A penumbral eclipse of the Moon occurred on 1 June, 1645 BC UT Old Style, with maximum eclipse at 03:48 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 18% of the Moon's disc for 2 hours and 4 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 2 hours and 4 minutes. Maximum eclipse was at 03:48:26 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 2nd eclipse in lunar Saros series 33.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 33, is linked to solar Saros series 40. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 03:48:26 on 1 Jun UT TDT Date/time (max) 14:25:07 on 1 Jun TDT
Saros Series 33 Number in Series 2
Penumbral Magnitiude 0.1846 Central Magnitiude -0.8302
Gamma -1.461 Path Width (km)
Delta T 10h37m Error ± 1h18m (95%)
Penumbral Duration 2h04m 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.