A penumbral eclipse of the Moon occurred on 6 November, 1711 BC UT Old Style, with maximum eclipse at 00:10 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 15% of the Moon's disc for 1 hour and 44 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 1 hour and 44 minutes. Maximum eclipse was at 00:10:11 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 eclipse belongs to lunar Saros series -11.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series -11, is linked to solar Saros series -4. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 00:10:11 on 6 Nov UT TDT Date/time (max) 11:11:13 on 6 Nov TDT
Saros Series -11 Number in Series
Penumbral Magnitiude 0.1488 Central Magnitiude -0.8413
Gamma 1.4737 Path Width (km)
Delta T 11h01m Error ± 1h25m (95%)
Penumbral Duration 1h44m 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 22:11:39 UTC.