Solar eclipse of August 30, 1905

Last updated

Solar eclipse of August 30, 1905
PSM V68 D565 Sun corona of August 20 1905 taken with 40 foot camera.png
SE1905Aug30T.png
Map
Type of eclipse
NatureTotal
Gamma 0.5708
Magnitude 1.0477
Maximum eclipse
Duration226 s (3 min 46 s)
Coordinates 42°30′N4°18′W / 42.5°N 4.3°W / 42.5; -4.3
Max. width of band192 km (119 mi)
Times (UTC)
Greatest eclipse13:07:26
References
Saros 143 (17 of 72)
Catalog # (SE5000) 9293

A total solar eclipse occurred on August 30, 1905. [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 Canada, Newfoundland Colony (now belonging to Canada), Spain, French Algeria (now Algeria), French Tunisia (now Tunisia), Ottoman Tripolitania (now Libya) include the capital Tripoli, Egypt, Ottoman Empire (the parts now belonging to Saudi Arabia) including Mecca, Emirate of Jabal Shammar (now belonging to Saudi Arabia), Aden Protectorate (now belonging to Yemen), and Muscat and Oman (now Oman).

Contents

This eclipse was observed from Alcalà de Xivert in Spain. [4] It was also observed by members of the British Astronomical Association from various locations. [5] [6]

An eclipse-viewing party at Daroca PSM V68 D557 Eclipse party at daroca.png
An eclipse-viewing party at Daroca
Painting by Enrique Simonet Enrique Simonet - Eclipse - 1905.JPG
Painting by Enrique Simonet

Solar eclipses of 1902–1907

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 1902 to 1907
Descending node Ascending node
108 April 8, 1902
SE1902Apr08P.png
Partial
113October 1, 1902
118 March 29, 1903
SE1903Mar29A.png
Annular
123 September 21, 1903
SE1903Sep21T.png
Total
128 March 17, 1904
SE1904Mar17A.png
Annular
133 September 9, 1904
SE1904Sep09T.png
Total
138 March 6, 1905
SE1905Mar06A.png
Annular
143 August 30, 1905
SE1905Aug30T.png
Total
148 February 23, 1906
SE1906Feb23P.png
Partial
153 August 20, 1906
SE1906Aug20P.png
Partial

Solar 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8910
SE1743May23P.png
May 23, 1743
SE1761Jun03P.png
June 3, 1761
SE1779Jun14P.png
June 14, 1779
111213
SE1797Jun24T.png
June 24, 1797
SE1815Jul06T.png
July 6, 1815
SE1833Jul17T.png
July 17, 1833
141516
SE1851Jul28T.png
July 28, 1851
SE1869Aug07T.png
August 7, 1869
SE1887Aug19T.png
August 19, 1887
171819
SE1905Aug30T.png
August 30, 1905
SE1923Sep10T.png
September 10, 1923
SE1941Sep21T.png
September 21, 1941
202122
SE1959Oct02T.png
October 2, 1959
SE1977Oct12T.png
October 12, 1977
SE1995Oct24T.png
October 24, 1995
232425
SE2013Nov03H.png
November 3, 2013
SE2031Nov14H.png
November 14, 2031
SE2049Nov25H.png
November 25, 2049
262728
SE2067Dec06H.png
December 6, 2067
SE2085Dec16A.png
December 16, 2085

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. In the 19th century:

In the 22nd century:

Notes

  1. "The Coming Total Solar Eclipse Of Sun". The Brantford Weekly Expositor. Brantford, Ontario, Canada. August 31, 1905. p. 12. Retrieved October 27, 2023 via Newspapers.com.
  2. "OBSERVERS' SUCCESS. DETAILS OF THE ECLIPSE FROM SOUTHERN STATIONS". Evening Standard. London, Greater London, England. August 31, 1905. p. 12. Retrieved October 27, 2023 via Newspapers.com.
  3. "OLD SOL'S TOTAL ECLIPSE". The Sabetha Republican-Herald. Sabetha, Kansas. August 31, 1905. p. 6. Retrieved October 27, 2023 via Newspapers.com.
  4. Fabricio Cardenas, Vieux papiers des Pyrénées-Orientales, Eclipse solaire de 1905 à Perpignan, 20 March 2015
  5. British Astronomical Association; Levander, Frederick William (1906). The total solar eclipse 1905 : Reports of observations made by members of the British Astronomical Association of the total solar eclipse of 1905, August 30. University of California Libraries. London : British Astronomical Association.
  6. "Page 8". The Guardian. London, Greater London, England. August 31, 1905. p. 8. Retrieved October 27, 2023 via Newspapers.com.
  7. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.

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References