A total eclipse of the Moon occurs on Monday 10 November, 2087 UT, with maximum eclipse at 12:02 UT. The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see the Moon 50% 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 27 minutes in total.
The penumbral eclipse lasts for 5 hours and 16 minutes.
The partial eclipse lasts for 3 hours and 27 minutes.
The total eclipse lasts for 1 hour and 29 minutes.
Maximum eclipse is at 12:02:39 UT.
During this eclipse the Moon will be at perigee, making it extremely large.
At maximum eclipse it will be 0.568° in apparent
diameter, which is 6.9% 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)
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 30th eclipse in lunar Saros series 137.The surrounding eclipses in this Saros series are:
This Saros series, lunar Saros series 137,
is linked to solar Saros series 144. The
nearest partner eclipses in that series are:
Eclipse Parameters
| UT Date/time (max) | 12:02:39 on 10 Nov UT |
TDT Date/time (max) | 12:05:33 on 10 Nov TDT |
| Saros Series | 137 |
Number in Series | 30 |
| Penumbral Magnitiude | 2.4654 |
Central Magnitiude | 1.5006 |
| Gamma | -0.2043 |
Path Width (km) | |
| Delta T | 2m54s |
Error | ± 1m15s (95%) |
| Penumbral Duration | 5h16m |
Partial Duration | 3h27m |
| Total Duration | 1h29m |
| |
| Partial Rating | |
Total Rating | |
| Sun Distance | 148172950 km (22.3%) |
Moon Distance | 356999 km (1.2%) |
| Sun Diameter | 0.538° |
Moon Diameter | 0.558° - 0.568° |
| Apogee | 19:19 on 28 Oct UT |
Perigee | 19:56 on 10 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)
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.
