An annular eclipse of the Sun occurs on Monday 9 March, 2798 UT, with maximum eclipse at 17:47 UT. A small annular eclipse will cover only 92% of the Sun in a very broad path, 291 km wide at maximum, and will last 9 minutes and 57 seconds.

The annular eclipse lasts for 9 minutes and 57 seconds. Maximum eclipse is at 17:47:21 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 3 eclipses:

This is the 31st eclipse in solar Saros series 162.The surrounding eclipses in this Saros series are:

This Saros series, solar Saros series 162, is linked to lunar Saros series 155. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 17:47:21 on 9 Mar UT TDT Date/time (max) 18:37:54 on 9 Mar TDT
Saros Series 162 Number in Series 31
Penumbral Magnitiude Central Magnitiude 0.9238
Gamma -0.158 Path Width (km) 291
Delta T 50m33s Error ± 42m31s (95%)
Penumbral Duration Partial Duration
Total Duration 9m57s
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 22:11:48 UTC.