Solar eclipse of January 3, 1908

Last updated
Solar eclipse of January 3, 1908
SE1908Jan03T.png
Map
Type of eclipse
NatureTotal
Gamma 0.1934
Magnitude 1.0437
Maximum eclipse
Duration254 s (4 min 14 s)
Coordinates 11°48′S145°06′W / 11.8°S 145.1°W / -11.8; -145.1
Max. width of band149 km (93 mi)
Times (UTC)
Greatest eclipse21:45:22
References
Saros 130 (46 of 73)
Catalog # (SE5000) 9299

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, January 3, 1908, [1] [2] [3] [4] with a magnitude of 1.0437. 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 Ebon Atoll in German New Guinea (now in Marshall Islands), British Western Pacific Territories (the part now belonging to Kiribati), Line Islands (now in Kiribati), Phoenix Islands (now in Kiribati) on January 4 (Saturday), and Costa Rica on January 3 (Friday). The green line means eclipse begins or ends at sunrise or sunset. The magenta line means mid eclipse at sunrise or sunset, or northern or southern penumbra limits. The green point means eclipse obscuration of 50%. The blue line means umbral northern and southern limits.

Contents

Observations

The eclipse was observed by astronomer William Wallace Campbell of Lick Observatory, viewed from Flint Island, Kiribati, an uninhabited island in the Line Islands. The team of Lick Observatory departed from San Francisco on November 22, 1907, and arrived in Papeete, Tahiti Island, the capital of French Polynesia on December 4. After making preparations of supplies and logistics personnel, it departed again on the evening of December 7 and arrived at Flint Island on the afternoon of the 9: [5]

1908 01 03 Lick.jpg

Astronomers from the Royal Astronomical Society, Sydney Observatory and surveyors from New Zealand also observed the total eclipse near the observation site of Lick Observatory. The team successfully took images of the corona. [6]

Eclipses in 1908

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 130

Inex

Triad

Solar eclipses of 1906–1909

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. [7]

Solar eclipse series sets from 1906 to 1909
Ascending node Descending node
115 July 21, 1906
SE1906Jul21P.png
Partial		120 January 14, 1907
SE1907Jan14T.png
Total
125 July 10, 1907
SE1907Jul10A.png
Annular		130 January 3, 1908
SE1908Jan03T.png
Total
135 June 28, 1908
SE1908Jun28A.png
Annular		140 December 23, 1908
SE1908Dec23H.png
Hybrid
145 June 17, 1909
SE1909Jun17H.png
Hybrid		150 December 12, 1909
SE1909Dec12P.png
Partial

Saros 130

This eclipse is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular eclipses in the series. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occurs at the Moon’s descending node. [8]

Series members 43–56 between 1853 and 2300
434445
SE1853Nov30T.png
November 30, 1853 		SE1871Dec12T.png
December 12, 1871 		SE1889Dec22T.png
December 22, 1889
464748
SE1908Jan03T.png
January 3, 1908 		SE1926Jan14T.png
January 14, 1926 		SE1944Jan25T.png
January 25, 1944
495051
SE1962Feb05T.png
February 5, 1962 		SE1980Feb16T.png
February 16, 1980 		SE1998Feb26T.png
February 26, 1998
525354
SE2016Mar09T.png
March 9, 2016 		SE2034Mar20T.png
March 20, 2034 		SE2052Mar30T.png
March 30, 2052
555657
SE2070Apr11T.png
April 11, 2070 		SE2088Apr21T.png
April 21, 2088 		SE2106May03T.png
May 3, 2106
585960
SE2124May14T.png
May 14, 2124		 SE2142May25T.png
May 25, 2142		 SE2160Jun04T.png
June 4, 2160
616263
SE2178Jun16T.png
June 16, 2178		 SE2196Jun26T.png
June 26, 2196		 SE2214Jul08T.png
July 8, 2214
646566
SE2232Jul18T.png
July 18, 2232		 SE2250Jul30P.png
July 30, 2250		 SE2268Aug09P.png
August 9, 2268
67
SE2286Aug20P.png
August 20, 2286

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. ↑ "Obscured by the clouds". The Journal and Tribune. Knoxville, Tennessee. 1908-01-04. p. 8. Retrieved 2023-11-01– via Newspapers.com.
  2. ↑ "Clouds hide eclipse; many are disappointmented". St. Louis Globe-Democrat. St. Louis, Missouri. 1908-01-04. p. 1. Retrieved 2023-11-01– via Newspapers.com.
  3. ↑ "FLINT ISLAND PARTY VIEWS SUN ECLIPSE". The San Francisco Examiner. San Francisco, California. 1908-01-04. p. 6. Retrieved 2023-11-01– via Newspapers.com.
  4. ↑ "The sun's obscuration". The Daily Telegraph. Sydney, New South Wales, Australia. 1908-01-04. p. 10. Retrieved 2023-11-01– via Newspapers.com.
  5. ↑ Powerhouse Museum. "Solar Eclipse, Flint Island, Kiribati, 1908". Powerhouse Museum, Australia. Retrieved 11 March 2016.
  6. ↑ Sebastian Albrecht. "The Lick Observatory-Crocker Expedition to Flint Island". Journal of the Royal Astronomical Society of Canada. 2: 115–131. Archived from the original on 23 August 2019.
  7. ↑ 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.
  8. ↑ "Saros Series catalog of solar eclipses". NASA.

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References

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