A penumbral eclipse of the Moon occurred on Wednesday 28 November, 2012 UT, lasting from 12:14–16:50 UT. This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 92% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 36 minutes. The Moon was visible from North America (the beginning of the eclipse), Asia and Australia, and most of Europe and Africa (the end of the eclipse).

The timings of the eclipse are as follows. You would have been able to see the eclipse if the Moon was up as seen from your location; but note that this penumbral eclipse would have been very difficult to see in practice:

Penumbral eclipse began: 12:14:59 UT
Maximum eclipse: 14:32:59 UT
Penumbral eclipse ended: 16:50:59 UT

During this eclipse the Moon was at apogee, making it very small. At maximum eclipse it was 0.498° in apparent diameter, which is 6.3% 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 11th eclipse in lunar Saros series 145.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 14:32:59 on 28 Nov UT TDT Date/time (max) 14:34:07 on 28 Nov TDT
Saros Series 145 Number in Series 10
Penumbral Magnitiude 0.9155 Central Magnitiude -0.1873
Gamma -1.0869 Path Width (km)
Delta T 1m08s Error ± 0m01s (95%)
Penumbral Duration 4h36m Partial Duration
Total Duration
Partial Rating Total Rating
Sun Distance 147565394 km (9.7%) Moon Distance 406347 km (99.3%)
Sun Diameter 0.540° Moon Diameter 0.490° - 0.498°
Perigee 10:22 on 14 Nov UT Apogee 19:35 on 28 Nov UT
Contact p1 12:14:59 on 28 Nov UT Contact p2
Contact u1 Contact u2
Max eclipse 14:32:59 on 28 Nov UT
Contact u3 Contact u4
Contact p3 Contact p4 16:50:59 on 28 Nov 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 22:11:46 UTC.