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March 29 , 2001

Galileo Discovers Variable Star


Edwin L. Aguirre Sky and Telescope

The Galileo spacecraft is making discoveries light-years away from Jupiter. Courtesy NASA/JPL/Caltech.

Last June the Galileo spacecraft orbiting Jupiter temporarily lost sight of one of the reference stars it uses to maintain proper orientation. Flight engineers suspected that the probe's star scanner had broken down. "I spent about a week working on it," says Paul Fieseler (Jet Propulsion Laboratory), "and concluded that the star scanner wasn't broken, but perhaps the star was." After a thorough check, Fieseler and his colleagues determined that the star itself had briefly faded from view.

The star in question is 2nd-magnitude Delta Velorum, part of the False Cross, which consists of stars in Vela and Carina. Known to be a quadruple-star system, it is one of 150 bright targets tracked by Galileo to keep its low-gain antenna pointed at Earth. Follow-up observations by amateur variable-star observer Sebastian Otero (Buenos Aires, Argentina) and professional astronomer Christopher Lloyd (Rutherford Appleton Laboratory) revealed that Delta Velorum is a hitherto unknown eclipsing binary. Its brightest member is actually two stars of similar brightness orbiting each other. Every 45 days one mutually eclipses the other, causing Delta's total brightness to dip from magnitude 1.96 to 2.3 for a few hours. Galileo apparently lost track of the star during one of its periodic dimmings.

 

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