Solar eclipse of January 14, 1907

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Solar eclipse of January 14, 1907
SE1907Jan14T.png
Map
Type of eclipse
NatureTotal
Gamma0.8628
Magnitude1.0281
Maximum eclipse
Duration145 sec (2 m 25 s)
Coordinates38°18′N 86°24′E / 38.3°N 86.4°E / 38.3; 86.4
Max. width of band189 km (117 mi)
Times (UTC)
Greatest eclipse6:05:43
References
Saros120 (55 of 71)
Catalog # (SE5000)9297

A total solar eclipse occurred on January 14, 1907. 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 Russian Empire (the parts now belonging to Russia, Kazakhstan, Uzbekistan, Tajikistan and Kyrgyzstan) and China (now northwestern China, Mongolia and northern part of northeastern China).

Observations[edit]

Supervision of a solar eclipse near station Chernjaevo on January, 1st, 1907

Observations of the solar eclipse were made from the Tian Shan Mountains.[citation needed]

Related eclipses[edit]

Solar eclipses 1906–1909[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.[1]

Saros 120[edit]

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending node.

See also[edit]

Notes[edit]

  1. ^ 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.

References[edit]