NASA'S Hubble Shows Hyperfast Star Was Booted From Milky Way
WASHINGTON -- NASA's Hubble Space Telescope has detected a
hypervelocity star, a rare phenomenon moving three times faster than
our sun.
The star may have been created in a cosmic misstep. A hundred million
years ago, a triple-star system was traveling through the bustling
center of our Milky Way galaxy when it wandered too close to the
galaxy's giant black hole. The black hole captured one of the stars
and hurled the other two out of the Milky Way. The two outbound stars
merged to form a super-hot blue star traveling at incredible speeds.
This story may seem like science fiction, but Hubble astronomers say
it is the most likely scenario for the creation of a so-called
hypervelocity star, known as HE 0437-5439. It is one of the fastest
ever detected with a speed of 1.6 million mph. Hubble observations
confirm that the stellar speedster hails from the Milky Way's core,
settling some confusion about the star's original home.
Most of the roughly 16 known hypervelocity stars, all discovered since
2005, are thought to be exiles from the heart of our galaxy. But this
Hubble result is the first direct observation linking such a star to
an origin in the center of the galaxy.
"Using Hubble, we can for the first time trace back to where the star
came from by measuring the star's direction of motion on the sky,"
said astronomer Warren Brown of the Harvard-Smithsonian Center for
Astrophysics in Cambridge, Mass. "Our measurements point directly to
the Milky Way center."
Brown, a member of the Hubble team that observed the star, is the lead
author on a paper about the finding published online July 20 in the
Astrophysical Journal Letters.
Brown said, "These exiled stars are rare in the Milky Way's population
of 100 billion stars. For every 100 million stars in the galaxy,
there lurks one hypervelocity star."
The stellar outcast already is cruising in the Milky Way's distant
outskirts about 200,000 light-years from the galaxy's center. Using
Hubble to measure the runaway star's direction and determine the
Milky Way's core as its starting point, Brown and Gnedin's team
calculated how fast the star had to have been ejected to reach its
current location.
"Studying these stars could provide more clues about the nature of
some of the universe's unseen mass, and it could help astronomers
better understand how galaxies form," said team leader Oleg Gnedin of
the University of Michigan in Ann Arbor.
The star's age is another mystery. Based on the speed and position of
HE 0437-5439, the star would have to be 100 million years old to have
journeyed from the Milky Way's core. Yet its mass -- nine times that
of our sun-- and blue color mean that it should have burned out after
only 20 million years -- far shorter than the transit time it took to
get to its current location.
Astronomers have proposed two possibilities to solve the age problem.
The star either dipped into the Fountain of Youth by becoming a blue
straggler, or it was flung out of the Large Magellanic Cloud, a
neighboring galaxy.
In 2008 a team of astronomers thought they had solved the mystery.
They found a match between the exiled star's chemical makeup and the
characteristics of stars in the Large Magellanic Cloud. The rogue
star's position also is close to the neighboring galaxy, only 65,000
light-years away. The new Hubble result, however, settles the debate
over the star's birthplace and places it in the Milky Way.
The most likely explanation for the star's blue color and extreme
speed is that it was part of a triple-star system that was involved
in a gravitational billiards game with the galaxy's monster black
hole. This concept for imparting an escape velocity on stars was
first proposed in 1988. The theory predicted the Milky Way's black
hole should eject a star about once every 100,000 years.
The triple-star system contained a pair of closely orbiting stars and
a third outer member also gravitationally tied to the group. The
black hole pulled the outer star away from the tight binary system.
The doomed star's momentum was transferred to the stellar twosome,
boosting the duo to escape velocity from the galaxy. As the pair
rocketed away, they went on with normal stellar evolution.
The more massive companion evolved more quickly, puffing up to become
a red giant. It enveloped its partner, and the two stars spiraled
together, merging into one superstar, the blue straggler that Hubble
observed. A blue straggler is a relatively young, massive star
produced by the merger of two lighter-weight stars.
Astronomers used the sharp vision of Hubble's Advanced Camera for
Surveys to make two separate observations of the wayward star 3.5
years apart. Team member Jay Anderson of the Space Telescope Science
Institute in Baltimore developed a technique to measure the star's
position relative to each of 11 distant background galaxies. These
background galaxies form a reference frame in which Anderson compared
the star's position in 2006 and 2009 to calculate how far it had moved.
"Hubble excels with this type of measurement," Anderson said. "This
observation would be challenging to do from the ground."
The team is trying to determine the homes of four other unbound stars,
all located on the fringes of the Milky Way.
"We are targeting massive "B" stars, like HE 0437-5439," said Brown,
who has discovered 14 of the 16 known hypervelocity stars. "These
stars shouldn't live long enough to live in the distant outskirts of
the Milky Way, so we shouldn't expect to find them there. But the
quantity of stars in the outer region is much less than in the core,
so we have a better chance of finding these unusual objects."
For graphics and more information about HE 0437-5439, visit:
http://www.nasa.gov/hubble
Source: NASA
