An annular eclipse of the Sun occurs on Tuesday 20 October, 2218 UT, with maximum eclipse at 11:33 UT. The Sun will be 94% covered in a moderate annular eclipse, lasting 5 minutes and 41 seconds and covering a very broad path, 280 km wide at maximum.
The annular eclipse lasts for 5 minutes and 41 seconds. Maximum eclipse is at 11:33:48 UT.
During this eclipse the Sun will be 0.535° in apparent diameter, 0.3% larger than average. The Moon will be just 4 days past apogee, making it fairly small. At maximum eclipse it will be 0.504° in apparent diameter, which is 5.2% smaller than average; this is not large enough to cover the Sun, which is why this is an annular eclipse. 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 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 annular solar eclipse. It also shows the broader area in which a partial eclipse will be seen. (Click on it for the
full-sized version.)
This eclipse season contains 2 eclipses:
This is the 47th eclipse in solar Saros series 137.The surrounding eclipses in this Saros series are:
This Saros series, solar Saros series 137, is linked to lunar Saros series 130. The nearest partner eclipses in that series are:
UT Date/time (max) | 11:33:48 on 20 Oct UT | TDT Date/time (max) | 11:41:56 on 20 Oct TDT |
---|---|---|---|
Saros Series | 137 | Number in Series | 47 |
Penumbral Magnitiude | Central Magnitiude | 0.9416 | |
Gamma | -0.6411 | Path Width (km) | 280 |
Delta T | 8m08s | Error | ± 5m22s (95%) |
Penumbral Duration | Partial Duration | ||
Total Duration | 5m41s | ||
Partial Rating | Total Rating | ||
Sun Distance | 149132761 km (42.1%) | Moon Distance | 400102 km (86.9%) |
Sun Diameter | 0.535° | Moon Diameter | 0.498° - 0.504° |
Apogee | 15:10 on 16 Oct UT | Perigee | 12:34 on 1 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, and the Moon data page displays detailed information on the Moon's key dates.
Data last updated: 2015-06-21 22:11:47 UTC.