SETI bioastro: FW: Spacecraft to Launch, Designed to Harpoon Cosmic 'Moby Dick'

From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Feb 19 2004 - 21:11:43 PST

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    >From: NASA Jet Propulsion Laboratory <info_at_jpl.nasa.gov>
    >Reply-To: NASA Jet Propulsion Laboratory <info_at_jpl.nasa.gov>
    >To: ljk4_at_msn.com
    >Subject: Spacecraft to Launch, Designed to Harpoon Cosmic 'Moby Dick'
    >Date: Thu, 19 Feb 2004 16:27:01 -0600
    >
    >DC Agle (818) 393-9011
    >Jet Propulsion Laboratory, Pasadena, Calif.
    >
    >Donald Savage (202) 358-1727
    >NASA Headquarters, Washington, D.C.
    >
    >Release: 2004-065 February 19, 2004
    >
    >Spacecraft to Launch, Designed to Harpoon Cosmic 'Moby Dick'
    >
    >Like the massive white whale in Herman Melville's 1851
    >classic "Moby Dick," comets have long been considered swift,
    >elusive harbingers of change. So it should be of little
    >surprise that one of the best ways for scientists to study
    >the mysteries of comets is to harpoon one.
    >
    >The European Space Agency's Rosetta spacecraft is scheduled
    >to lift off on Feb. 26, 2004, at 2:16 am Eastern time, from
    >the Kourou spaceport in French Guiana, on the northeastern
    >coast of South America. The launch will be the beginning of
    >a ten-and-a-half year odyssey to comet Churyumov-Gerasimenko
    >that includes flybys of Mars (2007) and the Earth (2005,
    >2007 and 2009).
    >
    >Among the instruments aboard the Rosetta spacecraft are
    >three instruments funded by NASA and a key component of a
    >fourth. The NASA instruments will examine Churyumov-
    >Gerasimenko from the orbiter.
    >
    >"This comet has only about three-hundred-thousandths the
    >gravity of Earth," said Dr. Claudia Alexander, project
    >scientist for the U.S. role in the mission, from NASA's Jet
    >Propulsion Laboratory Pasadena, Calif. "The Rosetta
    >spacecraft will be able to make observations from as close
    >as 2 kilometers (1.2 miles). The data from our state-of-the-
    >art instruments will be amazing," she added.
    >
    >Rosetta will reach Churyumov-Gerasimenko, a four-kilometer-
    >diameter (2.5-mile) comet, in May 2014. When this rendezvous
    >occurs, Churyumov-Gerasimenko will be about three times as
    >far from the sun as Earth is. Over the next 18 months
    >Rosetta will study how the comet changes as it moves closer
    >to the sun. In November 2014, Rosetta will drop its
    >experiment-laden, harpoon-firing lander on Churyumov-
    >Gerasimenko's icy nucleus.
    >
    >"What you have to understand is that comets are primordial
    >remnants of the early solar system," explained Dr. Paul
    >Weissman of JPL. "They are the keys to understanding the way
    >the whole solar system, our Earth, and how even we came into
    >being. And with Rosetta we will be able to observe, study
    >and analyze this primordial material up close for more than
    >a year," he said.
    >
    >JPL supplied the Microwave Instrument for Rosetta Orbiter,
    >the first of its type on any interplanetary mission. This
    >instrument can reveal the abundances of selected gases,
    >their temperatures, the speed at which they are coming off the
    >nucleus, and the temperature of the nucleus. Scientists will
    >use the instrument to monitor changes in how vapors are
    >released from the nucleus as the coma and tail grow. They
    >will be studying water, carbon monoxide, ammonia and
    >methanol, four of the most abundant gases from comets. Dr.
    >Samuel Gulkis of JPL's Earth and Space Sciences Division is
    >principal investigator.
    >
    >The Southwest Research Institute, based in San Antonio,
    >supplied two NASA instruments for Rosetta. One is an imaging
    >telescope/spectrometer capable of analyzing the composition
    >both of gases released by the comet and of the comet's
    >surface. A goal of scientists using the instrument is to learn about
    >the temperatures at which comets form and evolve, by
    >determining the relative abundance of noble gases, such as
    >helium, neon and argon. Principal investigator for the
    >ultraviolet instrument is Dr. Alan Stern of the institute's
    >Space Studies Department in Bolder, Colo.
    >
    >Dr. James Burch, of the Institute's Instrumentation and
    >Space Research Division, San Antonio, is principal
    >investigator for Rosetta's Ion and Electron Spectrometer.
    >This device will measure the environment of charged
    >particles surrounding comet Churyumov-Gerasimenko. It will also study
    >the interaction
    >between that environment and the solar wind of charged
    >particles speeding outward from the Sun.
    >
    >Key electronics for a fourth instrument, the Rosetta Orbiter
    >Spectrometer for Ion and Neutral Analysis, have been
    >supplied by Lockheed Martin Advanced Technology Center, Palo
    >Alto, Calif. This instrument will examine gases surrounding
    >the comet.
    >
    >JPL, a division of the California Institute of Technology in
    >Pasadena, manages the microwave instrument for NASA's Office
    >of Space Science, Washington, D.C.
    >
    >For information about the Rosetta mission visit:
    >
    >http://jpl.convio.net/site/R?i=lvkPT2sX_INO-3BCLCXxIg..
    >
    > -end-
    >
    >

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