An annular eclipse of the Sun occurs on Monday 31 May, 2421 UT, with maximum eclipse at 18:14 UT. A large annular eclipse will cover 98% of the Sun, creating a dramatic spectacle for observers in a path up to 95 km wide; it will last 2 minutes and 32 seconds at the point of maximum eclipse.

The annular eclipse lasts for 2 minutes and 32 seconds. Maximum eclipse is at 18:14:04 UT.

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 2 eclipses:

This is the 39th eclipse in solar Saros series 144.The surrounding eclipses in this Saros series are:

This Saros series, solar Saros series 144, is linked to lunar Saros series 137. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 18:14:04 on 31 May UT TDT Date/time (max) 18:32:59 on 31 May TDT
Saros Series 144 Number in Series 39
Penumbral Magnitiude Central Magnitiude 0.975
Gamma 0.3451 Path Width (km) 95
Delta T 18m55s Error ± 15m12s (95%)
Penumbral Duration Partial Duration
Total Duration 2m32s
Partial Rating Total Rating

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.

Data last updated: 2015-06-21 22:11:47 UTC.