A penumbral eclipse of the Moon occurred on 16 March, 0311 BC UT Old Style, with maximum eclipse at 16:29 UT. At maximum eclipse, 93% 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 4 hours and 24 minutes overall.
The penumbral eclipse lasted for 4 hours and 24 minutes. Maximum eclipse was at 16:29:09 UT.
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.)
This eclipse season contains 2 eclipses:
This was the 21st eclipse in lunar Saros series 66.The surrounding eclipses in this Saros series are:
This Saros series, lunar Saros series 66, is linked to solar Saros series 73. The nearest partner eclipses in that series are:
UT Date/time (max) | 16:29:09 on 16 Mar UT | TDT Date/time (max) | 20:24:55 on 16 Mar TDT |
---|---|---|---|
Saros Series | 66 | Number in Series | 21 |
Penumbral Magnitiude | 0.9322 | Central Magnitiude | -0.1125 |
Gamma | 1.0618 | Path Width (km) | |
Delta T | 3h56m | Error | ± 11m51s (95%) |
Penumbral Duration | 4h24m | 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.