A penumbral eclipse of the Moon occurred on 17 January, 0596 BC UT Old Style, with maximum eclipse at 08:28 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 12% of the Moon's disc for 1 hour and 45 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 1 hour and 45 minutes. Maximum eclipse was at 08:28:21 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 63.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 63, is linked to solar Saros series 70. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 08:28:21 on 17 Jan UT TDT Date/time (max) 13:37:39 on 17 Jan TDT
Saros Series 63 Number in Series 8
Penumbral Magnitiude 0.1188 Central Magnitiude -0.966
Gamma -1.5161 Path Width (km)
Delta T 5h09m Error ± 15m14s (95%)
Penumbral Duration 1h45m 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 22:11:41 UTC.