More than a third of the planets discovered so far beyond our solar system are Jupiter-size giants that orbit their star closer than the planet Mercury to our Sun. Being so close to their star, these planets are hot. They can hold on to an extensive atmosphere in spite of the heat, only because of their large size and strong surface gravity. These two new planets are much smaller, however, with masses only about one tenth that of Jupiter. They must be very hot, and it is not clear whether they have sufficient gravity to hold a massive atmosphere or to permit large amounts of ice in their interiors, as is the case for Neptune and Uranus within our solar system. Thus is is probably not appropriate to call them "hot Neptunes" by analogy with the previously known "hot Jupiters". They may be very different from anything we know in our own system.
In addition to the the press release noted below, you can find out more about these new planets in the article "Neptune-Class Worlds" at http://www.astrobio.net/news/article1165.html
NAI Senior Scientist
Results from NASA-funded research have put humankind just a little closer to answering the age old question, "Are we alone in the universe?"
Astronomers have announced the first discovery of a new class of planets beyond our solar system. The Neptune-sized planets -- about 10 to 20 times the size of Earth -- are far smaller than any ot the previously detected extrasolar "gas giants." It's even possible that the new class of planets are rocky, like Earth and Mars, and scientists are enthusiatic about the discoveries that may come next.
"These Neptune-sized planets prove that Jupiter-sized, gas giants aren't the only planets out there," Dr. Geoffrey Marcy, one of the planet co-discoverers, said. His partner, Dr. Paul Butler, added, "We are beginning to see smaller and smaller planets. Earth-like planets are the next destination."
In addition, one of the new planets joins three others around the nearby star 55 Cancri to form the first known four-planet system.
The discoveries consist of two new planets. They were discovered by the world renowned planet-hunting team of Butler and Marcy of the Carnegie Institute of Washington and University of California, Berkeley, respectively; and Barbara McArthur of the University of Texas, Austin. Both findings were peer- reviewed and accepted for future publication in the Astrophysical Journal. NASA and the National Science Foundation funded the research.
Because the new planets are smaller than Jupiter, it is possible they are made of rock, or rock and ice, rather than gas. According to the scientists, the planets may have, like Earth, formed through gradual accumulation of rocky bodies. "A planet of Neptune's size may not have enough mass to hold onto gas, but at this point we don't know," Butler said.
"NASA, along with our partner NSF, is extremely proud of this significant planetary discovery," said Al Diaz, Associate Administrator of NASA's Science Mission Directorate. "The outcome of the tremendous work of the project scientists is a shining example of the value of space exploration."
Future NASA planet-hunting missions, including Kepler, the Space Interferometry Mission and the Terrestrial Planet Finder, will seek such Earth-like planets. Nearly 140 extrasolar planets have been discovered.
Both of the new planets stick very close to their parent stars, whipping around them in a matter of days. The first planet, discovered by Marcy and Butler, circles a small star called Gliese 436 about every two-and-one-half days at just a small fraction of the distance between Earth and the Sun, or 4.1 million kilometers (2.6 million miles). This planet is only the second known to orbit an M dwarf, a type of low-mass star four-tenths the size of our own sun. Gliese 436 is located in our galactic backyard, 30 light-years away in the constellation Leo.
The second planet, found by McArthur, speeds around 55 Cancri in just under three days, also at a fraction of the distance between Earth and the sun, at approximately 5.6 million kilometers (3.5 million miles). Three larger planets also revolve around the star every 15, 44 and 4,520 days, respectively. Marcy and Butler discovered the outermost of these in 2002. It is still the only known Jupiter-like gas giant to reside as far away from its star as our own Jupiter. The 55 Cancri is about 5 billion years old, a bit lighter than the sun, and is located 41 light-years away in the constellation Cancer. "55 Cancri is a premier laboratory for the study of planetary system formation and evolution," McArthur said.
Both discoveries were made using the "radial velocity" technique, in which a planet's gravitational tug is detected by the wobble it produces in the parent star. Butler, Marcy and collaborators, including Dr. Deborah Fischer of San Francisco State University and Dr. Steven Vogt of the University of California, Santa Cruz, discovered their "Neptune" after careful observation of 950 nearby stars with the W.M. Keck Observatory in Mauna Kea, Hawaii. They were able to spot such a relatively small planet, because the star it tugs on is small and more susceptible to wobbling.
McArthur and collaborators Drs. Michael Endl, William Cochran and Fritz Benedict of the University of Texas discovered their "Neptune" after obtaining over 100 observations of 55 Cancri from the Hobby- Eberly Telescope at McDonald Observatory in West Texas. Combining this data with past data from Marcy, Fischer and Butler from the Lick Observatory in California, and archival data from NASA's Hubble Space Telescope, the team was able to model the orbit of 55 Cancri's outer planet. This, in turn, allowed them to clearly see the orbits of the other three inner planets, including the new Neptune-sized one.
Whitney Clavin (626) 354-4673/354-5011
Jet Propulsion Laboratory, Pasadena, Calif.
Donald Savage (202) 358-1547
NASA Headquarters, Washington, D.C.