Solar eclipse of February 14, 1915

Last updated
Solar eclipse of February 14, 1915
SE1915Feb14A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.2024
Magnitude 0.9789
Maximum eclipse
Duration124 sec (2 m 4 s)
Coordinates 24°00′S120°42′E / 24°S 120.7°E / -24; 120.7
Max. width of band77 km (48 mi)
Times (UTC)
Greatest eclipse4:33:20
References
Saros 129 (46 of 80)
Catalog # (SE5000) 9315

An annular solar eclipse occurred on February 14, 1915. [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. 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 Australia, Papua in Dutch East Indies (today's Indonesia), German New Guinea (now belonging to Papua New Guinea), and the South Seas Mandate of Japan (the parts now belonging to FS Micronesia and Marshall Islands, including Palikir).

Contents

Solar eclipses of 1913–1917

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. [5]

Solar eclipse series sets from 1913–1917
Descending node Ascending node
114 August 31, 1913
SE1913Aug31P.png
Partial		119 February 25, 1914
SE1914Feb25A.png
Annular
124 August 21, 1914
SE1914Aug21T.png
Total		129 February 14, 1915
SE1915Feb14A.png
Annular
134 August 10, 1915
SE1915Aug10A.png
Annular		139 February 3, 1916
SE1916Feb03T.png
Total
144 July 30, 1916
SE1916Jul30A.png
Annular		149 January 23, 1917
SE1917Jan23P.png
Partial
154 July 19, 1917
SE1917Jul19P.png
Partial

Saros 129

It is a part of Saros cycle 129, repeating every 18 years, 11 days, containing 80 events. The series started with partial solar eclipse on October 3, 1103. It contains annular eclipses on May 6, 1464 through March 18, 1969, hybrid eclipses from March 29, 1987 through April 20, 2023 and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. The longest duration of totality was 3 minutes, 43 seconds on June 25, 2131 . All eclipses in this series occurs at the Moon’s ascending node. [6]

Series members 46–56 occur between 1901 and 2100:
464748
SE1915Feb14A.png
February 14, 1915 		SE1933Feb24A.png
February 24, 1933 		SE1951Mar07A.png
March 7, 1951
495051
SE1969Mar18A.png
March 18, 1969 		SE1987Mar29H.png
March 29, 1987 		SE2005Apr08H.png
April 8, 2005
525354
SE2023Apr20H.png
April 20, 2023 		SE2041Apr30T.png
April 30, 2041 		SE2059May11T.png
May 11, 2059
5556
SE2077May22T.png
May 22, 2077 		SE2095Jun02T.png
June 2, 2095

Tritos series

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.

Series members between 1801 and 2100
SE1805Dec21A.gif
December 21, 1805
(Saros 119)		 SE1816Nov19T.gif
November 19, 1816
(Saros 120)		 SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1838Sep18A.gif
September 18, 1838
(Saros 122)		 SE1849Aug18T.gif
August 18, 1849
(Saros 123)		 SE1860Jul18T.gif
July 18, 1860
(Saros 124)
SE1871Jun18A.gif
June 18, 1871
(Saros 125)		 SE1882May17T.png
May 17, 1882
(Saros 126)		 SE1893Apr16T.png
April 16, 1893
(Saros 127)
SE1904Mar17A.png
March 17, 1904
(Saros 128)		 SE1915Feb14A.png
February 14, 1915
(Saros 129)		 SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1936Dec13A.png
December 13, 1936
(Saros 131)		 SE1947Nov12A.png
November 12, 1947
(Saros 132)		 SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134)		 SE1980Aug10A.png
August 10, 1980
(Saros 135)		 SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137)		 SE2013May10A.png
May 10, 2013
(Saros 138)		 SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140)		 SE2046Feb05A.png
February 5, 2046
(Saros 141)		 SE2057Jan05T.png
January 5, 2057
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)		 SE2078Nov04A.png
November 4, 2078
(Saros 144)		 SE2089Oct04T.png
October 4, 2089
(Saros 145)
SE2100Sep04T.png
September 4, 2100
(Saros 146)

In the 22nd century:

In the 23rd century:

Notes

  1. ↑ "PARTIAL ECLIPSE TO-DAY". The Sun. Sydney, New South Wales, Australia. 1915-02-14. p. 3. Retrieved 2023-11-12– via Newspapers.com.
  2. ↑ "PARTIAL ECLIPSE OF THE SUN". The Age. Melbourne, Victoria, Victoria, Australia. 1915-02-15. p. 10. Retrieved 2023-11-12– via Newspapers.com.
  3. ↑ "SOLAR ECLIPSE. LARGE SUN SPOT VISIBLE". The Sydney Morning Herald. Sydney, New South Wales, New South Wales, Australia. 1915-02-15. p. 8. Retrieved 2023-11-12– via Newspapers.com.
  4. ↑ "OLD SOL IS ECLIPSED, BUT NOT VISIBLE HERE". Vancouver Daily World. Vancouver, British Columbia, Canada. 1915-02-15. p. 5. Retrieved 2023-11-12– via Newspapers.com.
  5. ↑ 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.
  6. ↑ Espenak, F. "NASA Catalog of Solar Eclipses of Saros 129". eclipse.gsfc.nasa.gov.

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References

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