A penumbral eclipse of the Moon occurred on 11 May, 0734 BC UT Old Style, with maximum eclipse at 12:15 UT. In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 23 minutes exactly, it was impossible to see in practice.

The penumbral eclipse lasted for 23 minutes exactly. Maximum eclipse was at 12:15:48 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 last eclipse in lunar Saros series 19.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 19, is linked to solar Saros series 26. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 12:15:48 on 11 May UT TDT Date/time (max) 18:01:26 on 11 May TDT
Saros Series 19 Number in Series
Penumbral Magnitiude 0.0063 Central Magnitiude -1.0025
Gamma 1.5565 Path Width (km)
Delta T 5h46m Error ± 17m01s (95%)
Penumbral Duration 23m00s 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.