Fast-track planet. (Astronomy).Astronomers Famous astronomers and astrophysicists include: Directory: A B C D E F G H I J K L M N O P Q R S T U V W X Y Z A
Both close-in planets were revealed by a periodic dip in starlight star·light n. The light from the stars. starlight Noun the light that comes from the stars Noun 1. , suggesting that a small body is regularly passing in front of a star, as seen from Earth. This planet-hunting technique is called the transit method. Klaus Werner of the Institute for Astronomy The Institute for Astronomy (IfA) is a research unit within the University of Hawaii system, led by Dr. Rolf-Peter Kudritzki as Director. IfA main headquarters are located at 2680 Woodlawn Drive in Honolulu, Hawaii; additional facilities are located at Kula, Maui and Hilo on the and Astrophysics astrophysics, application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. in Tubingen, Germany, and his colleagues homed in on a star whose brightness drops by 2 percent about every 28.5 hours. The researchers then examined the spectra of this sunlike star, known as OGLE-TR-3, and found a wobble wobble /wob·ble/ (wob´'l) to move unsteadily or unsurely back and forth or from side to side. See under hypothesis. wob·ble n. 1. in its motion, indicating the tug of the unseen planet. The transit method, which requires a special alignment among the planet, the star, and Earth, provides enough information to yield the planet's actual mass, but the wobble method doesn't. In an upcoming Astronomy Astrophysics, the team reports that the planet weighs half as much as Jupiter but is only one-fifth as dense. The low density suggests the extrasolar planet extrasolar planet also called exoplanet Planet that orbits a star other than the Sun. The existence of extrasolar planets, many light-years from Earth, was confirmed in 1992 with the detection of three bodies circling a pulsar. has ballooned in response to the heat from its star. Werner notes that a planet can't get closer to a sunlike star than half the distance the new planet is from OGLE-TR-3. At greater proximity, a planet would be torn apart by the star's gravity. |
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