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  • Frits Westra
    Forwarded by: fwestra@hetnet.nl Originally from: baalke@jpl.nasa.gov Original Subject: US Astronomers Meet At Arecibo To Discuss Next-Generation Radio
    Message 1 of 1 , Mar 4 6:52 AM
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      Forwarded by: fwestra@...
      Originally from: baalke@...
      Original Subject: US Astronomers Meet At Arecibo To Discuss Next-Generation Radio Telescope
      Original Date: Fri, 3 Mar 2000 16:18:27 -0800 (PST)

      ========================== Forwarded message begins ======================


      U.S. astronomers meet at Arecibo to discuss spending, siting and science
      for mammoth-size, next-generation radio telescope

      FOR RELEASE: March 3, 2000

      Contact: David Brand
      Office: (607) 255-3651
      E-mail: deb27@...

      ARECIBO, P.R. -- It would be one of the largest scientific instruments ever
      assembled, a radio telescope composed of perhaps 1,000 antennas spread out
      over more than 600 miles and costing more than $600 million dollars. And it
      would make possible high-resolution probes of the outer edges of the
      universe, giving a window on the evolution of galaxies, the birth and death
      of stars and a detailed portrait of our own solar system.

      The global astronomy community has dubbed the new telescope the Square
      Kilometer Array, or SKA, and it hopes that if funding and technical
      problems can be overcome, the massive instrument will be focusing its beams
      on the distant universe within a decade or so.

      To attempt to put a pragmatic and realistic face on the huge project, which
      would be the new generation of low-frequency radio telescope, more than 60
      radio astronomers affiliated with the U.S. segment of the international
      planning effort -- the SKA U.S. Consortium -- held their first meeting Feb.
      28 and 29 at Arecibo Observatory, which is managed by Cornell University,
      through the National Astronomy and Ionosphere Center (NAIC), for the
      National Science Foundation (NSF).

      "The SKA is only going to succeed after a considerable gestation period,"
      said Paul Goldsmith, Cornell astronomy professor and director of the NAIC.
      But he warned the astronomers that "there must be clear, incremental
      progress on the project."

      Planning for the telescope has been under way since 1997 by institutes in
      six nations, and Holland, Canada and China have each produced a different
      telescope design. The U.S. role is to concentrate on designing an array
      made up of a large number of small antennas -- each acting as a separate
      radio telescope -- noted the chair of the U.S. Consortium, Jackie Hewitt of
      the Massachusetts Institute of Technology.

      Speakers from Cornell and the nine other members of the U.S. Consortium, as
      well as the larger astronomy community, described not only the quantum leap
      in the view of the radio universe that the SKA would make possible, but
      also issues such as how to prevent radio interference from affecting such a
      hugely sensitive instrument, how to write the complex software needed to
      operate the telescope, where to site it and how to pay for it. It is
      assumed that the United States will bear about one-third of the cost.

      Colin Lonsdale of MIT's Haystack Observatory noted that a telescope made up
      of perhaps 1,000 antenna "stations" would provide superb imaging fidelity,
      with more accurate calibration than currently possible, with each station
      capable of imaging objects in many directions simultaneously. The
      telescope would depend heavily on electronics, he said, requiring about
      5,000 kilometers of connecting fiber-optics cable.

      Although the telescope's span would be 1,000 kilometers (620 miles), its
      actual collecting area for radio beams would be only about a square
      kilometer, or about a half square mile. The antennas would form a type of
      telescope called an interferometer, in which radio signals from distant
      objects in the universe are captured by separate antennas and brought
      together at a central processor. The single image produced would have a
      resolution equivalent to an image produced by an antenna 1,000 kilometers
      in diameter.

      Because definition improves as a telescope's diameter increases, the SKA
      would be 100 times more sensitive than today's most powerful radio
      telescopes, such as Arecibo and the Very Large Array (VLA), west of
      Socorro, N.M., consisting of 27 antennas arranged in a Y pattern up to 22
      miles across. The SKA's collecting area would be an order of magnitude
      greater than the VLA's.

      Where should such a massive telescope be located, particularly since it
      would have to be expandable up to 1,000 kilometers in some directions?
      Meeting chair Yervant Terzian, the David C. Duncan Professor of Astronomy
      and Space Sciences at Cornell, said the project would be handicapped until
      a site was located. The site, he said, must be relatively free of radio
      interference and in an accessible region of a politically stable country
      with no weather extremes. At the top of his list was the Upper
      Gascoyne-Murchison region of Western Australia. He also mentioned the
      Southwestern United States.

      "How and who makes this decision I have no idea," he said. "But this is
      not a premature discussion. These sensitivities must be addressed."

      Although most of the participants assumed that the telescope would be
      funded by national agencies such as the NSF, Mike Davis of NAIC, an adjunct
      professor of astronomy at Cornell, suggested seeking private funding.
      This, he said, might mean a much slower development period for the
      telescope, but sections could be put into operation as they were built.
      "We could grow the SKA into existence with interim use along the way," he
      said.

      Bernard Burke, professor of physics and astronomy at MIT, however, warned
      that the major technical problems facing the planners were mainly
      cost-related, which could inflate the project's budget. This is a warning
      signal, he said, noting that the superconducting supercollider overran its
      budget and was canceled by the U.S. Congress.

      One of the most serious technical problems, radio interference, was
      outlined by Rick Fisher of the National Radio Astronomy Observatory (NRAO),
      who said that such a massive instrument would be highly susceptible to
      radio frequency interference. He spoke about current research into
      suppressing this radio noise to levels that would allow the SKA to function
      without interference. "It is going to take years of research before we are
      down to the levels of sensitivity that radio astronomers will need," he
      said.

      But the window on the universe that the SKA would make possible -- what
      some called a true radio map of the sky -- held much of the meeting's
      attention. Cornell astronomy Professor James Cordes said that the SKA
      would be able to probe "by many factors of 10" more of the universe than is
      now possible with the Arecibo radio telescope. And it would allow the
      detection of tens to hundreds more pulsars -- fast-spinning, highly dense
      stars called neutron stars -- in other galaxies. Possibly it also would
      answer such questions as "What is the endgame for neutron stars?" and "What
      is the relation of neutron stars to supernovae?"

      Said Cordes, "SKA can dramatically alter our knowledge of galactic
      compacted objects." Furthermore, said Cornell astronomy Professor Riccardo
      Giovanelli, "SKA could make important contributions in the field of spiral
      galaxies still being formed."

      Indeed, such high-resolution images would be possible with the SKA that
      astronomers could make an "extensive survey" of much of the solar system,
      including the outer planets, asteroids and comets, said Donald Campbell,
      Cornell astronomy professor and associate director of NAIC. "SKA could
      actually produce images as good as those from the NEAR spacecraft," which
      on Feb. 14 became the first spacecraft to orbit an asteroid, he said.

      The SKA's importance to space exploration also was noted by Sandy Weinreb
      of NASA's Jet Propulsion Laboratory, who said that the agency is exploring
      the possibility of building an SKA-like instrument for its Deep Space
      Network. Had this been operational last year when the Mars Climate Orbiter
      spacecraft was lost as it went into Martian orbit, he said, the mission's
      off-course problems would have been detected and corrected.

      The U.S. Consortium members, besides Cornell/NAIC, are the University of
      California at Berkeley, the California Institute of Technology, MIT,
      Georgia Institute of Technology, Ohio State University, NRAO, the SETI
      Institute, Harvard/Smithsonian Astrophysical Observatory and the University
      of Minnesota.

      Related World Wide Web sites: The following sites provide
      additional information on this news release. Some might not be part of the
      Cornell University community, and Cornell has no control over their content
      or availability.

      -- SKA U.S. Consortium: <http:// www.usska.org>

      -- Arecibo Observatory: <http://naic.edu>

      -30-



      The web version of this release may be found at

      http://www.news.cornell.edu/releases/March00/SKA_meeting.deb.html

      EDITORS: For further information on this release, contact Professor Donald
      Campbell at Arecibo National Observatory (787) 878-2612.


      Cornell University News Service
      Surge 3
      Cornell University
      Ithaca, NY 14853
      607-255-4206
      cunews@...
      http://www.news.cornell.edu

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