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  • [Date]: 5 September 293 BC
    [Time ofgreatest eclipse]: 05:33:58
    [Saros cycle]: 59
    [Type]: Hybrid
    [Magnitude]: 1.0123
    [Centralduration]: 01m 14s
    [Location]: 16°12′S 146°48′E / 16.2°S 146.8°E / -16.2; 146.8
    [Path width]: 47 km (29 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 28 October 230 BC
    [Time ofgreatest eclipse]: 16:31:34
    [Saros cycle]: 78
    [Type]: Annular
    [Magnitude]: 0.9882
    [Centralduration]: 00m 47s
    [Location]: 61°00′S 70°00′W / 61.0°S 70.0°W / -61.0; -70.0
    [Path width]: 88 km (55 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 31 December 225 BC
    [Time ofgreatest eclipse]: 14:24:47
    [Saros cycle]: 57
    [Type]: Hybrid
    [Magnitude]: 1.0046
    [Centralduration]: 00m 24s
    [Location]: 43°54′S 24°06′E / 43.9°S 24.1°E / -43.9; 24.1
    [Path width]: 17 km (11 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 3 May 276 BC
    [Time ofgreatest eclipse]: 05:03:29
    [Saros cycle]: 82
    [Type]: Partial
    [Magnitude]: 0.1713
    [Centralduration]:
    [Location]: 70°18′S 155°12′W / 70.3°S 155.2°W / -70.3; -155.2
    [Path width]:
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 8 October 258 BC
    [Time ofgreatest eclipse]: 13:17:29
    [Saros cycle]: 49
    [Type]: Partial
    [Magnitude]: 0.5270
    [Centralduration]:
    [Location]: 71°42′S 68°48′W / 71.7°S 68.8°W / -71.7; -68.8
    [Path width]:
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 18 November 213 BC
    [Time ofgreatest eclipse]: 17:55:03
    [Saros cycle]: 68
    [Type]: Annular
    [Magnitude]: 0.9431
    [Centralduration]: 06m 10s
    [Location]: 29°42′S 42°24′W / 29.7°S 42.4°W / -29.7; -42.4
    [Path width]: 214 km (133 mi)
    [Geographical area]:
    [Ref(s)]:

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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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