Solar eclipse of January 14, 1907 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | 0.8628 |
Magnitude | 1.0281 |
Maximum eclipse | |
Duration | 145 sec (2 m 25 s) |
Coordinates | 38°18′N86°24′E / 38.3°N 86.4°E |
Max. width of band | 189 km (117 mi) |
Times (UTC) | |
Greatest eclipse | 6:05:43 |
References | |
Saros | 120 (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 of the solar eclipse were made from the Tian Shan Mountains.[ citation needed ]
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]
Solar eclipse series sets from 1906–1909 | ||||
---|---|---|---|---|
Ascending node | Descending node | |||
115 | July 21, 1906 Partial | 120 | January 14, 1907 Total | |
125 | July 10, 1907 Annular | 130 | January 3, 1908 Total | |
135 | June 28, 1908 Annular | 140 | December 23, 1908 Hybrid | |
145 | June 17, 1909 Hybrid | 150 | December 12, 1909 Partial |
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.
Series members 55–65 occur between 1901 and 2100 | ||
---|---|---|
55 | 56 | 57 |
January 14, 1907 | January 24, 1925 | February 4, 1943 |
58 | 59 | 60 |
February 15, 1961 | February 26, 1979 | March 9, 1997 |
61 | 62 | 63 |
March 20, 2015 | March 30, 2033 | April 11, 2051 |
64 | 65 | |
April 21, 2069 | May 2, 2087 |
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