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  • [Date]: 17 June 1890
    [Time ofgreatest eclipse]: 09:55:05
    [Saros cycle]: 135
    [Type]: Annular
    [Magnitude]: 0.9625
    [Centralduration]: 04m 09s
    [Location]: 36°30′N 29°18′E / 36.5°N 29.3°E / 36.5; 29.3
    [Path width]: 140 km (87 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.2246

  • [Date]: 22 December 1889
    [Time ofgreatest eclipse]: 12:54:15
    [Saros cycle]: 130
    [Type]: Total
    [Magnitude]: 1.0449
    [Centralduration]: 04m 18s
    [Location]: 12°42′S 12°48′W / 12.7°S 12.8°W / -12.7; -12.8
    [Path width]: 152 km (94 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.1888

  • [Date]: 8 September 1885
    [Time ofgreatest eclipse]: 20:51:52
    [Saros cycle]: 123
    [Type]: Total
    [Magnitude]: 1.0332
    [Centralduration]: 02m 31s
    [Location]: 49°36′S 156°30′W / 49.6°S 156.5°W / -49.6; -156.5
    [Path width]: 211 km (131 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: -0.8489

  • [Date]: 31 January 1870
    [Time ofgreatest eclipse]: 15:26:25
    [Saros cycle]: 148
    [Type]: Partial
    [Magnitude]: 0.4781
    [Centralduration]:
    [Location]: 69°54′S 100°00′E / 69.9°S 100.0°E / -69.9; 100.0
    [Path width]:
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: -1.2829

  • [Date]: 30 October 1883
    [Time ofgreatest eclipse]: 23:50:54
    [Saros cycle]: 141
    [Type]: Annular
    [Magnitude]: 0.9238
    [Centralduration]: 10m 17s
    [Location]: 15°36′N 174°54′W / 15.6°N 174.9°W / 15.6; -174.9
    [Path width]: 331 km (206 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: 0.5030

  • [Date]: 6 May 1883
    [Time ofgreatest eclipse]: 21:53:49
    [Saros cycle]: 136
    [Type]: Total
    [Magnitude]: 1.0634
    [Centralduration]: 05m 58s
    [Location]: 8°06′S 144°36′W / 8.1°S 144.6°W / -8.1; -144.6
    [Path width]: 229 km (142 mi)
    [Geographical area]:
    [Ref(s)]:
    [Gamma]: -0.4250

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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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