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Two Discoveries Reveal Diversity of Galaxy's Extrasolar Planets
(From the May/June 2006 issue of StarDate magazine)

Radio astronomers studying a disk of planet-forming material around a star 500 light-years from Earth have found that the inner disk rotates in the opposite direction of the outer disk. This never-before-seen behavior means that planets that form close to this star will orbit it one direction, and planets formed farther out in the other.

A five-Earth-mass planet orbits a red dwarf star. Above, portions of this planet-forming disk rotate in opposite directions.
A five-Earth-mass planet orbits a red dwarf star.

Anthony Remijan of the National Radio Astronomy Observatory and Jan Hollis of NASA's Goddard Space Flight Center used the Very Large Array radio telescope in New Mexico to track molecules of silicon monoxide as they orbited in the disk of this star. The molecules emit radio waves at known frequencies. These frequencies shift higher or lower, depending on the molecules' motions toward or away from Earth. These "Doppler shifts" revealed the opposite rotations of the inner and outer disk.

Though never seen around a star, "similar structures and dynamics commonly occur on small and large scales throughout the universe," Hollis said.

The two astronomers speculate that this star was formed by the merger of two large gas clouds rotating in opposite directions.

A large group of astronomers has found the least massive extrasolar planet yet. Only five times more massive than Earth, it orbits a small, cool red dwarf star every 10 years at about three times the Earth-Sun distance.

"This finding means that Earth-mass planets are not that uncommon," team member Kailash Sahu of the Space Telescope Science Institute said. "If we found one, there must be more."

Astronomers took advantage of a phenomenon called "gravitational microlensing" to discover the planet. When a massive star passes precisely in front of a background star, the gravity of the foreground star acts like a lens, amplifying the light coming from the background star. The more massive the foreground star, the longer this "light boost" lasts. And if the foreground star has an unseen planetary companion, that lengthens the boost, too. In this case, the lensing event lasted a dozen hours longer than expected — revealing the presence of the unseen planet. — Rebecca Johnson


» More information about extrasolar planets

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