Astronomers Claim Potential Mini Solar System

For several years, astronomers have struggled to distinguish between planets, stars, and in-between objects known as brown dwarfs.

Brown dwarfs are generally thought to be more massive than planets, but not hefty enough to ignite the thermonuclear fusion that powers a normal star.

So things get really confusing when a brown dwarf has an object orbiting it. Is that a planet?

Things get even more confusing when, as now, astronomers discover a modest brown dwarf -- one with a mass that could be considered planet-like -- that looks as if its about to spawn planet-like objects.

A team led by Kevin Luhman of Penn State University announced Tuesday the discovery of a brown dwarf just eight times the mass of Jupiter. It's considered a brown dwarf in part because it formed alone in space, not orbiting anything else. And it is encircled by a disk of material that looks very much like planet-forming regions seen around real stars.

Nobody knows if the gas and dust in the disk will coalesce into planets. But Luhman speculates that the newfound setup could evolve into a miniature solar system.

"Here we have a Sun that is so small it is the size of a planet," he said. "The question then becomes, what do we call any little bodies that might be born from this disk: planets or moons?"

"Some go by size, and others go by how the object formed," says study team member Giovanni Fazio of the Harvard-Smithsonian Center for Astrophysics. "For instance, this new object would be called a planet based on its size, but a brown dwarf based on how it formed."

Luhman and colleagues studied the brown dwarf, called Cha 110913-773444, with NASA's Spitzer Space Telescope, the Hubble Space Telescope, and two telescopes in the Chilean Andes, the Blanco telescope of the Cerro Tololo Inter-American Observatory and the Gemini South telescope.

The object is 500 light-years away in the constellation Chameleon. It is about 2 million years old. Our Sun is about 4.6 billion years old.

The results will be detailed in the Dec. 10 issue of Astrophysical Journal Letters.