There's more to the North Star than meets the eye

70652986 — Mon, 26 Mar 2007 06:24:03 -0400

We tend to think of the North Star, Polaris, as a steady, solitary point of light that guided sailors in ages past. But there is more to the North Star than meets the eye - two faint stellar companions. The North Star is actually a triple star system. And while one companion can be seen easily through small telescopes, the other hugs Polaris so tightly that it has never been seen directly - until now.

By stretching the capabilities of NASA's Hubble Space Telescope to the limit, astronomers have photographed the close companion of Polaris for the first time. They presented their findings Jan. 9, 2006 in a press conference at the 207th meeting of the American Astronomical Society in Washington, D.C.

"The star we observed is so close to Polaris that we needed every available bit of Hubble's resolution to see it," said Smithsonian astronomer Nancy Evans (Harvard-Smithsonian Center for Astrophysics).

The companion proved to be less than two-tenths of an arcsecond from Polaris - an incredibly tiny angle equivalent to the apparent diameter of a quarter located 19 miles away. At the system's distance of 430 light-years, that translates into a physical separation of about 2 billion miles.

"The brightness difference between the two stars made it even more difficult to resolve them," stated Howard Bond of the Space Telescope Science Institute (STScI). Polaris is a supergiant more than two thousand times brighter than the Sun, while its companion is a main-sequence star. "With Hubble, we've pulled the North Star's companion out of the shadows and into the spotlight."

By watching the motion of the companion star, Evans and her colleagues expect to learn not only the stars' orbits but also their masses. Measuring the mass of a star is one of the most difficult tasks facing stellar astronomers.

Harvard continues legacy of Cepheid discoveries

70652986 — Mon, 26 Mar 2007 05:31:01 -0400

Cepheids are important to astronomers for their key role as extragalactic distance indicators. Cepheids are variable stars that regularly brighten and dim as they pulsate rhythmically. Their pulsation period is proportional to their intrinsic brightness - the longer the period, the brighter the star. A comparison of intrinsic to apparent brightness yields the distance to the Cepheid. Ninety years ago, Harvard astronomer Henrietta Leavitt spent years painstakingly examining thousands of sky photographs to search for and study variable stars, which led to the discovery of the period-luminosity relationship for Cepheid variables. Today, another astronomer at what has become the Harvard-Smithsonian Center for Astrophysics is continuing Leavitt's pioneering work on Cepheids. Smithsonian astrophysicist Nancy Remage Evans and colleagues used the unique capabilities of NASA's Hubble Space Telescope to study Cepheids in known binary systems. Their goal was to find the masses of the Cepheids - a fundamental stellar property. Instead, they announced in May 2003 at the 202nd meeting of the American Astronomical Society that they have uncovered a hidden, third star in the Cepheid system Y Carinae. More surprisingly, of the 14 total star systems with the most complete orbital information, seven were found to be likely triple systems, a remarkably high percentage.

all Nancy Remage Evans stories

There's more to the North Star than meets the eye

Harvard continues legacy of Cepheid discoveries