A penumbral eclipse of the Moon occurred on 31 March, 1783 BC UT Old Style, with maximum eclipse at 08:53 UT. In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 9% of the Moon's disc for 1 hour and 27 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 1 hour and 27 minutes. Maximum eclipse was at 08:53:23 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 last eclipse in lunar Saros series -16.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series -16, is linked to solar Saros series -9. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 08:53:23 on 31 Mar UT TDT Date/time (max) 20:21:55 on 31 Mar TDT
Saros Series -16 Number in Series
Penumbral Magnitiude 0.0908 Central Magnitiude -0.9234
Gamma -1.5119 Path Width (km)
Delta T 11h29m Error ± 1h34m (95%)
Penumbral Duration 1h27m 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.