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How to steal a million stars? EUROPEAN SOUTHERN OBSERVATORY NEWS RELEASE Posted: February 11, 2006
Based on observations with European Southern Observatory's Very Large Telescope, a team of Italian astronomers reports that the stellar cluster Messier 12 must have lost to our Milky Way galaxy close to one million low-mass stars.
This photo shows the centre of the globular cluster Messier 12 as observed with the FORS-1 multi-mode instrument on ESO's Very Large Telescope. Credit: ESO
"In the solar neighbourhood and in most stellar clusters, the least
massive stars are the most common, and by far", said Guido De Marchi
(ESA), lead author of the study. "Our observations with ESO's VLT
show this is not the case for Messier 12".
The team, which also includes Luigi Pulone and Francesco Paresce
(INAF, Italy), measured the brightness and colours of more than
16,000 stars within the globular cluster Messier 12 with the
FORS1 multi-mode instrument attached to one of the Unit Telescopes of
ESO's VLT at Cerro Paranal (Chile). The astronomers could study stars
that are 40 million times fainter than what the unaided eye can see
(magnitude 25).
Messier 12 is one of about 200 globular clusters known in our
Galaxy. These are large groupings of 10,000 to more than a million
stars that were formed together in the youth of the Milky Way, about
12 to 13 billion years ago. Globular clusters are a key tool for
astronomers, because all the stars in a globular cluster share a
common history. They were all born together, at the same time and
place, and only differ from one another in their mass. By accurately
measuring the brightness of the stars, astronomers can determine
their relative sizes and stage of evolution precisely. Globular
clusters are thus very helpful for testing theories of how stars evolve.
An artist's impression of the orbit of the globular cluster Messier 12 in the Milky Way. Due to gravitational disruption, this cluster continuously loses stars, in particular light ones. This process is enhanced when it passes through the central plane in which most of the Galaxy's stars and nebulae are located. The cluster emerges in a less dense state after such a passage. The stars that are lost move on in orbits similar to that of the cluster and populate the halo of the Milky Way. Credit: ESO
Located at a distance of 23,000 light years in the constellation
Ophiuchus (The Serpent-holder), Messier 12 got its name by being the
12th entry in the catalogue of nebulous objects compiled in 1774 by
French astronomer and comet chaser Charles Messier. It is also known
to astronomers as NGC 6218 and contains about 200 000 stars, most of
them having a mass between 20 and 80 percent of the mass of the Sun.
"It is however clear that Messier 12 is surprisingly devoid of low-
mass stars", said De Marchi. "For each solar-like star, we would
expect roughly four times as many stars with half that mass. Our VLT
observations only show an equal number of stars of different masses."
Globular clusters move in extended elliptical orbits that
periodically take them through the densely populated regions of our
Galaxy, the plane, then high above and below, in the ‘halo'. When
venturing too close to the innermost and denser regions of the Milky
Way, the ‘bulge', a globular cluster can be perturbed, the smallest
stars being ripped away.
"We estimate that Messier 12 lost four times as many stars as it
still has", said Francesco Paresce. "That is, roughly one million
stars must have been ejected into the halo of our Milky Way".
The total remaining lifetime of Messier 12 is predicted to be about
4.5 billion years, i.e. about a third of its present age. This is
very short compared to the typical expected globular cluster's
lifetime, which is about 30 billion years.
The same team of astronomers had found in 1999, another example of a
globular cluster that lost a large fraction of its original content.
The scientists hope to discover and study many more clusters like
these, since catching clusters while being disrupted should clarify
the dynamics of the process that shaped the halo of our home galaxy,
the Milky Way.