A penumbral eclipse of the Moon occurred on 16 October, 0043 BC UT Old Style, with maximum eclipse at 12:25 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 17% of the Moon's disc for 2 hours and 8 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 2 hours and 8 minutes. Maximum eclipse was at 12:25:11 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 was the 4th eclipse in lunar Saros series 84.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 84, is linked to solar Saros series 91. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 12:25:11 on 16 Oct UT TDT Date/time (max) 15:27:47 on 16 Oct TDT
Saros Series 84 Number in Series 4
Penumbral Magnitiude 0.1734 Central Magnitiude -0.9243
Gamma 1.4899 Path Width (km)
Delta T 3h03m Error ± 9m03s (95%)
Penumbral Duration 2h08m 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 22:11:42 UTC.