Images reveal possible origin of young stars.Newborn stars have no business being anywhere near the monster black hole that lies at the center of the Milky Way Milky Way, the galaxy of which the sun and solar system are a part, seen as a broad band of light arching across the night sky from horizon to horizon; if not blocked by the horizon, it would be seen as a circle around the entire sky. . The tidal forces that the black hole exerts on the cold, low-density clouds of gas and dust that give rise to stars are so enormous that they would rip the cloud to shreds long before stars could emerge. Nonetheless, the galactic center contains hundreds of massive, newborn stars, a puzzle that Andrea Ghez Andrea Mia Ghez is an astronomer and professor in the Department of Physics and Astronomy at UCLA. She received a BS in physics from the Massachusetts Institute of Technology in 1987 and her Ph.D. at the California Institute of Technology in 1991. of the University of California, Los Angeles UCLA comprises the College of Letters and Science (the primary undergraduate college), seven professional schools, and five professional Health Science schools. Since 2001, UCLA has enrolled over 33,000 total students, and that number is steadily rising. calls the paradox of youth (SN: 6/21/03, p. 394). Ghez and her colleagues say that they have now solved the puzzle. Astronomers have had two leading theories to explain the young stars' existence. According to according to prep. 1. As stated or indicated by; on the authority of: according to historians. 2. In keeping with: according to instructions. 3. one model, the stars didn't form in their current locations but instead were ferried in as part of a massive star cluster star cluster, a group of stars near each other in space and resembling each other in certain characteristics that suggest a common origin for the group. Stars in the same cluster move at the same rate and in the same direction. with enough gravity to stick together even as it entered the black hole's arena. In this scenario, the star cluster broke apart soon after its arrival, sprinkling the region with young, massive stars in either circular or elliptical el·lip·tic or el·lip·ti·cal adj. 1. Of, relating to, or having the shape of an ellipse. 2. Containing or characterized by ellipsis. 3. a. orbits around the galactic center. In another model, the young stars formed where they now reside but arose within a flattened disk of gas and dust that managed to stay intact despite its proximity to the black hole. In this case, all the stars should have the circular orbits they would have had when born. The stars would lie too far apart for their mutual gravity to have altered their orbits from circular to elliptical. Ghez and her colleagues recorded a series of unusually sharp images of stars at the galactic center taken by a laser system on one of the world's largest visible-light telescope, the Keck II telescopes atop Hawaii's Mauna Kea Mauna Kea (mou`nə kā`ə), dormant volcano, 13,796 ft (4,205 m) high, in the south central part of the island of Hawaii. It is the loftiest peak in the Hawaiian Islands and the highest island mountain in the world, rising c. . Beamed into space, the laser light acts as a virtual star, enabling a rapidly adjustable mirror on the telescope to continuously change shape to compensate for the blurring caused by Earth's turbulent atmosphere. The team tracked the motion of more than 30 slow-moving, young stars that lie a few light-months from the galaxy's core. That's just far enough away from the center that the black hole couldn't have distorted the shapes of the star's original orbits. The images reveal that most of the 30 massive stars have elliptical orbits, indicating that, as migration theory suggests, these stars did indeed travel to the galactic center after forming elsewhere, says UCLA UCLA University of California at Los Angeles UCLA University Center for Learning Assistance (Illinois State University) UCLA University of Carrollton, TX and Lower Addison, TX astronomer Jessica Lu, a member of Ghez' team.--R.C. |
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