A penumbral eclipse of the Moon occurred on 8 May, 0267 BC UT Old Style, with maximum eclipse at 14:23 UT. In this virtually non-existant eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow; although the eclipse lasted 16 minutes and 23 seconds, it was impossible to see in practice.

The penumbral eclipse lasted for 16 minutes and 23 seconds. Maximum eclipse was at 14:23:19 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 1st eclipse in lunar Saros series 75.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 75, is linked to solar Saros series 82. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 14:23:19 on 8 May UT TDT Date/time (max) 18:09:15 on 8 May TDT
Saros Series 75 Number in Series 1
Penumbral Magnitiude 0.0028 Central Magnitiude -1.0667
Gamma -1.5751 Path Width (km)
Delta T 3h46m Error ± 11m22s (95%)
Penumbral Duration 16m23s 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.