Random  | Best Random Tools

  • [Date]: 28 May 45 BC
    [Time ofgreatest eclipse]: 15:49:54
    [Saros cycle]: 85
    [Type]: Partial
    [Magnitude]: 0.8701
    [Centralduration]:
    [Location]: 63°24′N 154°12′W / 63.4°N 154.2°W / 63.4; -154.2
    [Path width]:
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 3 January 56 BC
    [Time ofgreatest eclipse]: 03:05:23
    [Saros cycle]: 79
    [Type]: Hybrid
    [Magnitude]: 1.0054
    [Centralduration]: 00m 31s
    [Location]: 32°30′N 171°48′E / 32.5°N 171.8°E / 32.5; 171.8
    [Path width]: 34 km (21 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 3 December 46 BC
    [Time ofgreatest eclipse]: 07:59:17
    [Saros cycle]: 80
    [Type]: Annular
    [Magnitude]: 0.9105
    [Centralduration]: 07m 10s
    [Location]: 71°42′S 63°18′E / 71.7°S 63.3°E / -71.7; 63.3
    [Path width]: 592 km (368 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 31 August 51 BC
    [Time ofgreatest eclipse]: 23:33:54
    [Saros cycle]: 63
    [Type]: Total
    [Magnitude]: 1.0290
    [Centralduration]: 02m 38s
    [Location]: 28°42′S 139°12′W / 28.7°S 139.2°W / -28.7; -139.2
    [Path width]: 127 km (79 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 3 February 86 BC
    [Time ofgreatest eclipse]: 03:13:49
    [Saros cycle]: 68
    [Type]: Annular
    [Magnitude]: 0.9709
    [Centralduration]: 03m 15s
    [Location]: 25°00′S 175°00′W / 25.0°S 175.0°W / -25.0; -175.0
    [Path width]: 105 km (65 mi)
    [Geographical area]:
    [Ref(s)]:

  • [Date]: 5 January 29 BC
    [Time ofgreatest eclipse]: 09:33:30
    [Saros cycle]: 60
    [Type]: Annular
    [Magnitude]: 0.9915
    [Centralduration]: 00m 58s
    [Location]: 12°36′N 84°06′E / 12.6°N 84.1°E / 12.6; 84.1
    [Path width]: 37 km (23 mi)
    [Geographical area]:
    [Ref(s)]:

New Random Display   Display All Items(251)

About This Tool

Astronomical phenomena such as a total solar eclipse could provide a unique opportunity to test Einstein’s theory because the light paths of other distant objects can bend as they pass near the Sun, but it is still visible to sun watchers on Earth because the sky darkens when the sun is completely blocked by the Moon. Data on eclipses by astronomers have been recorded as early as 1st century BC, and detailed information is stored in this random tool for further viewing by interested parties.

Details of these eclipses in the 1st century BC can also be seen through the generator. There were 92 partial eclipses, 77 annular eclipses, 65 total, and 17 hybrid eclipses. If you need to see specific data for each view, date of occurrence, Saros cycle, Magnitude, Type, Central duration, Path width, Location, etc., remember the very detailed form of this record for the favorites builder.

Click the "Display All Items" button and you will get a list of solar eclipses in the 1st century BC.

Copyright © 2024 BestRandoms.com All rights reserved.