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  • [Date]: 26 August 330 BC
    [Time ofgreatest eclipse]: 06:39:50
    [Saros cycle]: 49
    [Type]: Partial
    [Magnitude]: 0.7263
    [Centralduration]:
    [Location]: 70°42′S 90°18′E / 70.7°S 90.3°E / -70.7; 90.3
    [Path width]:
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    [Ref(s)]:

  • [Date]: 5 October 369 BC
    [Time ofgreatest eclipse]: 17:12:24
    [Saros cycle]: 57
    [Type]: Total
    [Magnitude]: 1.0304
    [Centralduration]: 02m 48s
    [Location]: 20°18′S 23°42′W / 20.3°S 23.7°W / -20.3; -23.7
    [Path width]: 108 km (67 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 13 March 312 BC
    [Time ofgreatest eclipse]: 06:17:39
    [Saros cycle]: 44
    [Type]: Total
    [Magnitude]: 1.0476
    [Centralduration]: 02m 58s
    [Location]: 64°54′N 103°42′E / 64.9°N 103.7°E / 64.9; 103.7
    [Path width]: 680 km (420 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 22 May 389 BC
    [Time ofgreatest eclipse]: 06:32:18
    [Saros cycle]: 70
    [Type]: Total
    [Magnitude]: 1.0251
    [Centralduration]: 02m 12s
    [Location]: 41°48′S 153°36′E / 41.8°S 153.6°E / -41.8; 153.6
    [Path width]: 179 km (111 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 12 April 388 BC
    [Time ofgreatest eclipse]: 01:57:00
    [Saros cycle]: 42
    [Type]: Partial
    [Magnitude]: 0.8230
    [Centralduration]:
    [Location]: 71°36′N 104°30′E / 71.6°N 104.5°E / 71.6; 104.5
    [Path width]:
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  • [Date]: 28 January 327 BC
    [Time ofgreatest eclipse]: 21:53:54
    [Saros cycle]: 74
    [Type]: Partial
    [Magnitude]: 0.5408
    [Centralduration]:
    [Location]: 69°00′S 71°30′E / 69.0°S 71.5°E / -69.0; 71.5
    [Path width]:
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About This Tool

Looking back in time, the random instrument recorded 56 total eclipses of all the eclipses recorded at 4th century BC. And there were nearly five eclipses in 374 BC. Detailed information all collated in this random tool, for those interested in astronomy friends can further view.

First of all, not every eclipse is a total solar eclipse. The Sun is about 400 times the diameter of the Moon, therefore, only when the sun and moon’s orbit “Meet”and the distance between the sun and the Earth reaches at least 400 times the distance between the Sun and the Moon, the moon can completely block the sun from the Earth’s rays, forming a total solar eclipse. Even though we’ve missed all the eclipses in the 4th century BC, but we can still use this generator to sort out the exact date, location, coordinates, time, type, Path width, Central duration, and so on.

Click the "Display All Items" button and you will get a list of solar eclipses in the 4th century BC.

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