An annular eclipse of the Sun occurred on Friday 22 September, 2006 UT, lasting from 08:39–14:40 UT. A small annular eclipse covered only 94% of the Sun in a very broad path, 261 km wide at maximum, and lasted 7 minutes and 9 seconds. It was visible from central America east across the Atlantic, finishing south of Africa. The partial eclipse was visible in eastern South America and south and west Africa.
The timings of the phases of the overall eclipse worldwide are as follows. In any particular place it would have been seen for a significantly shorter duration as the shadow moved across the Earth:
Partial eclipse began: | 08:39:57 UT |
Annular eclipse began: | 09:48:32 UT |
Maximum eclipse: | 11:40:11 UT |
Annular eclipse ended: | 13:31:34 UT |
Partial eclipse ended: | 14:40:14 UT |
During this eclipse the Sun was 0.531° in apparent diameter, 0.3% smaller than average. The Moon was at apogee, making it very small. At maximum eclipse it was 0.497° in apparent diameter, which is 6.5% smaller than average; this was not large enough to cover the Sun, which is why this was 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.
The annular eclipse started in Guyana, then crossed Suriname and French Guiana, clipping a croner of Brazil, before heading off into the Atlantic. It crossed south of Africa, including the Prince Edward Islands, and finished just short of Heard Island.
This map shows the visibility of the eclipse. The shaded area saw the annular solar eclipse; however, near the edges of this area, the eclipse was very short. The bold line shows the centre of the path, where the eclipse lasted longest.
Use the zoom controls to zoom in and out; hover your mouse over any point on the centreline to see the time and duration of the eclipse at that point. You can pan and zoom the map to see detail for any part of the eclipse path.
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.)
This eclipse season contains 2 eclipses:
This was the 16th 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:
UT Date/time (max) | 11:40:11 on 22 Sep UT | TDT Date/time (max) | 11:41:16 on 22 Sep TDT |
---|---|---|---|
Saros Series | 144 | Number in Series | 16 |
Penumbral Magnitiude | Central Magnitiude | 0.9352 | |
Gamma | -0.4062 | Path Width (km) | 261 |
Delta T | 1m05s | Error | ± 0m00s (95%) |
Penumbral Duration | Partial Duration | ||
Total Duration | 7m09s | ||
Partial Rating | Total Rating | ||
Sun Distance | 150157113 km (63.3%) | Moon Distance | 406475 km (99.6%) |
Sun Diameter | 0.531° | Moon Diameter | 0.490° - 0.497° |
Apogee | 05:22 on 22 Sep UT | Perigee | 14:08 on 6 Oct UT |
Contact p1 | 08:39:57 on 22 Sep UT | Contact p2 | |
Contact u1 | 09:48:32 on 22 Sep UT | Contact u2 | 09:54:34 on 22 Sep UT |
Max eclipse | 11:40:11 on 22 Sep UT | ||
Contact u3 | 13:25:32 on 22 Sep UT | Contact u4 | 13:31:34 on 22 Sep UT |
Contact p3 | Contact p4 | 14:40:14 on 22 Sep 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 22:11:46 UTC.