A penumbral eclipse of the Moon occurred on 28 September, 1428 BC UT Old Style, with maximum eclipse at 15:00 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 11% of the Moon's disc for 1 hour and 29 minutes, which was essentially impossible to see.

The penumbral eclipse lasted for 1 hour and 29 minutes. Maximum eclipse was at 15:00:06 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 3rd eclipse in lunar Saros series 43.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 15:00:06 on 28 Sep UT TDT Date/time (max) 00:19:20 on 29 Sep TDT
Saros Series 43 Number in Series 3
Penumbral Magnitiude 0.1116 Central Magnitiude -0.8563
Gamma -1.4879 Path Width (km)
Delta T 9h19m Error ± 54m49s (95%)
Penumbral Duration 1h29m 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. For this eclipse, this makes the date shown on this site different to NASA's date.

Data last updated: 2015-06-21 22:11:39 UTC.