A penumbral eclipse of the Moon occurs on Saturday 20 February, 2027 UT, lasting from 21:12 on 20 Feb–01:13 on 21 Feb UT. At maximum eclipse, 93% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 4 hours and 1 minute overall, and will be visible from the eastern Americas, Europe, Africa, and most of Asia.

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: 21:12:20 UT
Maximum eclipse: 23:12:50 UT
Penumbral eclipse ends: 01:13:19 on 21 Feb UT

During this eclipse the Moon will be just a day past perigee, making it very large. At maximum eclipse it will be 0.558° in apparent diameter, which is 5.0% larger than average. The statistics page has information on the ranges of the sizes of the Sun and Moon, and the Moon data page displays detailed information on the Moon's key dates.

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.

The interactive map is currently not available.

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 18th eclipse in lunar Saros series 143.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 143, is linked to solar Saros series 150. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 23:12:50 on 20 Feb UT TDT Date/time (max) 23:14:06 on 20 Feb TDT
Saros Series 143 Number in Series 18
Penumbral Magnitiude 0.9266 Central Magnitiude -0.0569
Gamma -1.048 Path Width (km)
Delta T 1m16s Error ± 0m10s (95%)
Penumbral Duration 4h01m Partial Duration
Total Duration
Partial Rating Total Rating
Sun Distance 147920278 km (17.1%) Moon Distance 363285 km (13.7%)
Sun Diameter 0.539° Moon Diameter 0.548° - 0.558°
Perigee 07:31 on 19 Feb UT Apogee 05:42 on 3 Mar UT
Contact p1 21:12:20 on 20 Feb UT Contact p2
Contact u1 Contact u2
Max eclipse 23:12:50 on 20 Feb UT
Contact u3 Contact u4
Contact p3 Contact p4 01:13:19 on 21 Feb 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, and the Moon data page displays detailed information on the Moon's key dates.

Data last updated: 2015-06-21 22:11:46 UTC.