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GAINESVILLE, Fla. — Using the world’s largest optical telescope, a
team of University of Florida
astronomers has pioneered a new method of observing planets outside our
solar system. The method suggests that large Earth-based telescopes
could play a leading role in rapidly accelerating research on
“extrasolar” planets.
The results obtained from the Gran
Telescopio Canarias, a telescope in Spain’s Canary Islands
partially owned by the University of Florida, are of such high precision
that the astronomers are already planning to use the technique to learn
more about “super-Earth-sized” planets – larger than Earth but smaller
than Neptune – that have already been identified by space-based
observatories.
The astronomers used the technique to study two giant, previously
discovered planets passing in front of their parent stars. It minimized
the atmosphere’s distortion of starlight by measuring the light received
within a small range of colors. The tunable filters of the
Spanish-built instrument OSIRIS, the first instrument to be mounted on
the Gran Telescopio Canarias, or GTC, allowed the spectrum to be
“dissected” precisely.
“We want to explore the unique features of OSIRIS on the world’s
biggest telescope, so we’re developing new ways to observe with its
filters,” said Eric Ford,
a UF assistant professor of astronomy and co-author of an article on
the research that appeared online Wednesday and will be published in the
Monthly Notices of the Royal Astronomical Society.
Even though observing a restricted range of colors limits the amount
of light available, Ford said, “the GTC is big enough and its
instrumentation is so advanced that we can still collect sufficient
light from the stars and measure their brightness precisely.”
The results show that the precision obtained was “excellent,” in
Ford’s words, and was hardly affected by the atmosphere. The extrasolar
planets, called TrES-2b and TrES-3b, were observed in June and August of
last year.
Ford said the new technique does not replace existing methods to
search for planets, but rather provides new information about planets
that pass in front of their parent stars, and have already been
discovered by other observatories such as NASA’s Kepler space telescope.
Its main virtue is that it provides better measurements of the planets’
orbits and the chemical composition of their atmospheres.
Given the growing number of extrasolar planets being detected, the
researchers are confident this new technique will be a powerful new tool
for learning about distant planets and how they differ from Earth.
Knicole Colón, lead author of the article and a UF graduate student
in astronomy, said she is “optimistic that these techniques will become
much more common in the future as astronomers seek ways of improving the
precision of observations when studying Neptune-like and super-Earth
sized planets discovered by space missions.”
The GTC began scientific observations in 2009 after nine years under
construction. UF, which owns a 5 percent share, is the only U.S.
institution with part ownership of the telescope.
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