A total eclipse of the Moon occurs on Thursday 14 April, 2033 UT, lasting from 16:11–22:13 UT. A shallow total eclipse will see the Moon in relative darkness for 49 minutes and 12 seconds. The Moon will be 9% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers from Europe, Africa, most of Asia, and Australia. The partial eclipse will last for 3 hours and 35 minutes in total.

The timings of the phases of the eclipse are as follows. You will be able to see each phase of the eclipse if the Moon is up at the corresponding time as seen from your location; however the penumbral phase will be very difficult to see in practice, so you may want to start watching at the partial phase:

Penumbral eclipse begins: 16:11:54 UT
Partial eclipse begins: 17:25:03 UT
Total eclipse begins: 18:47:56 UT
Maximum eclipse: 19:12:32 UT
Total eclipse ends: 19:37:09 UT
Partial eclipse ends: 21:00:02 UT
Penumbral eclipse ends: 22:13:05 UT

During this eclipse the Moon will be just 2 days past apogee, making it very small. At maximum eclipse it will be 0.501° in apparent diameter, which is 5.6% 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 various stages. The bright area in the middle will see the whole eclipse; the coloured bands to the right will see the start of the eclipse, and those on the left will see the end. 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. Hover your mouse over the tags to see what will be visible from each area on the map. 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 31st eclipse in lunar Saros series 132.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 19:12:31 on 14 Apr UT TDT Date/time (max) 19:13:51 on 14 Apr TDT
Saros Series 132 Number in Series 30
Penumbral Magnitiude 2.1711 Central Magnitiude 1.0944
Gamma 0.3954 Path Width (km)
Delta T 1m20s Error ± 0m14s (95%)
Penumbral Duration 6h01m Partial Duration 3h35m
Total Duration 49m12s
Partial Rating Total Rating
Sun Distance 150057736 km (61.3%) Moon Distance 403453 km (93.5%)
Sun Diameter 0.531° Moon Diameter 0.493° - 0.501°
Apogee 02:27 on 12 Apr UT Perigee 14:44 on 27 Apr UT
Contact p1 16:11:54 on 14 Apr UT Contact p2
Contact u1 17:25:03 on 14 Apr UT Contact u2 18:47:56 on 14 Apr UT
Max eclipse 19:12:32 on 14 Apr UT
Contact u3 19:37:09 on 14 Apr UT Contact u4 21:00:02 on 14 Apr UT
Contact p3 Contact p4 22:13:05 on 14 Apr 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.