Solar eclipse of September 9, 1904

Summary

A total solar eclipse occurred on September 9, 1904.[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. 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. Totality was visible from German New Guinea (the part now belonging to Marshall Islands) on September 10 and Chile on September 9.

Solar eclipse of September 9, 1904
Map
Type of eclipse
NatureTotal
Gamma−0.1625
Magnitude1.0709
Maximum eclipse
Duration380 s (6 min 20 s)
Coordinates3°42′S 134°30′W / 3.7°S 134.5°W / -3.7; -134.5
Max. width of band234 km (145 mi)
Times (UTC)
Greatest eclipse20:44:21
References
Saros133 (39 of 72)
Catalog # (SE5000)9291

The event is mentioned in James Joyce's novel Ulysses.

Related eclipses edit

Solar eclipses 1902–1907 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 1902 to 1907
Descending node   Ascending node
108 April 8, 1902
 
Partial
113 October 1, 1902
118 March 29, 1903
 
Annular
123 September 21, 1903
 
Total
128 March 17, 1904
 
Annular
133 September 9, 1904
 
Total
138 March 6, 1905
 
Annular
143 August 30, 1905
 
Total
148 February 23, 1906
 
Partial
153 August 20, 1906
 
Partial

Saros 133 edit

Solar Saros 133, repeating every 18 years, 11 days, contains 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435, through January 13, 1526, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[5] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.

Series members 30–56 occur between 1742 and 2211
30 31 32
June 3, 1742 June 13, 1760  
June 24, 1778
33 34 35
July 4, 1796 July 17, 1814 July 27, 1832
36 37 38
August 7, 1850  
August 18, 1868
 
August 29, 1886
39 40 41
 
September 9, 1904  
September 21, 1922
 
October 1, 1940
42 43 44
 
October 12, 1958
 
October 23, 1976
 
November 3, 1994
45 46 47
 
November 13, 2012
 
November 25, 2030
 
December 5, 2048
48 49 50
 
December 17, 2066
 
December 27, 2084
 
January 8, 2103
51 52 53
 
January 19, 2121
 
January 30, 2139
 
February 9, 2157
54 55 56
 
February 21, 2175
 
March 3, 2193
 
March 15, 2211

Inex series edit

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. In the 18th century:

  • Solar Saros 127: Total Solar Eclipse of 1731 Jan 08
  • Solar Saros 128: Annular Solar Eclipse of 1759 Dec 19
  • Solar Saros 129: Annular Solar Eclipse of 1788 Nov 27
Inex series members between 1801 and 2200:
Near lunar perigee After lunar apogee
Before lunar perigee
Before lunar apogee
After lunar perigee
 
November 9, 1817
(Saros 130)
 
October 20, 1846
(Saros 131)
 
September 29, 1875
(Saros 132)
 
September 9, 1904(Saros 133)  
August 21, 1933
(Saros 134)
 
July 31, 1962
(Saros 135)
 
July 11, 1991
(Saros 136)
 
June 21, 2020
(Saros 137)
 
May 31, 2049
(Saros 138)
 
May 11, 2078
(Saros 139)
 
April 23, 2107
(Saros 140)
 
April 1, 2136
(Saros 141)
 
March 12, 2165
(Saros 142)
 
February 21, 2194
(Saros 143)

In the 23rd century:

  • Solar Saros 144: Annular Solar Eclipse of 2223 Feb 01
  • Solar Saros 145: Total Solar Eclipse of 2252 Jan 12
  • Solar Saros 146: Annular Solar Eclipse of 2280 Dec 22

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. ^ "To-day's eclipse". Evening Post. Nottingham, Nottinghamshire, England. 1904-09-09. p. 2. Retrieved 2023-10-27 – via Newspapers.com.
  2. ^ "SOLAR ECLIPSE". The Hawaiian Star. Honolulu, Hawaii. 1904-09-09. p. 8. Retrieved 2023-10-27 – via Newspapers.com.
  3. ^ "Solar Eclipse and Earthquake Shock". Altoona Tribune. Altoona, Pennsylvania. 1904-09-10. p. 1. Retrieved 2023-10-27 – 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. ^ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros133.html

References edit

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