SETI bioastro: FW: JPL: Dust From Black Holes is Found

From: LARRY KLAES (ljk4_at_msn.com)
Date: Wed Oct 10 2007 - 06:01:34 PDT

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    >From: "AAS Press Officer Dr. Steve Maran" <Steve.Maran_at_aas.org>
    >To: "AAS Press Officer Dr. Steve Maran" <steve.maran_at_aas.org>
    >Subject: JPL: Dust From Black Holes is Found
    >Date: Tue, 9 Oct 2007 16:52:07 -0400
    >

    THE FOLLOWING RELEASE WAS RECEIVED FROM THE JET PROPULSION LABORATORY, IN
    PASADENA, CALIFORNIA, AND IS FORWARDED FOR YOUR INFORMATION. (FORWARDING
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    Maran, American Astronomical Society steve.maran_at_aas.org 1-202-328-2010
    x116

    Contact:
    Whitney Clavin
    1-818-354-4673 Whitney.clavin_at_jpl.nasa.gov

    NEWS RELEASE: 2007-114 Oct. 9, 2007

    ASTRONOMERS FIND DUST IN THE WIND OF BLACK HOLES

    The hit song that proclaimed, "All we are is dust in the wind," may have
    some cosmic truth to it. New findings from NASA's Spitzer Space Telescope
    suggest that space dust - the same stuff that makes up living creatures and
    planets - was manufactured in large quantities in the winds of black holes
    that populated our early universe.

    The findings are a significant new clue in an unsolved mystery: where did
    all the dust in the young universe originate?

    "We were surprised to find what appears to be freshly made dust entrained in
    the winds that blow away from supermassive black holes," said Ciska
    Markwick-Kemper of the University of Manchester, U.K. Markwick-Kemper is
    lead author of a new paper appearing in an upcoming issue of the
    Astrophysical Journal Letters. "This could explain where the dust came from
    that was needed to make the first generations of stars in the early
    universe."

    Space dust is essential to the formation of planets, stars, galaxies and
    even life as we know it. The dust in our corner of the universe was piped
    out by dying stars that were once a lot like our sun. But, when the universe
    was less than a tenth of its present age of 13.7 billion years, sun-like
    stars hadn't been around long enough to die and make dust. So, what produced
    the precious substance back when the universe was just a toddler?

    Theorists have long-postulated that short-lived, massive exploding stars, or
    supernovae, might be the source of this mysterious dust, while others have
    proposed that a type of energetic, growing supermassive black hole, called a
    quasar, could be a contributing factor. A quasar consists of a supermassive
    black hole surrounded by a dusty doughnut-shaped cloud that feeds it.
    Theoretically, dust could form in the outer portion of the winds that slowly
    blow away from this doughnut cloud.

    "Quasars are like the Cookie Monster," said co-author Sarah Gallagher of the
    University of California at Los Angeles, who is currently a visiting
    astronomer at the University of Western Ontario, Canada. "They are messy
    eaters, and they can consume less matter than they spit out in the form of
    winds."

    Nobody has found conclusive proof that either quasar winds or supernovae can
    create enough dust to explain what is observed in the early universe.
    Markwick-Kemper and her team decided to test the former theory and
    investigate a quasar, called PG2112+059, located in the center of a galaxy
    about 8 billion light-years way. Although this particular quasar is not
    located in the early universe, because it is closer, it is an easier target
    for addressing the question of whether quasars can make dust. The team used
    Spitzer's infrared spectrograph instrument to split apart infrared light
    from the quasar and look for signs of various minerals.

    They found a mix of the ingredients that make up glass, sand, marble and
    even rubies and sapphires. While the mineral constituting glass was
    expected, the minerals for sand, marble and rubies were a surprise. Why?
    These minerals are not typically detected floating around galaxies,
    suggesting they could have been freshly formed in the winds rushing away
    from the quasar.

    For instance, the ingredient that makes up sand, crystalline silicate,
    doesn't survive for long free-floating in space. Radiation from stars zaps
    the minerals back to an amorphous, glass-like state. The presence of
    crystalline silicate therefore suggests something - possibly the quasars
    winds - is churning out the newly made substance.

    Markwick-Kemper and her team say the case of the missing dust is not firmly
    shut. They hope to study more quasars for further evidence of their
    dust-making abilities. Also, according to the astronomers, quasars may not
    be the only source of dust in the early universe. "Supernovae might have
    been more important for creating dust in some environments, while quasars
    were more important in others," said Markwick-Kemper. "For now, we are very
    excited to have identified the different species of dust in a quasar
    billions of light-years away."

    Other authors of this paper include Dean Hines of the Space Science
    Institute, Boulder, Colo., and Jeroen Bouwman of the Max Planck Institute
    for Astronomy, Heidelberg, Germany. NASA's Jet Propulsion Laboratory,
    Pasadena, Calif., 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, also
    in Pasadena. Caltech manages JPL for NASA. Spitzer's infrared spectrograph
    was built by Cornell University, Ithaca, N.Y. Its development was led by Jim
    Houck of Cornell.

    For graphics and more information about Spitzer, visit
    http://www.spitzer.caltech.edu/spitzer and http://www.nasa.gov/spitzer .

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