A penumbral eclipse of the Moon occurs on Thursday 30 October, 2031 UT, lasting from 05:49–09:41 UT. This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 72% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 52 minutes. The Moon will be visible in the Americas, eastern Asia and Australia, and western Europe and Africa.

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

Penumbral eclipse begins: 05:49:29 UT
Maximum eclipse: 07:45:26 UT
Penumbral eclipse ends: 09:41:15 UT

During this eclipse the Moon will be 7 days after perigee and 7 days before apogee. At maximum eclipse it will be 0.526° in apparent diameter, which is 0.9% 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 will be visible within the bright area on the map. Note that the map is approximate, and if you are near the edge of the area of visibility, the moon will be very close to the horizon and may not be 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 is the 53rd eclipse in lunar Saros series 117.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 07:45:26 on 30 Oct UT TDT Date/time (max) 07:46:45 on 30 Oct TDT
Saros Series 117 Number in Series 52
Penumbral Magnitiude 0.7161 Central Magnitiude -0.3204
Gamma 1.1773 Path Width (km)
Delta T 1m19s Error ± 0m13s (95%)
Penumbral Duration 3h52m Partial Duration
Total Duration
Partial Rating Total Rating
Sun Distance 148571801 km (30.5%) Moon Distance 384547 km (56.0%)
Sun Diameter 0.537° Moon Diameter 0.518° - 0.526°
Perigee 20:07 on 22 Oct UT Apogee 02:46 on 6 Nov UT
Contact p1 05:49:29 on 30 Oct UT Contact p2
Contact u1 Contact u2
Max eclipse 07:45:26 on 30 Oct UT
Contact u3 Contact u4
Contact p3 Contact p4 09:41:15 on 30 Oct 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.