SETI public: FW: NASA's Spitzer Telescope Sees Signs of Alien Asteroid Belt

From: LARRY KLAES (ljk4_at_msn.com)
Date: Wed Apr 20 2005 - 13:38:03 PDT

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    >From: "NASA Jet Propulsion Laboratory" <info@jpl.nasa.gov>
    >Reply-To: <info@jpl.nasa.gov>
    >To: "Larry Klaes" <ljk4@msn.com>
    >Subject: NASA's Spitzer Telescope Sees Signs of Alien Asteroid Belt
    >Date: Wed, 20 Apr 2005 11:11:19 -0700
    >
    >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 (818) 354-4673
    >Jet Propulsion Laboratory, Pasadena, Calif.
    >
    >News Release: 2005-060                            April 20, 2005
    >
    >NASA's Spitzer Telescope Sees Signs of Alien Asteroid Belt
    >
    >NASA's Spitzer Space Telescope has spotted what may be the dusty
    >spray of asteroids banging together in a belt that orbits a star
    >like our Sun. The discovery offers astronomers a rare glimpse at
    >a distant star system that resembles our home, and may represent
    >a significant step toward learning if and where other Earths
    >form.
    >
    >"Asteroids are the leftover building blocks of rocky planets like
    >Earth," said Dr. Charles Beichman of the California Institute of
    >Technology, Pasadena, Calif. Beichman is lead author of a paper
    >that will appear in the Astrophysical Journal. "We can't directly
    >see other terrestrial planets, but now we can study their dusty
    >fossils."
    >
    >Asteroid belts are the junkyards of planetary systems. They are
    >littered with the rocky scraps of failed planets, which
    >occasionally crash into each other, kicking up plumes of dust. In
    >our own solar system, asteroids have collided with Earth, the
    >moon and other planets.
    >
    >If confirmed, the new asteroid belt would be the first detected
    >around a star about the same age and size as our Sun. The star,
    >called HD69830, is located 41 light-years away from Earth. There
    >are two other known distant asteroid belts, but they circle
    >younger, more massive stars.
    >
    >While this new belt is the closest known match to our own, it is
    >not a perfect twin. It is thicker than our asteroid belt, with 25
    >times as much material. If our solar system had a belt this
    >dense, its dust would light up the night skies as a brilliant
    >band.
    >
    >The alien belt is also much closer to its star. Our asteroid belt
    >lies between the orbits of Mars and Jupiter, whereas this one is
    >located inside an orbit equivalent to that of Venus.
    >
    >Yet, the two belts may have one important trait in common. In our
    >solar system, Jupiter acts as an outer wall to the asteroid belt,
    >shepherding its debris into a series of bands. Similarly, an
    >unseen planet the size of Saturn or smaller may be marshalling
    >this star's rubble.
    >
    >One of NASA's future planet-hunting missions, SIM PlanetQuest,
    >may ultimately identify such a planet orbiting HD 69830.  The
    >mission, which will detect planets as small as a few Earth
    >masses, is scheduled to launch in 2011.
    >
    >Beichman and colleagues used Spitzer's infrared spectrograph to
    >observe 85 Sun-like stars. Only HD 69830 was found to possibly
    >host an asteroid belt. They did not see the asteroids themselves,
    >but detected a thick disk of warm dust confined to the inner
    >portion of the star system. The dust most likely came from an
    >asteroid belt in which dusty smash-ups occur relatively
    >frequently, about every 1,000 years.
    >
    >"Because this belt has more asteroids than ours, collisions are
    >larger and more frequent, which is why Spitzer could detect the
    >belt," said Dr. George Rieke, University of Arizona, Tucson, co-
    >author of the paper. "Our present-day solar system is a quieter
    >place, with impacts of the scale that killed the dinosaurs
    >occurring only every 100 million years or so."
    >
    >To confirm that the dust detected by Spitzer is indeed ground-up
    >asteroids, a second less-likely theory will have to be ruled out.
    >According to the astronomers, it is possible a giant comet,
    >almost as big as Pluto, got knocked into the inner solar system
    >and is slowly boiling away, leaving a trail of dust. This
    >hypothesis came about when the astronomers discovered the dust
    >around the star consists of small silicate crystals like those
    >found in comet Hale-Bopp. One of these crystals is the bright
    >green-colored gem called forsterite.
    >
    >"The 'super comet' theory is more of a long shot," Beichman said,
    >"but we'll know soon enough." Future observations of the star
    >using Spitzer and ground-based telescopes are expected to
    >conclude whether asteroids or comets are the source of the dust.
    >
    >Other authors of this study include G. Bryden, T. Gautier, K.
    >Stapelfeldt and M. Werner of NASA's Jet Propulsion Laboratory,
    >Pasadena, Calif.; and K. Misselt, J. Stansberry and D. Trilling
    >of the University of Arizona.
    >
    >The Jet Propulsion Laboratory manages the Spitzer Space Telescope
    >mission for NASA's Science Mission Directorate, Washington.
    >Science operations are conducted at the Spitzer Science Center,
    >at the California Institute of Technology in Pasadena. Caltech
    >manages JPL for NASA. Spitzer's infrared spectrograph was built
    >by Cornell University, Ithaca, N.Y. Its development was led by
    >Dr. Jim Houck of Cornell.
    >
    >For artist's concepts and more information, visit:
    >www.spitzer.caltech.edu/spitzer .
    >
    >                               -end-
    >
    >
    >
    >
    >
    >

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