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  • [Date]: 2 March 292 BC
    [Time ofgreatest eclipse]: 11:51:44
    [Saros cycle]: 64
    [Type]: Annular
    [Magnitude]: 0.9559
    [Centralduration]: 04m 42s
    [Location]: 34°00′S 72°30′E / 34.0°S 72.5°E / -34.0; 72.5
    [Path width]: 178 km (111 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 20 November 251 BC
    [Time ofgreatest eclipse]: 01:28:50
    [Saros cycle]: 48
    [Type]: Partial
    [Magnitude]: 0.7230
    [Centralduration]:
    [Location]: 62°36′N 101°06′W / 62.6°N 101.1°W / 62.6; -101.1
    [Path width]:
    [Geographical area]:
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  • [Date]: 13 April 201 BC
    [Time ofgreatest eclipse]: 23:12:36
    [Saros cycle]: 74
    [Type]: Annular
    [Magnitude]: 0.9382
    [Centralduration]: 06m 00s
    [Location]: 50°54′S 91°24′W / 50.9°S 91.4°W / -50.9; -91.4
    [Path width]: 483 km (300 mi)
    [Geographical area]:
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  • [Date]: 16 September 237 BC
    [Time ofgreatest eclipse]: 12:48:23
    [Saros cycle]: 79
    [Type]: Total
    [Magnitude]: 1.0366
    [Centralduration]: 02m 24s
    [Location]: 62°00′N 77°12′E / 62.0°N 77.2°E / 62.0; 77.2
    [Path width]: 272 km (169 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 25 June 205 BC
    [Time ofgreatest eclipse]: 17:33:02
    [Saros cycle]: 72
    [Type]: Total
    [Magnitude]: 1.0686
    [Centralduration]: 06m 36s
    [Location]: 1°42′S 33°06′W / 1.7°S 33.1°W / -1.7; -33.1
    [Path width]: 247 km (153 mi)
    [Geographical area]:
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  • [Date]: 18 October 240 BC
    [Time ofgreatest eclipse]: 21:21:02
    [Saros cycle]: 49
    [Type]: Partial
    [Magnitude]: 0.5077
    [Centralduration]:
    [Location]: 71°18′S 155°24′E / 71.3°S 155.4°E / -71.3; 155.4
    [Path width]:
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About This Tool

In order for a solar eclipse to occur, our moon must be almost in direct alignment with the Sun and the Earth. Solar eclipses occur when the Moon is in a new phase and crosses between the Earth and the Sun. However, eclipses at different stages can only occur in two opposite seasons each year. This makes the eclipse all the more precious. Scientists and astronomers of every age have worked tirelessly to study eclipses and use this precious time to observe the stars.

In the 3rd century BC, we can see 226 eclipses organized by a random tool, the exact date, and location of each eclipse, Time of greatest eclipse, Saros cycle, Type, Magnitude, Central duration, Location, Path width, etc. are all recorded in detail in this generator for further viewing by interested friends.

Click the "Display All Items" button and you will get a list of solar eclipses in the 3rd century BC.

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