A penumbral eclipse of the Moon occurred on 18 April, 1801 BC UT Old Style, with maximum eclipse at 11:32 UT. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 64% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 31 minutes.

The penumbral eclipse lasted for 3 hours and 31 minutes. Maximum eclipse was at 11:32:03 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 eclipse. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 3 eclipses:

This was the 8th eclipse in lunar Saros series 22.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 22, is linked to solar Saros series 29. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 11:32:03 on 18 Apr UT TDT Date/time (max) 23:07:28 on 18 Apr TDT
Saros Series 22 Number in Series 8
Penumbral Magnitiude 0.6444 Central Magnitiude -0.3352
Gamma 1.2007 Path Width (km)
Delta T 11h35m Error ± 1h36m (95%)
Penumbral Duration 3h31m Partial Duration
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 22:11:38 UTC.