A hybrid eclipse of the Sun occurred on Sunday 3 November, 2013 UT, lasting from 10:04–15:28 UT. The Sun was darkened for 1 minute and 40 seconds by a dramatic hybrid eclipse covering a narrow path at most 58 km wide. This was a sight worth seeing, and was visible across the Atlantic starting east of Florida, and across central Africa. The partial eclipse was visible in northern South America, the extreme eastern US, and most of 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: 10:04:34 UT
Central eclipse began: 11:05:17 UT
Maximum eclipse: 12:46:28 UT
Central eclipse ended: 14:27:43 UT
Partial eclipse ended: 15:28:21 UT

During this eclipse the Sun was 0.537° in apparent diameter, 0.8% larger than average. The Moon was just 3 days before perigee, making it relatively large. At the start and end of the eclipse, the Moon was 0.537°, which is smaller than the Sun; hence the eclipse was annular at that point. However, at maximum eclipse the Moon was 0.546° in apparent diameter, which is 2.8% larger than average, large enough to cover the Sun; and so a total eclipse was seen at that point. Thus this was a hybrid eclipse. The statistics page has information on the ranges of the sizes of the Sun and Moon.

The central eclipse begain in the Atlantic south of Bermuda, soon becoming total. It then crossed the ocean and passed just south of Sao Tome and Principe before making landfall in Gabon. It then crossed Congo, DR Congo, Uganda, Kenya, and Ethiopia, finishing as an extremely short total eclipse in Somalia.

Interactive Map

This map shows the visibility of the eclipse. The area shaded blue saw a total eclipse, and the areas shaded red saw an annular eclipse; however, near the edges of each 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.

Overview Map

This map sourced from NASA's Eclipse Web Site shows the visibility of the hybrid 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 2 eclipses:

This was the 23rd eclipse in solar Saros series 143.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 12:46:28 on 3 Nov UT TDT Date/time (max) 12:47:36 on 3 Nov TDT
Saros Series 143 Number in Series 22
Penumbral Magnitiude Central Magnitiude 1.0159
Gamma 0.3272 Path Width (km) 58
Delta T 1m08s Error ± 0m02s (95%)
Penumbral Duration Partial Duration
Total Duration 1m40s
Partial Rating Total Rating
Sun Distance 148393600 km (26.9%) Moon Distance 370507 km (28.0%)
Sun Diameter 0.537° Moon Diameter 0.537° - 0.546°
Apogee 14:25 on 25 Oct UT Perigee 09:28 on 6 Nov UT
Contact p1 10:04:34 on 3 Nov UT Contact p2
Contact u1 11:05:17 on 3 Nov UT Contact u2 11:05:21 on 3 Nov UT
Max eclipse 12:46:28 on 3 Nov UT
Contact u3 14:27:42 on 3 Nov UT Contact u4 14:27:43 on 3 Nov UT
Contact p3 Contact p4 15:28:21 on 3 Nov 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 listings 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.

Data last updated: 2015-06-21 22:11:46 UTC.