Monday, October 27, 2008

ScienceDaily (Oct. 27, 2008) — 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.
See also:
Space & Time






Reference
Asteroid belt
Gas giant
Near-Earth asteroid
Near-Earth object
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 .
Adapted from materials provided by NASA/Jet Propulsion Laboratory.

Related Stories:
Less Than One Week To Go To Name An Asteroid (June 11, 1999) — What's in a name? That could be up to you in the case of Asteroid 1992 KD. But you have to act fast there is only one week left to enter the Planetary Society's Name the Asteroid Contest, ... > read more
Large Asteroid Will Zoom Safely Past Earth (Sep. 29, 2004) — Although asteroid 4179 Toutatis will come no closer than four times the distance between Earth and the Moon (approximately 1.5 million kilometers or 961,000 miles), this will be the closest approach ... > read more
Scientists Analyze Asteroid Data From Deep Space 1 Mission (Aug. 2, 1999) — Engineering and science information from NASA's Deep Space 1 was transmitted from the spacecraft to ground controllers July 30, and the mission team continues to analyze the data. The ... > read more
Cassini Cameras Photograph Asteroid 2685 Masursky (Feb. 22, 2000) — Images taken by Saturn-bound Cassini spacecraft cameras last Jan. 23 have given planetary scientists first size estimates on asteroid 2685 Masursky and preliminary evidence that it may be different ... > read more
Astronomers Sight An Asteroid's Moon (Oct. 7, 1999) — Astronomers this week announced their discovery of a moon orbiting an asteroid, in the first images ever obtained of such an object from Earth. Only one satellite orbiting an asteroid had been seen ... > read more
Circumstellar Dust Takes Flight In 'The Moth' (Jan. 17, 2008) — What superficially resembles a giant moth floating in space is giving astronomers new insight into the formation and evolution of planetary systems. This is not your typical flying insect. It has a ... > read more
Astronomer Discovers New Asteroid Between Mars And Jupiter (Oct. 21, 1999) — Texas A&M University astronomer Don Carona and his colleagues at Stephen F. Austin State University (SFA) have discovered an asteroid orbiting the sun more than 200 million miles from Earth ... > read more
First Detailed Pictures Of Asteroid Reveal Bizarre System (Oct. 17, 2006) — The first detailed images of a binary asteroid system reveal a bizarre world where the highest points on the surface are actually the lowest, and the two asteroids dance in each other's gravitational ... > read more