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  • [Date]: 10 April 415 BC
    [Time ofgreatest eclipse]: 22:55:21
    [Saros cycle]: 61
    [Type]: Annular
    [Magnitude]: 0.9650
    [Centralduration]: 03m 25s
    [Location]: 29°30′N 112°42′W / 29.5°N 112.7°W / 29.5; -112.7
    [Path width]: 140 km (87 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 10 May 445 BC
    [Time ofgreatest eclipse]: 23:55:15
    [Saros cycle]: 50
    [Type]: Total
    [Magnitude]: 1.0654
    [Centralduration]: 05m 11s
    [Location]: 40°54′N 120°00′W / 40.9°N 120.0°W / 40.9; -120.0
    [Path width]: 236 km (147 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 2 July 420 BC
    [Time ofgreatest eclipse]: 20:06:15
    [Saros cycle]: 49
    [Type]: Annular
    [Magnitude]: 0.9517
    [Centralduration]: 05m 43s
    [Location]: 31°54′S 52°48′W / 31.9°S 52.8°W / -31.9; -52.8
    [Path width]: 312 km (194 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 15 October 435 BC
    [Time ofgreatest eclipse]: 03:38:57
    [Saros cycle]: 46
    [Type]: Partial
    [Magnitude]: 0.8875
    [Centralduration]:
    [Location]: 60°48′N 92°36′W / 60.8°N 92.6°W / 60.8; -92.6
    [Path width]:
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 9 May 472 BC
    [Time ofgreatest eclipse]: 16:41:49
    [Saros cycle]: 69
    [Type]: Total
    [Magnitude]: 1.0386
    [Centralduration]: 02m 06s
    [Location]: 67°18′N 92°36′W / 67.3°N 92.6°W / 67.3; -92.6
    [Path width]: 509 km (316 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 4 August 450 BC
    [Time ofgreatest eclipse]: 00:01:15
    [Saros cycle]: 38
    [Type]: Partial
    [Magnitude]: 0.1417
    [Centralduration]:
    [Location]: 62°48′N 21°12′E / 62.8°N 21.2°E / 62.8; 21.2
    [Path width]:
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    [Ref(s)]:

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About This Tool

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. Global total eclipses occur every 1.5 years on average. In the 5th century BC, we can see 62 total eclipses over the course of the century using this random tool.

In addition, in addition to total solar eclipses, partial solar eclipses, such as the existence of annular eclipses also allow astronomers to have more fun observation. Based on the observation equipment of different countries at that time, in this generator, we also list in detail the specific Time, place, type, coordinates, Magnitude, Central duration, Path width, Time of greatest eclipse and other basic knowledge required to observe an eclipse.

Click the "Display All Items" button and you will get a list of solar eclipses in the 5th century BC.

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