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Whitney Clavin 818-354-4673
Jet Propulsion Laboratory
whitney.clavin@jpl.nasa.gov
NEWS RELEASE: 2008-197 Oct. 27, 2008
Closest Planetary System Hosts Two Asteroid Belts
New observations from NASA's Spitzer Space Telescope indicate that the nearest planetary system to
our own has two asteroid belts. Our own solar system has just one.
The star at the center of the nearby system, called Epsilon Eridani, is a younger, slightly cooler and
fainter version of the sun. Previously, astronomers had uncovered evidence for two possible planets
in the system, and for a broad, outer ring of icy comets similar to our own Kuiper Belt.
Now, Spitzer has discovered that the system also has dual asteroid belts. One sits at approximately
the same position as the one in our solar system. The second, denser belt, most likely also populated
by asteroids, lies between the first belt and the comet ring. The presence of the asteroid belts implies
additional planets in the Epsilon Eridani system.
"This system probably looks a lot like ours did when life first took root on Earth," said Dana
Backman, an astronomer at the SETI Institute, in Mountain View, Calif., and outreach director for
NASA's Sofia mission. "The main difference we know of so far is that it has an additional ring of
leftover planet construction material." Backman is lead author of a paper about the findings to appear
Jan. 10 in the Astrophysical Journal.
Asteroid belts are rocky and metallic debris left over from the early stages of planet formation. Their
presence around other stars signals that rocky planets like Earth could be orbiting in the system's
inner regions, with massive gas planets circling near the belts' rims. In our own solar system, for
example, there is evidence that Jupiter, which lies just beyond our asteroid belt, caused the asteroid
belt to form long ago by stirring up material that would have otherwise coalesced into a planet.
Nowadays, Jupiter helps keep our asteroid belt confined to a ring.
Astronomers have detected stars with signs of multiple belts of material before, but Epsilon Eridani is
closer to Earth and more like our sun overall. It is 10 light-years away, slightly less massive than the
sun, and roughly 800 million years old, or one-fifth the age of the sun.
Because the star is so close and similar to the sun, it is a popular locale in science fiction. The
television series Star Trek and Babylon 5 referenced Epsilon Eridani, and it has been featured in
novels by Issac Asimov and Frank Herbert, among others.
The popular star was also one of the first to be searched for signs of advanced alien civilizations
using radio telescopes in 1960. At that time, astronomers did not know of the star's young age.
Spitzer observed Epsilon Eridani with both of its infrared cameras and its infrared spectrometer.
When asteroid and comets collide or evaporate, they release tiny particles of dust that give off heat,
which Spitzer can see. "Because the system is so close to us, Spitzer can really pick out details in the
dust, giving us a good look at the system's architecture," said co-author Karl Stapelfeldt of NASA's
Jet Propulsion Laboratory, Pasadena, Calif.
The asteroid belts detected by Spitzer orbit at distances of approximately 3 and 20 astronomical units
from the star (an astronomical unit is the average distance between Earth and the sun). For reference,
our own asteroid belt lies at about 3 astronomical units from the sun, and Uranus is roughly 19
astronomical units away.
One of the two possible planets previously identified around Epsilon Eridani, called Epsilon Eridani,
was discovered in 2000. The planet is thought to orbit at an average distance of 3.4 astronomical units
from the star -- just outside the innermost asteroid belt identified by Spitzer. This is the first time that
an asteroid belt and a planet beyond our solar system have been found in a similar arrangement as our
asteroid belt and Jupiter.
Some researchers had reported that Epsilon Eridani b orbits in an exaggerated ellipse ranging
between 1 and 5 astronomical units, but this means the planet would cross, and quickly disrupt, the
newfound asteroid belt. Instead, Backman and colleagues argue that this planet must have a more
circular orbit that keeps it just outside the belt.
The other candidate planet was first proposed in 1998 to explain lumpiness observed in the star's
outer comet ring. It is thought to lie near the inner edge of the ring, which orbits between 35 and 90
astronomical units from Epsilon Eridani.
The intermediate belt detected by Spitzer suggests that a third planet could be responsible for creating
and shepherding its material. This planet would orbit at approximately 20 astronomical units and lie
between the other two planets. "Detailed studies of the dust belts in other planetary systems are
telling us a great deal about their complex structure," said Michael Werner, co-author of the study
and project scientist for Spitzer at JPL. "It seems that no two planetary systems are alike."
JPL manages the Spitzer mission for NASA's Science Mission Directorate, Washington. Science
operations are conducted at the Spitzer Science Center at the California Institute of Technology in
Pasadena. Caltech manages JPL for NASA. More information about Spitzer is at
http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer . More information about
extrasolar planets and NASA's planet-finding program is at http://planetquest.jpl.nasa.gov .
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