Timezone / Date

You have not selected a timezone for eclipse timings, so all times are shown in UT (essentially GMT).

Accuracy

Due to the erratic rotation of the Earth, the time and location of the eclipse cannot be forecast perfectly. This eclipse's time is estimated to be accurate ± 7m10s (with 95% confidence). This equates to an error in longitude of ± 1.79 degrees, or around ± 197 km (122 miles) at the latitude of greatest eclipse.

An annular eclipse of the Sun occurs on Tuesday 17 June, 2262 UT, with maximum eclipse at 14:09 UT. A large annular eclipse will cover 98% of the Sun, creating a dramatic spectacle for observers in a path up to 92 km wide; it will last 3 minutes and 8 seconds at the point of maximum eclipse.

The annular eclipse lasts for 3 minutes and 8 seconds. Maximum eclipse is at 14:09:10 UT.

During this eclipse the Sun will be 0.525° in apparent diameter, 1.5% smaller than average. The Moon will be 11 days after perigee and 5 days before apogee. At maximum eclipse it will be 0.512° in apparent diameter, which is 3.6% 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.

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 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.)

Eclipse Season and Saros Series

This eclipse season contains 3 eclipses:

This is the 37th eclipse in solar Saros series 141.The surrounding eclipses in this Saros series are:

This Saros series, solar Saros series 141, is linked to lunar Saros series 134. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 14:09:10 on 17 Jun UT TDT Date/time (max) 14:19:15 on 17 Jun TDT
Saros Series 141 Number in Series 37
Penumbral Magnitiude Central Magnitiude 0.975
Gamma -0.2377 Path Width (km) 92
Delta T 10m05s Error ± 7m10s (95%)
Penumbral Duration Partial Duration
Total Duration 3m08s
Partial Rating Total Rating
Sun Distance 151912414 km (99.6%) Moon Distance 394959 km (76.7%)
Sun Diameter 0.525° Moon Diameter 0.504° - 0.512°
Perigee 18:59 on 6 Jun UT Apogee 14:06 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.