°W / 16.4; -161.4
Max. width of band52 km (32 mi)
Times (UTC)
Greatest eclipse22:52:25
References
Saros134 (38 of 71)
Catalog # (SE5000)9316

Related eclipses edit

Solar eclipse 1913–1917 edit

This eclipse is a member of a 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.[4]

Solar eclipse series sets from 1913 to 1917
Descending node   Ascending node
114 August 31, 1913
 
Partial
119 February 25, 1914
 
Annular
124 August 21, 1914
 
Total
129 February 14, 1915
 
Annular
134 August 10, 1915
 
Annular
139 February 3, 1916
 
Total
144 July 30, 1916
 
Annular
149 January 23, 1917
 
Partial
154 July 19, 1917
 
Partial

Saros 134 edit

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with a 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. All eclipses in this series occur at the Moon’s descending node.[5]

Series members 32–48 occur between 1801 and 2100:
32 33 34
 
June 6, 1807
 
June 16, 1825
 
June 27, 1843
35 36 37
 
July 8, 1861
 
July 19, 1879
 
July 29, 1897
38 39 40
 
August 10, 1915  
August 21, 1933
 
September 1, 1951
41 42 43
 
September 11, 1969
 
September 23, 1987
 
October 3, 2005
44 45 46
 
October 14, 2023
 
October 25, 2041
 
November 5, 2059
47 48
 
November 15, 2077
 
November 27, 2095

Tritos series edit

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Notes edit

  1. ^ "Partial Eclipse of Sun Will Be Seen Here Today". The Honolulu Advertiser. Honolulu, Hawaii. 1915-08-10. p. 7. Retrieved 2023-11-12 – via Newspapers.com.
  2. ^ "FINAL 1915 ECLIPSE IS WITH US TODAY: It Will Only Be Annular, However (Whatever That Is)". The Washington Times. Washington, District of Columbia. 1915-08-10. p. 5. Retrieved 2023-11-12 – via Newspapers.com.
  3. ^ "SUN DARKENED AT NOONDAY BY FINE ECLIPSE". Honolulu Star-Bulletin. Honolulu, Hawaii. 1915-08-10. p. 1. Retrieved 2023-11-12 – via Newspapers.com.
  4. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  5. ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.

References edit

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements