A hybrid eclipse of the Sun occurred on 11 May, 1468 BC UT Old Style, with maximum eclipse at 18:31 UT. A fleeting hybrid eclipse covered a narrow path at most 15 km wide and lasted for just 29 seconds at the point of maximum eclipse.

The hybrid eclipse lasted for 29 seconds. Maximum eclipse was at 18:31:03 UT.

Overview Map

This map sourced from NASA Goddard Space flight Center: GSFC Eclipse Web SiteGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. (NASA Goddard Space flight Center)
https://eclipse.gsfc.nasa.gov/eclipse.html
shows the visibility of the hybrid solar eclipse. It also shows the broader area in which a partial eclipse was seen. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 3 eclipses:

This eclipse belongs to solar Saros series 24.The surrounding eclipses in this Saros series are:

This Saros series, solar Saros series 24, is linked to lunar Saros series 17. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 18:31:03 on 11 May UT TDT Date/time (max) 04:04:18 on 12 May TDT
Saros Series 24 Number in Series
Penumbral Magnitiude Central Magnitiude 1.0043
Gamma -0.0476 Path Width (km) 15
Delta T 9h33m Error ± 58m44s (95%)
Penumbral Duration Partial Duration
Total Duration 0m29s
Partial Rating Total Rating

Note that while all dates and times on this site (except where noted) are in UT, which is within a second of civil time, the dates and times shown in NASA's eclipse listingsGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. (NASA Goddard Space flight Center)
https://eclipse.gsfc.nasa.gov/eclipse.html
are in the TDT timescale. For this eclipse, this makes the date shown on this site different to NASA's date.

Data last updated: 2015-06-21 22:11:39 UTC.