http://www.nytimes.com/2004/06/01/science/space/01star.html?ex=1086667200&en=2f369908cade1abe&ei=5062&partner=GOOGLEAstronomers have known for some time that Polaris, the North Star, sitting almost directly over the North Pole, is a Cepheid variable, a type of star that is caught in a cycle of bloating and collapsing because it has exhausted its hydrogen fuel.
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Yesterday at a meeting of the American Astronomical Society in Denver, astronomers reported that Polaris is even unsteadier than they had thought.
Even Polaris's average brightness has not remained the same, reported Dr. Edward F. Guinan of Villanova University. Measurements over the past half century show it has brightened 10 percent. When he and Scott Engle, an undergraduate, checked older records, they found more surprises.
In the 1800's, Polaris appeared to be 20 percent less bright. In the 1500's, the astronomer Tycho Brahe recorded an even dimmer value. Ptolemy of Alexandria in his star catalog of A.D. 140 listed Polaris as a third magnitude star. Magnitude is a scale devised by the Greek astronomer Hipparchus around 120 B.C. ranking stars from bright (1) to dim (6), a system still in use today.
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Meanwhile, Dr. David G. Turner of St. Mary's University in Halifax, Nova Scotia, said Polaris was much closer than had been thought. His research indicates that Polaris is 310 light-years away. The current accepted distance to Polaris is 430 light-years.
If Dr. Turner is correct, his findings offer an explanation for why Polaris appears as bright as it does. Until now, astronomers have suggested that the star possesses unusual internal pulsations that pump out additional light, but if it is nearer, that elaborate theory would be unnecessary.
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