A total eclipse of the Moon occurs on Wednesday 28 March, 2192 UT, with maximum eclipse at 21:49 UT. The Moon will be plunged into darkness for 1 hour and 32 minutes, in a deep total eclipse which will see the Moon 41% 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. The partial eclipse will last for 3 hours and 49 minutes in total.
The penumbral eclipse lasts for 6 hours and 11 minutes.
The partial eclipse lasts for 3 hours and 49 minutes.
The total eclipse lasts for 1 hour and 32 minutes.
Maximum eclipse is at 21:49:21 UT.
During this eclipse the Moon will be just 2 days past apogee, making it very small.
At maximum eclipse it will be 0.500° in apparent
diameter, which is 5.8% smaller 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)
shows the visibility of the eclipse. (Click on it for the
full-sized version.)
Eclipse Season and Saros Series
This eclipse season contains 3 eclipses:
This is the 33rd eclipse in lunar Saros series 135.The surrounding eclipses in this Saros series are:
This Saros series, lunar Saros series 135,
is linked to solar Saros series 142. The
nearest partner eclipses in that series are:
Eclipse Parameters
| UT Date/time (max) | 21:49:21 on 28 Mar UT |
TDT Date/time (max) | 21:56:24 on 28 Mar TDT |
| Saros Series | 135 |
Number in Series | 33 |
| Penumbral Magnitiude | 2.4966 |
Central Magnitiude | 1.412 |
| Gamma | -0.2202 |
Path Width (km) | |
| Delta T | 7m03s |
Error | ± 4m23s (95%) |
| Penumbral Duration | 6h11m |
Partial Duration | 3h49m |
| Total Duration | 1h32m |
| |
| Partial Rating | |
Total Rating | |
| Sun Distance | 149242476 km (44.4%) |
Moon Distance | 404218 km (95.1%) |
| Sun Diameter | 0.534° |
Moon Diameter | 0.492° - 0.500° |
| Apogee | 13:14 on 26 Mar UT |
Perigee | 23:01 on 10 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 listingsGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. (NASA Goddard Space flight Center)
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 22:11:47 UTC.
