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|Los Angeles, California – January 11, 2006: UCLA astronomers can determine, for the first time, orbits of massive young stars located a few light months from the enormous black hole at the center of our Milky Way galaxy – stars that hold an imprint of how they were born. The origin of young stars at the center of our galaxy has puzzled astronomers, but the orbits may be the key to unlocking the mystery, UCLA|
astronomy graduate student Jessica Lu reported today at the annual meeting of the
American Astronomical Society
in Washington, D.C.
The astronomers use a new laser virtual star at the
W.M. Keck Observatory
The hostile environment around the supermassive black hole should make it extremely difficult for stars to form, but many young stars have been detected around the black hole, said Lu, who reported that she and a UCLA team are tracking a puzzling group of more than 30 massive young stars of uncertain origins.
"How were these stars formed in such an inhospitable region?" Lu asked. "My advisor, Andrea Ghez, calls this mystery 'the paradox of youth.' Using the Keck's Laser Guide Star adaptive optics system, we expect to resolve the paradox. We are able to measure how these young stars move across the sky with an unparalleled precision (only two kilometers per second) and determine, for the first time, the orbit of each of the young stars located a few light months from the black hole.
"Just as a fingerprint can be used to identify a person, the information encoded in the orbits of the young stars will tell us how and where they formed," said Lu, a member of a UCLA research team including her advisor, Ghez, a UCLA professor of physics and astronomy.
The orbits of stars within the central 1.0×1.0 arcseconds of our Galaxy.
In the background, the central portion of a diffraction-limited image taken in 2004 is displayed. While every star in this image has been seen to move over the past 9 years, estimates of orbital parameters are only possible for the seven stars that have had significant curvature detected. The annual average positions for these seven stars are plotted as colored dots, which have increasing color saturation with time. Also plotted are the best fitting simultaneous orbital solutions. These orbits provide the best evidence yet for a supermassive black hole, which has a mass of 3.7 million times the mass of the Sun.
Image: UCLA Galactic Center Group
Lu added that these are the closest stars to the supermassive black hole
that have not had their orbits distorted by their inhospitable environment.
"The orbits of these young stars suggest the stars were born far
from the black hole in a massive star cluster,
which migrated in," Lu reported.
"We can now track the stars so precisely as they move around
the black hole that we can determine each star's exact orbit."
Black holes are collapsed stars so dense that nothing can escape their gravitational pull, not even light. Black holes cannot be seen directly, but their influence on nearby stars is visible, and provides a signature, Ghez said.
The research was conducted using the 10-meter Keck II Telescope, which is the world's first 10-meter telescope with a laser on it. The Laser Guide Star allows astronomers to "generate an artificial bright star" exactly where they want it, which reveals the atmosphere's distortions. The Laser Guide Star
adaptive optics observations have allowed the
research team to retroactively increase the accuracy, by a factor of ~10,
and precision of over 10 years of speckle astrometry of the Galactic Center.
The supermassive black hole, with a mass more than 3 million times that of our sun, is in the constellation of Sagittarius. The Galactic Center is located due south in the summer sky.
J.R. Lu, A.M. Ghez, K.Y. Matthews, S.D. Hornstein, M. Morris, M. Rafelski, E.E. Becklin, D.J. Thompson, D. Le Mignant, P. Wizinowich, R.D. Campbell, J.C.Y. Chin, M.A. van Dam, S.K. Hartman, E.M. Johansson, R.E. Lafon, P.J. Stomski, D.M. Summers and A. Bouchez,
"Constraints on Orbits and Origins of Young Stars in the Central Parsec of the Galaxy,"
American Astronomical Society Meeting 207, #98.06; Bulletin of the American Astronomical Society 37, 1327 (2006)
Press Release: University of California Los Angeles
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