A penumbral eclipse of the Moon occurred on 9 April, 1689 BC UT Old Style, with maximum eclipse at 17:33 UT. At maximum eclipse, 90% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 3 hours and 57 minutes overall.

The penumbral eclipse lasted for 3 hours and 57 minutes. Maximum eclipse was at 17:33:25 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 eclipse belongs to lunar Saros series 24.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 24, is linked to solar Saros series 31. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 17:33:25 on 9 Apr UT TDT Date/time (max) 04:26:27 on 10 Apr TDT
Saros Series 24 Number in Series
Penumbral Magnitiude 0.8975 Central Magnitiude -0.0642
Gamma 1.0578 Path Width (km)
Delta T 10h53m Error ± 1h23m (95%)
Penumbral Duration 3h57m 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.