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ALGOL |
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AlgolEclipsing binary, a pair of orbiting stars in the constellation Perseus, the fainter one of which eclipses the brighter one every 69 hours, causing the apparent brightness of the pair to drop by two-thirds. The brightness changes were first explained in 1782 by English amateur astronomer John Goodricke. He pointed out that the changes between magnitudes 2.2 and 3.5 repeated themselves exactly after an interval of 2.867 days and supposed this to be due to two stars orbiting round and eclipsing each other.
ALGOL
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Mercedes Richards and her colleagues from Pennsylvania State University in State College recorded radio waves from flares spewing from two nearby star systems, Beta Persei and V711 Tauri. But the technique was used so successfully with the rings of Saturn that it is being tried twice at Uranus -- first for about four hours, when the star Sigma Sagittarii (Nunki) will be occulted by the two outermost rings, and later by the star Beta Persei (Algol), whose track will encompass all nine. |
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