>Date: Tue, 27 Nov 2001 12:10:18 -0500 (EST)
>From: [EMAIL PROTECTED]
>Subject: HUBBLE MEASURES ATMOSPHERE ON WORLD AROUND ANOTHER STAR
>Sender: [EMAIL PROTECTED]
>To: undisclosed-recipients:;
>
>Donald Savage
>Headquarters, Washington               Nov. 27, 2001
>(Phone: 202/358-1547)
>
>Nancy Neal
>Goddard Space Flight Center, Greenbelt, Md.
>(Phone: 301/286-0039)
>
>Ray Villard
>Space Telescope Science Institute, Baltimore
>(Phone: 410/338-4514)
>
>RELEASE: 01-232
>
>HUBBLE MEASURES ATMOSPHERE ON WORLD AROUND ANOTHER STAR
>
>      Astronomers using NASA's Hubble Space Telescope have
>made the first direct detection and chemical analysis of the
>atmosphere of a planet outside our solar system. Their unique
>observations demonstrate it is possible with Hubble and other
>telescopes to measure the chemical makeup of extrasolar
>planets' atmospheres and potentially to search for chemical
>markers of life beyond Earth.
>
>The planet orbits a yellow, Sun-like star called HD 209458, a
>seventh-magnitude star (visible in an amateur telescope) that
>lies 150 light-years away in the autumn constellation
>Pegasus. Its atmospheric composition was probed when the
>planet passed in front of its parent star, allowing
>astronomers for the first time ever to see light from the
>star filtered through the planet's atmosphere.
>
>Lead investigator David Charbonneau of the California
>Institute of Technology, Pasadena, and the Harvard-
>Smithsonian Center for Astrophysics, Cambridge, Mass.;
>Timothy Brown of the National Center for Atmospheric
>Research, Boulder, Colo.; and colleagues used Hubble's
>spectrometer (the Space Telescope Imaging Spectrograph, or
>STIS) to detect the presence of sodium in the planet's
>atmosphere.
>
>"This opens up an exciting new phase of extrasolar planet
>exploration, where we can begin to compare and contrast the
>atmospheres of planets around other stars," says Charbonneau.
>The astronomers actually saw less sodium than predicted for
>the Jupiter-class planet, leading to one interpretation that
>high-altitude clouds in the alien atmosphere may have blocked
>some of the light. The team's findings are to be published in
>the Astrophysical Journal.
>
>The Hubble observation was not tuned to look for gases
>expected in a life-sustaining atmosphere (which is improbable
>for a planet as hot as the one observed). Nevertheless, this
>unique observing technique opens a new phase in the
>exploration of exoplanets, or extrasolar planets, say
>astronomers. Such observations could potentially provide the
>first direct evidence for life beyond Earth by measuring
>unusual abundances of atmospheric gases caused by the
>presence of living organisms.
>
>The planet was discovered in 1999 through its slight
>gravitational tug on the star. The planet was estimated to be
>70 percent the mass of the giant planet Jupiter, or 220 times
>more massive than Earth. Subsequently, astronomers discovered
>that the tilt of the planet's orbit makes it pass in front of
>the star -- relative to our line-of-sight from Earth --
>making it unique among all the approximately 80 extrasolar
>planets discovered to date. As the planet passes in front of
>the star, it causes the star to dim very slightly for the
>duration of the transit. Transit observations by Hubble and
>ground-based telescopes confirmed that the planet is
>primarily gaseous, rather than liquid or solid, meaning that
>the planet is a gas giant, like Jupiter and Saturn.
>
>The planet is an ideal target for repeat observations because
>it transits the star every 3.5 days -- which is the extremely
>short time it takes the planet to whirl around the star at a
>distance of merely four million miles from the star's
>surface. This close proximity heats the planet's atmosphere
>to a torrid 2,000 degrees Fahrenheit (1,100 degrees Celsius).
>
>Observations of four separate transits were made by Hubble in
>search of direct evidence of an atmosphere. During each
>transit a small fraction of the star's light on its way to
>Earth passed though the planet's atmosphere. When the color
>of the light was analyzed by STIS, the telltale "fingerprint"
>of sodium was detected. Though the star also has sodium in
>its outer layers, STIS precisely measured the added influence
>of sodium in the planet's atmosphere.
>
>The team, including Robert Noyes of the Harvard-Smithsonian
>Center for Astrophysics and Ronald Gilliland of the Space
>Telescope Science Institute in Baltimore, plans to look at HD
>209458 again with Hubble in other colors of the star's
>spectrum to see which are filtered by the planet's
>atmosphere. They hope eventually to detect methane, water
>vapor, potassium and other chemicals in the planet's
>atmosphere. Once other transiting giants are found in the
>next few years, the team expects to characterize chemical
>differences among the atmospheres of these planets.
>
>The Space Telescope Science Institute (STScI) is operated by
>the Association of Universities for Research in Astronomy,
>Inc. (AURA), for NASA, under contract with the Goddard Space
>Flight Center, Greenbelt, Md. The Hubble Space Telescope is a
>project of international co-operation between NASA and the
>European Space Agency (ESA). The National Center for
>Atmospheric Research is sponsored primarily by the National
>Science Foundation.
>
>                           -end-
>NOTE TO EDITORS: Electronic images, illustrations, animations
>and additional information are available at:
>http://oposite.stsci.edu/pubinfo/pr/2001/38
>and via links in
>http://oposite.stsci.edu/pubinfo/latest.html
>http://oposite.stsci.edu/pubinfo/pictures.html
>http://hubble.stsci.edu/go/news
>
>
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