Max. width of band 58 km (36 mi)
Date 3 November 2013
Duration 100 sec (1 m 40 s)
(P1) Partial begin 10:04:34
|Other Instances Solar eclipse of April 8 - 2, Solar eclipse of July 2 - 20, Solar eclipse of August 2, Solar eclipse of March 9, Solar eclipse of March 20|
A total solar eclipse occurred on 3 November 2013. It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western atlantic ocean at sunrise as an annular eclipse, and the rest is a narrow total solar eclipse.
Totality was visible from the northern Atlantic Ocean (east of Florida) to Africa (Gabon (landfall), R. Congo, DR Congo, Uganda, South Sudan, Kenya, Ethiopia, Somalia), with maximum of 1 minute and 39 seconds visible from the Atlantic Ocean south of Ivory Coast and Ghana.
Places with partial darkening were the Eastern coast of North America, southern Greenland, Bermuda, the Caribbean islands, Costa Rica, Panama, Northern South America, almost all the African continent, the Iberian Peninsula, Italy, Greece, Malta, Southern Russia, the Caucasus, Turkey and the Middle East.
This solar eclipse happened simultaneously with the 2013 Abu Dhabi Grand Prix, and it was possible to observe a partial solar eclipse in Abu Dhabi before the sunset while the F1 race took place, as shown briefly during its broadcast.
Solar eclipses 2011–2014
Each member in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. Note: Partial solar eclipses on January 4, 2011, and July 1, 2011, occur in the previous semester series.
It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).