An annular eclipse of the Sun occurred on 3 September, 1967 BC UT Old Style, with maximum eclipse at 03:54 UT. A small annular eclipse covered only 94% of the Sun in a broad path up to 227 km wide, and lasted 7 minutes and 41 seconds.

The annular eclipse lasted for 7 minutes and 41 seconds. Maximum eclipse was at 03:54:45 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 was seen. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 3 eclipses:

This eclipse belongs to solar Saros series 13.The surrounding eclipses in this Saros series are:

This Saros series, solar Saros series 13, is linked to lunar Saros series 6. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 03:54:45 on 3 Sep UT TDT Date/time (max) 16:35:18 on 3 Sep TDT
Saros Series 13 Number in Series
Penumbral Magnitiude Central Magnitiude 0.939
Gamma 0.0794 Path Width (km) 227
Delta T 12h41m Error ± 1h57m (95%)
Penumbral Duration Partial Duration
Total Duration 7m41s
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 22:11:38 UTC.