A partial eclipse of the Moon occurred on 13 April, 1095 BC UT Old Style, with maximum eclipse at 08:03 UT. The Earth's shadow on the moon was clearly visible in this eclipse, with 22% of the Moon in shadow; the partial eclipse lasted for 1 hour and 40 minutes.

The penumbral eclipse lasted for 4 hours and 16 minutes. The partial eclipse lasted for 1 hour and 40 minutes. Maximum eclipse was at 08:03:29 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 eclipse. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This eclipse belongs to lunar Saros series 14.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 14, is linked to solar Saros series 21. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 08:03:29 on 13 Apr UT TDT Date/time (max) 15:33:56 on 13 Apr TDT
Saros Series 14 Number in Series
Penumbral Magnitiude 1.1644 Central Magnitiude 0.2218
Gamma -0.9072 Path Width (km)
Delta T 7h30m Error ± 26m43s (95%)
Penumbral Duration 4h16m Partial Duration 1h40m
Total Duration
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.

Data last updated: 2015-06-21 22:11:40 UTC.