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Solar Eclipses of Historical Interest

Fred Espenak

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The following table of solar eclipses are each associated with some historical event of note. When selected, each eclipse links to a global map of Earth showing the region of visibility for that particular eclipse. The path of the Moon's penumbral shadow (red) covers the region of partial eclipse, while the track of the umbral shadow (blue) defines the path of total or annular eclipse. These figures are described in greater detail in the Key to Solar Eclipse Maps. Each figure is stored as a GIF of 65 kilobytes. In addition, a link to a table of eclipse path coordinates permits the plotting the track on higher detail maps.

Sources and/or literary references to many of these eclipses may be found at:

Ancient and Early Medieval Eclipses in European Sources

Eclipse Quotations

The references at the bottom of this page are also recommended for information on solar eclipses of historical interest. Those who are unfamiliar with the basic astronomy of solar eclipses may want to visit Solar Eclipses for Beginners. A complementary web page Lunar Eclipses of Historical Interest is also available.

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This web site is a work in progress. If you know of an historic eclipse of interest, please email the date and a little information or reference about the event to mailto:espenak@gsfc.nasa.gov. I will generate a map for the eclipse and add it to this page.
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Solar Eclipses: 2000 BCE to 1 BCE3
Date Eclipse
Type
Ecl. 1
Mag.
Central 2
Duration
Global
Map
Path Description/Event
-1374 May 03
(1375 BCE)
Total 1.029 02m05s map path Ugarit Eclipse
-1301 Jun 05
(1302 BCE)
Total 1.080 06m24s map path Early Chinese Eclipse
-1177 Apr 16
(1178 BCE)
Total 1.060 04m34s map path Homer's 'Odyssey'
-0898 Apr 20
(899 BCE)
Annular 0.959 03m05s map path China's 'Double-Dawn' Eclipse
-0762 Jun 15
(763 BCE)
Total 1.060 04m59s map path Assyrian Eclipse
-0647 Apr 06
(648 BCE)
Total 1.069 05m02s map path Archilochus' Eclipse
-0584 May 28
(585 BCE)
Total 1.080 06m05s map path Herodotus/Thales Eclipse (Medes vs. Lydians)
-0556 May 19
(557 BCE)
Total 1.026 02m22s map path The Siege of Larisa
-0479 Oct 02
(480 BCE)
Annular 0.932 07m58s map path Xerxes' Eclipse
-0430 Aug 03
(431 BCE)
Annular 0.984 01m04s map path Peloponnesian War
-0423 Mar 21
(424 BCE)
Annular 0.943 04m38s map path 8th Year of Peloponnesian War

Solar Eclipses: 1 CE to 2000 CE3
Date Eclipse
Type
Ecl. 1
Mag.
Central 2
Duration
Global
Map
Path Description/Event
0029 Nov 24 Total 1.022 01m59s map 1
map 2
path Crucifixion of Christ?
0033 Mar 19 Total 1.058 04m06s map path Crucifixion of Christ?
0059 Apr 30 Total 1.019 01m50s map path Plinius' Eclipse
0071 Mar 20 Hybrid 1.007 00m35s map path Plutarch's Eclipse
0346 Jun 06 Total 1.059 03m58s map path -
0418 Jul 19 Total 1.046 03m52s map path -
0569 Nov 24 Total 1.036 03m17s map path Eclipse Preceding Birth of Mohammad
0632 Jan 27 Annular 0.984 01m40s map path Death of Mohammad's Son Ibrahim
0671 Dec 07 Annular 0.924 10m18s map path -
0840 May 05 Total 1.076 05m46s map path Emperor Louis' Eclipse (Treaty of Verdun)
1230 May 14 Total 1.060 03m17s map path Major European Eclipse
1715 May 03 Total 1.063 04m14s map path Edmund Halley's Eclipse
1766 Aug 05 Annular 0.943 05m15s map path Captain Cook's Eclipse
1806 Jun 16 Total 1.060 04m55s map path Tecumseh's Eclipse
1868 Aug 18 Total 1.076 06m47s map path King of Siam's Eclipse
1878 Jul 29 Total 1.045 03m11s map path Pike's Peak Eclipse
1879 Jan 22 Annular 0.970 03m03s map path Zulu War Eclipse
1912 Apr 17 Hybrid 1.000 00m02s map path The 'Titanic' Eclipse
1919 May 29 Total 1.072 06m51s map path Einstein's Eclipse (Test of General Relativity)
1925 Jan 24 Total 1.030 02m32s map path NYC's Winter Morning Eclipse
1932 Aug 31 Total 1.026 01m45s map path Great Maine Eclipse

1Eclipse magnitude is the fraction of the Sun's diameter obscured by the Moon. For annular eclipses, the eclipse magnitude is always less than 1. For total eclipses, the eclipse magnitude is always greater than or equal to 1. For both annular and total eclipses, the value listed is actually the ratio of diameters between the Moon and the Sun.

2Central Duration is the duration of a total or annular eclipse at Greatest Eclipse. Greatest Eclipse is the instant when the axis of the Moon's shadow passes closest to Earth's center.

3BCE and CE are abbreviations for "Before Common Era" and "Common Era," respectively. They are the secular equivalents to the BC and AD dating conventions. (See: Year Dating Conventions )

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The solar ephemeris used for these predictions is based on the classic work of Newcomb [1895]. The lunar ephemeris was developed primarily from the work of Brown [1919] with improvements from Eckert, Jones and Clark [1954].

All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.

Permission is freely granted to reproduce this data when accompanied by an acknowledgment:

"Eclipse Predictions by Fred Espenak, NASA/GSFC"

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References

For more information on eclipses of historic interest, see the following:

  • Brewer, B., Eclipse, Earth View, Seattle, 1991.
  • Humphreys, Colin J. and Waddington, W. G., "Dating the Crucifixion", Nature, Vol. 306, No. 5945, p.743-746, 22 December 1983.
  • Littmann, M., Willcox, K., and Espenak, F. Totality - Eclipses of the Sun, Oxford University Press, New York, 1999.
  • Schaefer, Bradley E., "Solar Eclipses That Changed the World", Sky and Telescope, May, 1994, p.36-39.
  • Schaefer, Bradley E., "Lunar Eclipses That Changed the World", Sky and Telescope, December, 1992, p.639-642.
  • Schaefer, Bradley E., "Dating the Crucifixion", Sky and Telescope, April, 1989, p.374.
  • Schaefer, Bradley E., "Lunar Visibility and the Crucifixion", Q.Jl. R. astr. Soc., 1990, 31, p.53-67.
  • Steel, Duncan, "Eclipse", 1999

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    NASA logo
    Eclipse Predictions & WebMaster: Fred Espenak
    Planetary Systems Branch - Code 693
    e-mail: mailto:espenak@gsfc.nasa.gov

    NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771 USA

    Last revised: 2003 Jan 30 - F. Espenak

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