A penumbral eclipse of the Moon occurred on 13 March, 1605 BC UT Old Style, with maximum eclipse at 00:48 UT. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 49 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.

The penumbral eclipse lasted for 4 hours and 49 minutes. Maximum eclipse was at 00:48:24 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 2 eclipses:

This eclipse belongs to lunar Saros series -3.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series -3, is linked to solar Saros series 4. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 00:48:24 on 13 Mar UT TDT Date/time (max) 11:10:32 on 13 Mar TDT
Saros Series -3 Number in Series
Penumbral Magnitiude 1.061 Central Magnitiude -0.0113
Gamma 0.9992 Path Width (km)
Delta T 10h22m Error ± 1h13m (95%)
Penumbral Duration 4h49m 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.