SETI public: Fw: Scientists Discover First of a New Class of Extrasolar Planets

From: LARRY KLAES (ljk4_at_msn.com)
Date: Tue Aug 31 2004 - 10:52:06 PDT

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    ----- Original Message -----
    From: NASA Jet Propulsion Laboratory<mailto:info_at_jpl.nasa.gov>
    To: ljk4_at_msn.com<mailto:ljk4_at_msn.com>
    Sent: Tuesday, August 31, 2004 1:25 PM
    Subject: Scientists Discover First of a New Class of Extrasolar Planets

    MEDIA RELATIONS OFFICE
    JET PROPULSION LABORATORY
    CALIFORNIA INSTITUTE OF TECHNOLOGY
    NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
    PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011
    http://www.jpl.nasa.gov/>

    Whitney Clavin (626) 354-4673/354-5011
    Jet Propulsion Laboratory, Pasadena, Calif.

    Donald Savage (202) 358-1547
    NASA Headquarters, Washington, D.C.

    News Release:
    2004-212
     August 31, 2004

    Scientists Discover First of a New Class of Extrasolar Planets

    Astronomers announced today the first discovery of a new class of
    planets beyond our solar system about 10 to 20 times the size of Earth
    - far smaller than any previously detected. The planets make up a new
    class of Neptune-sized extrasolar planets.

    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 Drs. Paul Butler and
    Geoffrey 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.

    "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."

    "These Neptune-sized planets prove that Jupiter-sized, gas giants
    aren't the only planets out there," Marcy said. Butler added,
    "We are beginning to see smaller and smaller planets. Earth-like
    planets are the next destination."

    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.

    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.

    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.

    For visuals depicting the new planets and information about NASA's
    planet-hunting missions on the Internet, visit:
    http://planetquest.jpl.nasa.gov/news/ssu_images.html>

    http://planetquest.jpl.nasa.gov/>

    -end-


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