A total eclipse of the Moon occurs on Sunday 18 November, 2040 UT, lasting from 16:06–22:00 UT. The Moon will be plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which will see the Moon 40% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour for observers from Europe, Asia, and Australia. The partial eclipse will last for 3 hours and 40 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: 16:06:31 UT
Partial eclipse begins: 17:13:01 UT
Total eclipse begins: 18:19:19 UT
Maximum eclipse: 19:03:15 UT
Total eclipse ends: 19:47:10 UT
Partial eclipse ends: 20:53:27 UT
Penumbral eclipse ends: 22:00:06 UT

During this eclipse the Moon will be 9 days after perigee and 6 days before apogee. At maximum eclipse it will be 0.519° in apparent diameter, which is 2.2% 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 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.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This is the 21st eclipse in lunar Saros series 136.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 19:03:15 on 18 Nov UT TDT Date/time (max) 19:04:40 on 18 Nov TDT
Saros Series 136 Number in Series 20
Penumbral Magnitiude 2.4525 Central Magnitiude 1.3974
Gamma 0.2361 Path Width (km)
Delta T 1m25s Error ± 0m20s (95%)
Penumbral Duration 5h54m Partial Duration 3h40m
Total Duration 1h28m
Partial Rating Total Rating
Sun Distance 147851971 km (15.7%) Moon Distance 389554 km (65.9%)
Sun Diameter 0.539° Moon Diameter 0.511° - 0.519°
Perigee 06:18 on 9 Nov UT Apogee 19:13 on 24 Nov UT
Contact p1 16:06:31 on 18 Nov UT Contact p2
Contact u1 17:13:01 on 18 Nov UT Contact u2 18:19:19 on 18 Nov UT
Max eclipse 19:03:15 on 18 Nov UT
Contact u3 19:47:10 on 18 Nov UT Contact u4 20:53:27 on 18 Nov UT
Contact p3 Contact p4 22:00:06 on 18 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 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.

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.