A penumbral eclipse of the Moon occurred on 27 February, 1477 UT Old Style, with maximum eclipse at 20:08 UT. At maximum eclipse, 91% 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 23 minutes overall.

The penumbral eclipse lasted for 4 hours and 23 minutes. Maximum eclipse was at 20:08:09 UT.

During this eclipse the Moon was 10 days after perigee and 5 days before apogee. At maximum eclipse it was 0.515° in apparent diameter, which is 2.9% smaller than average. The statistics page has information on the ranges of the sizes of the Sun and Moon.

Interactive Map

This map shows the visibility of the eclipse at maximum eclipse, when it was visible within the bright area on the map. Note that the map is approximate, and if you were near the edge of the area of visibility, the moon was very close to the horizon and may not have been practically visible.

You can use the zoom controls to zoom in and out, and pan to see areas of interest. The green marker in the centre shows where the Moon will be directly overhead at maximum eclipse.

Overview Map

This map sourced from NASA's Eclipse Web Site shows the visibility of the eclipse. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This was the 19th eclipse in lunar Saros series 124.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 20:08:09 on 27 Feb UT TDT Date/time (max) 20:11:49 on 27 Feb TDT
Saros Series 124 Number in Series 18
Penumbral Magnitiude 0.9104 Central Magnitiude -0.1454
Gamma 1.0767 Path Width (km)
Delta T 3m40s Error ± 0m39s (95%)
Penumbral Duration 4h23m Partial Duration
Total Duration
Partial Rating Total Rating
Sun Distance 148868297 km (36.7%) Moon Distance 392486 km (71.7%)
Sun Diameter 0.536° Moon Diameter 0.507° - 0.515°
Perigee 11:37 on 17 Feb UT Apogee 07:48 on 5 Mar UT

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 listings are in the TDT timescale.

The Sun and Moon distances are shown in km, and as a percentage of their minimum - maximum distances; hence 0% is the closest possible (Earth's perihelion, or the Moon's closest possible perigee) and 100% is the farthest (aphelion, the farthest apogee). The statistics page has information on the ranges of sizes of the Sun and Moon.

Data last updated: 2015-06-21 22:11:45 UTC.