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Astronomers have used NASA's Hubble Space Telescope to peer into the center of
a dense swarm of stars called Omega Centauri. Located some 17,000 light-years
from Earth, Omega Centauri is a massive globular star cluster, containing
several million stars swirling in locked orbits around a common center of
gravity. The stars are packed so densely in the cluster's core that it is
difficult for ground-based telescopes to make out individual stars. Hubble's
high resolution is able to pick up where ground-based telescopes leave off,
capturing distinct points of light from stars at the very center of the
Omega Centauri is so large in our sky that only a small part of it fits
within the field of view of the Wide Field and Planetary Camera 2 (WFPC2)
on the Hubble Space Telescope. Yet even this tiny patch contains some 50,000
stars, all packed into a region only about 13 light-years wide. For
comparison, a similarly sized region centered on the Sun would contain
about a half dozen stars.
The vast majority of stars in this Hubble image are faint, yellow-white dwarf
stars similar to our Sun. The handful of bright yellow-orange stars are red
giants that have begun to exhaust their nuclear fuel and have expanded to
diameters about a hundred times that of the Sun. A number of faint blue stars
are also visible in the image. These are in a brief phase of evolution between
the dwarf stage and the red-giant stage, during which the surface temperature
is high. The stars in Omega Centauri are all very old, about 12 billion years.
Stars with a mass as high as that of our Sun have already completed their
evolution and have faded away as white dwarfs, too faint to be seen even in
the Hubble image.
The stars in the core of Omega Centauri are so densely packed that occasionally
one of them will actually collide with another one. Even in the dense center of
Omega Centauri, stellar collisions will be infrequent. But the cluster is so
old that many thousands of collisions have occurred.
What happens when stars collide? These Hubble images were taken to help answer
that question. When stars collide head-on, they probably just merge together
and make one bigger star. But if the collision is a near miss, they may go
into orbit around each other, forming a close binary star system.
Searching for a needle in a haystack, scientists have found two binary star
systems in these Hubble images that may have had such an origin. Both of them
are close pairs in which once component is a white dwarf that pulls gas off of
its companion. When the gas falls onto the surface of the white dwarf, it is
heated to the point that it emits ultraviolet light. These unusual emissions
enabled scientists to pinpoint these two faint stars among the myriad of other
faint stars in the cluster.
Omega Centauri is the most luminous and massive globular star cluster in the
Milky Way. It is one of the few globular clusters that can be seen with the
unaided eye. Named by Johann Bayer in 1603 as the 24th brightest object in the
constellation Centaurus, it resembles a small cloud in the southern sky and
might easily be mistaken for a comet.
This Hubble WFPC2 image was taken on June 11, 1997 in ultraviolet, red, and
H-alpha filters. The science team, led by Dr. Adrienne Cool of San Francisco
State University includes Jennifer Carson, a former SFSU student who is now
at UCLA, Charles Bailyn at Yale and Jonathan Grindlay at Harvard. These data
are currently being used by Jeff Carlin and Daryl Haggard, two SFSU students,
to look for optical counterparts of X-ray sources recently discovered with
the Chandra Observatory. This image was produced by the Hubble Heritage Team
October 4, 2001
Credits: NASA and The Hubble Heritage Team (STScI/AURA)