The list of known exoplanets in the galaxy just got bigger, thanks to the first observations of NASA's Kepler space telescope, which found five new lightweight worlds orbiting.
"I would like to announce today the discovery of five exoplanets by Kepler," said Kepler science director William Borucki of NASA's Ames Research Center in Moffett Field, Calif., here today at the 215th meeting of the .
The planet-hunting Kepler, which hopes to discover alien Earths, also found an odd object orbiting a star and is measuring the quakes that ripple across stellar surface.
The five newfound planets are all much larger than the Earth-sized bodies Kepler was designed to find, with one coming in at around the size of Neptune, and the other four measuring larger than .
All five planets orbit very close to their stars, with orbital periods of around three to four days, and so are very hot. Their temperatures are above those of molten lava; even iron would melt on their surfaces.
"So these are very hot, very bright planets," Borucki said.
While the Neptune-sized planets, dubbed Kepler 4b, is about the density of the ice giants in our solar system (and so likely has an abundance of elements heavier than hydrogen and helium), one of the other newfound planets, Kepler 7b, has one of the lowest densities of any planet ever discovered, Borucki said.
While these planets aren't the type that scientists hope Kepler will ultimately find, the observations that the telescope has made so far show that "we do have the sensitivity to find Earth-size planets," Borucki said.
Kepler, which launched on March 6, 2009, looks for dips in the light curves of stars that indicate a planet transiting in front of the star (from the perspective of Earth).
Kepler also observes occultations of planets, or the light curve dips that occur when the planet moves behind its parent star. The telescope has made one strange observation of a system where the light curve from the orbiting body dips more during the occultation than during its transit, which suggests that it is much hotter than its parent star – certainly an odd situation for a planet-star system. The body could be a small, relatively cool white dwarf, but its size is too big for a white dwarf.
"So we're not quite sure what we're seeing here," Borucki said.
Kepler has also shown its ability to measure the oscillations that occur at a star's surface that cause it to "ring like a bell" and its brightness to vary. Studying this stellar seismology can help scientists better understand the age and structure of stars. Kepler data for one star has pinned down that star's diameter from within a 10 percent margin of error to within 1 percent.
"This in turn gives astronomers much better knowledge of the planet's density, in the case studied this has improved from about 50 percent uncertainty to five percent, which is very important for understanding exoplanets, said Ron Gilliland of thein Baltimore, Md., and the principal investigator for Kepler's astroseismology program.
The results announced at the meeting come from just the first 43 days of Kepler observations; scientists now have more than eight months of data to comb through, Borucki said.