Автор: Пользователь скрыл имя, 18 Декабря 2010 в 09:09, контрольная работа
Controlling Robots with the Mind. Astronomical hunt ends in success.Augmented Reality: A New Way of Seeing. Atomic memory developed. Examination Topics for Advanced Students.
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-
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http://oposite.stsci.edu/
and via links in
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http://hubble.stsci.edu/
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