By Paul Rincon
Science reporter, BBC News, Seattle
Andromeda, imaged here in the infra-red by Nasa's Spitzer telescope
Astronomers have found an enormous halo of stars around the Andromeda galaxy.
The discovery suggests the nearby spiral galaxy, also
known as M31, is as much as five times bigger than astronomers had
In fact, Andromeda's "suburbs" are so vast that they nearly overlap with those of our own Milky Way galaxy.
University of California researchers presented their
findings at a meeting of the American Astronomical Society (AAS) taking
place in Seattle, US.
Andromeda is a spiral galaxy similar to the Milky Way.
About 2.5 million light-years away from Earth, it is the largest galaxy
in the "local group", which also includes the Milky Way and about 30
Spiral galaxies consist of a bright central bulge with a
dense concentration of stars, surrounded by a flat rotating disc of
Extending out from the disc is a spherical halo of sparsely distributed stars.
Theories of galaxy formation predict that the halo of a large galaxy is
the first component to form. The disc and central bulge develop some
Studying the Milky Way's halo is difficult because Earth
is buried within the galaxy; astronomers do not have an external
vantage point from which to view the whole galaxy.
The halos of distant galaxies are nearly impossible to resolve, because astronomers cannot see individual stars.
Andromeda is at the perfect distance: it is just far
enough for astronomers to see the whole galaxy, and just close enough
for them to observe individual stars.
Smooth and even
A team from the University of California at Santa Cruz
(UCSC) detected a sparse population of red giant stars - bright,
bloated stars in a late stage of stellar evolution.
These appeared to be smoothly distributed around Andromeda out to a distance of 500,000 light-years from the galaxy's centre.
"I am absolutely astounded by how big this halo is,"
said UCSC Professor Puragra Guhathakurta, one of the researchers in the
"As we looked farther and farther out, we kept finding stars that look like halo stars."
The astronomer said he thought that previous groups had
mistakenly identified the outer parts of Andromeda's central bulge as
Stars in the Milky Way's halo are very old, but earlier studies had found those in Andromeda's were of intermediate age.
In addition, the Milky Way's halo stars contained fewer
heavy metals compared with those in the inner parts of the galaxy -
they were "chemically anaemic". This finding was consistent with
theories of galaxy formation.
However, previous work had found that stars in
Andromeda's halo were a factor of 10 richer in heavy metals than those
in the Milky Way.
Observations used in this study came from Nasa's Hubble telescope
Dr Jason Kalirai, another member of the UCSC team, said
the project had partly been started to resolve some of these
He explained that his team had extended their search for
stars in Andromeda further out from the galaxy centre than previous
studies had done.
This was made possible by developing a technique that
allowed true Andromeda stars to be isolated from other objects along
the same line of sight.
They found a clear break in the surface brightness of
stars from the inner parts of Andromeda and fainter ones from outer
parts of the galaxy.
This clean break is seen in the Milky Way, but had previously not been reported in Andromeda.
If theories of galaxy formation and analogies drawn with
the Milky Way were correct, the stars in this outer region should be
depleted in heavy metals compared with those in the inner parts of
This is in fact what the team found.
Paul Hodge, an astronomer who has written a book on
Andromeda, said it had not been possible to resolve differences in the
outer part of the galaxy until the advent of powerful observatories
such as the Hubble Space Telescope.
"For the first time, Andromeda has a very extensive
outer envelope, and we're now learning that it's not just extensive,
it's complicated," said the University of Washington researcher.