Solar eclipse of September 9, 1904

A total solar eclipse occurred at the Moon's ascending node of orbit on Friday, September 9, 1904,[1][2][3] with a magnitude of 1.0709. 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.

Observations

edit

The National Astronomical Observatory of Chile established an observation station in Taltal, Antofagasta, but the eclipse was clouded out and could not be seen. In the capital city Santiago, a partial eclipse was seen just before sunset.[4]

edit

Eclipses in 1904

edit

Metonic

edit

Tzolkinex

edit

Half-Saros

edit

Tritos

edit

Solar Saros 133

edit

Inex

edit

Triad

edit

Solar eclipses of 1902–1906

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.[5]

The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1902 to 1906
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
108 April 8, 1902
 
Partial
1.5024 113 October 1, 1902
118 March 29, 1903
 
Annular
0.8413 123 September 21, 1903
 
Total
−0.8967
128 March 17, 1904
 
Annular
0.1299 133 September 9, 1904
 
Total
−0.1625
138 March 6, 1905
 
Annular
−0.5768 143
 
August 30, 1905
 
Total
0.5708
148 February 23, 1906
 
Partial
−1.2479 153 August 20, 1906
 
Partial
1.3731

Saros 133

edit

This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 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; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]

Series members 34–55 occur between 1801 and 2200:
34 35 36
 
July 17, 1814
 
July 27, 1832
 
August 7, 1850
37 38 39
 
August 18, 1868
 
August 29, 1886
 
September 9, 1904
40 41 42
 
September 21, 1922
 
October 1, 1940
 
October 12, 1958
43 44 45
 
October 23, 1976
 
November 3, 1994
 
November 13, 2012
46 47 48
 
November 25, 2030
 
December 5, 2048
 
December 17, 2066
49 50 51
 
December 27, 2084
 
January 8, 2103
 
January 19, 2121
52 53 54
 
January 30, 2139
 
February 9, 2157
 
February 21, 2175
55
 
March 3, 2193

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. ^ W. W. Campbell (10 December 1904). "The Total Eclipse of September 9, 1904". Publications of the Astronomical Society of the Pacific. 16. Astronomical Society of the Pacific: 266–267.
  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. ^ "NASA - Catalog of Solar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.

References

edit