YAHOO.COM - The Milky Way galaxy, home of Earth's solar system, may actually be only half as massive as currently thought, scientists say.
Stars in the far outer reaches of the Milky Way,
between 260,000 and 490,000 light-years from the galactic center, are
cruising around surprisingly slowly, researchers found. Galactic mass
and star velocities are linked, so the results could have big
implications.
"Because these velocities are so low, the mass of our galaxy may be
much lower than we once thought," lead author Alis Deason, of the
University of California, Santa Cruz, told reporters Wednesday (Jan. 9)
at the 221st meeting of the American Astronomical Socity in Long Beach,
Calif.
"If we infer the properties of the stars that we think are reasonable,
then we find the mass of the Milky Way could be half as massive as we
currently believe," added Deason, who performed the research while at
the University of Cambridge in England. [Stunning Photos of Our Milky Way Galaxy]
The Milky Way is composed of three main parts: a central bulge, a
relatively flat disk and a roughly spherical surrounding halo.
Deason and her team looked far out into the Milky Way's halo,
which extends far beyond the 100,000-light-year-wide disk. They
measured the radial velocities of a sample of distant halo stars using
two different instruments: the European Southern Observatory's 8.2-meter
telescope in Chile and the 4.2-meter William Herschel Observatory in
Spain.
They found that the dispersion, or spread, of halo-star velocities was
about half that seen for stars closer to the galactic center.
"This was quite a surprise when we found this," Deason said.
Using this information, the team calculated that the total mass of the
Milky Way out to such extreme distances may be between 500 billion and 1
trillion times that of our sun — substantially lower than the current
leading estimate, Deason said.
But the new study is not necessarily the final word on the Milky Way's mass, which is not well understood.
"The problem is, we are really in unknown territory," Deason said. "We
are assuming properties of these stars that are the same in the inner
parts of the galaxy. And this is something that really needs to be
verified, what we're assuming, in terms of their density profile and
also what their orbits are like."
Future work along these lines could help astronomers map the
distribution of mass throughout the Milky Way, Deason said, potentially
shedding light on the mysterious dark matter that is thought to make up more than 80 percent of all matter in the universe.
"I think we will be able to use measurements like this to not only say
what the total mass is, but also if the dark matter distribution is what
we expect," she said. "At the moment, we just don't know."