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  • [Date]: 16 March 1885
    [Time ofgreatest eclipse]: 17:45:43
    [Saros cycle]: 118
    [Type]: Annular
    [Magnitude]: 0.9778
    [Centralduration]: 01m 55s
    [Location]: 48°54′N 106°06′W / 48.9°N 106.1°W / 48.9; -106.1
    [Path width]: 132 km (82 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.8030

  • [Date]: 28 May 1900
    [Time ofgreatest eclipse]: 14:53:56
    [Saros cycle]: 126
    [Type]: Total
    [Magnitude]: 1.0249
    [Centralduration]: 02m 10s
    [Location]: 44°48′N 46°30′W / 44.8°N 46.5°W / 44.8; -46.5
    [Path width]: 92 km (57 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.3943

  • [Date]: 1 February 1813
    [Time ofgreatest eclipse]: 08:58:27
    [Saros cycle]: 118
    [Type]: Annular
    [Magnitude]: 0.9820
    [Centralduration]: 01m 53s
    [Location]: 27°54′N 40°24′E / 27.9°N 40.4°E / 27.9; 40.4
    [Path width]: 91 km (57 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.7151

  • [Date]: 20 October 1892
    [Time ofgreatest eclipse]: 18:36:06
    [Saros cycle]: 122
    [Type]: Partial
    [Magnitude]: 0.9054
    [Centralduration]:
    [Location]: 61°24′N 33°18′W / 61.4°N 33.3°W / 61.4; -33.3
    [Path width]:
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 1.0286

  • [Date]: 9 August 1877
    [Time ofgreatest eclipse]: 05:30:24
    [Saros cycle]: 114
    [Type]: Partial
    [Magnitude]: 0.3889
    [Centralduration]:
    [Location]: 62°18′N 138°36′W / 62.3°N 138.6°W / 62.3; -138.6
    [Path width]:
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 1.3277

  • [Date]: 21 November 1862
    [Time ofgreatest eclipse]: 18:29:48
    [Saros cycle]: 111
    [Type]: Partial
    [Magnitude]: 0.0580
    [Centralduration]:
    [Location]: 68°48′S 99°06′E / 68.8°S 99.1°E / -68.8; 99.1
    [Path width]:
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: -1.5051

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About This Tool

For hundreds of years, Newton’s Newton’s law of universal gravitation held an unassailable position in the scientific community, for at that time, almost all astronomical observations were in perfect accord with Newton’s predictions. But in the mid 19th century, as Mercury’s orbit was also observed by astronomers, Newton’s predictions fell short. And these 242 eclipses, recorded in this random tool, perfectly explain why these errors occur.

The solar eclipse of the 19th century was so powerful that it almost changed the way many people defined eclipses. We can use the generator to find the exact date, location, type, coordinates, range, Path width, Magnitude, Central duration, Saros cycle, and more for each eclipse. The solar eclipse of this century had to wait for Einstein’s new theory of alternative gravity: the general relativity. A hundred years later, Einstein’s theory was proved correct.

Click the "Display All Items" button and you will get a list of solar eclipses in the 19th century.

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