A total eclipse of the Moon occurs on Wednesday 9 June, 2123 UT, with maximum eclipse at 05:02 UT. A dramatic total eclipse lasting 1 hour and 46 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 56 minutes in total.
The penumbral eclipse lasts for 6 hours and 14 minutes. The partial eclipse lasts for 3 hours and 56 minutes. The total eclipse lasts for 1 hour and 46 minutes. Maximum eclipse is at 05:02:09 UT.
During this eclipse the Moon will be just a day past apogee, making it very small. At maximum eclipse it will be 0.498° in apparent diameter, which is 6.1% 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.
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.
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.)
This eclipse season contains 3 eclipses:
This is the 36th eclipse in lunar Saros series 132.The surrounding eclipses in this Saros series are:
This Saros series, lunar Saros series 132, is linked to solar Saros series 139. The nearest partner eclipses in that series are:
UT Date/time (max) | 05:02:09 on 9 Jun UT | TDT Date/time (max) | 05:06:28 on 9 Jun TDT |
---|---|---|---|
Saros Series | 132 | Number in Series | 36 |
Penumbral Magnitiude | 2.8189 | Central Magnitiude | 1.7487 |
Gamma | 0.0406 | Path Width (km) | |
Delta T | 4m19s | Error | ± 2m10s (95%) |
Penumbral Duration | 6h14m | Partial Duration | 3h56m |
Total Duration | 1h46m | ||
Partial Rating | Total Rating | ||
Sun Distance | 151806364 km (97.4%) | Moon Distance | 405675 km (98.0%) |
Sun Diameter | 0.525° | Moon Diameter | 0.491° - 0.498° |
Apogee | 23:20 on 7 Jun UT | Perigee | 19:17 on 22 Jun 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 22:11:47 UTC.