Andrew Yee
February 24th 06, 04:02 AM
Nancy Neal-Jones (301) 286-0039
Bill Steigerwald (301) 286-5017
Goddard Space Flight Center, Greenbelt, Md.
Whitney Clavin (818) 354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
For Release: February 21, 2006
ssc2006-07
NASA's Spitzer Makes Hot Alien World the Closest Directly Detected
A NASA-led team of astronomers have used NASA's Spitzer Space Telescope to
detect a strong flow of heat radiation from a toasty planet orbiting a
nearby star. The findings allowed the team to "take the temperature" of
the planet.
"This is the closest extrasolar planet to Earth that has ever been
detected directly, and it presents the strongest heat emission ever seen
from an exoplanet," said Drake Deming of NASA's Goddard Space Flight
Center, Greenbelt, Md. Deming is the lead author of a paper on this
observation to be published in the Astrophysical Journal on June 10. An
advance copy of the paper will be posted on the astro-ph website on Feb.
22 [http://arxiv.org/abs/astro-ph/0602443].
The planet "HD 189733b" orbits a star that is a near cosmic neighbor to
our sun, at a distance of 63 light years in the direction of the Dumbbell
Nebula. It orbits the star very closely, just slightly more than three
percent of the distance between Earth and the sun. Such close proximity
keeps the planet roasting at about 844 Celsius (about 1,551 Fahrenheit),
according to the team's measurement.
The planet was discovered last year by François Bouchy of the Marseille
Astrophysics Laboratory, France, and his team. The discovery observations
allowed Bouchy's team to determine the planet's size (about 1.26 times
Jupiter's diameter), mass (1.15 times Jupiter), and density (about 0.75
grams per cubic centimeter). The low density indicates the planet is a gas
giant like Jupiter.
The observations also revealed the orbital period (2.219 days) and the
distance from the parent star. From this distance and the temperature of
the parent star, Bouchy's team estimated the planet's temperature was at
least several hundred degrees Celsius, but they were not able to measure
heat or light emitted directly from the planet.
"Our direct measurement confirms this estimate," said Deming. This
temperature is too high for liquid water to exist on the planet or any
moons it might have. Since known forms of life require liquid water, it is
unlikely to have emerged there.
Last year, Deming's team and another group based at the
Harvard-Smithsonian Center for Astrophysics used Spitzer to make the first
direct detection of light from alien worlds, by observing the warm
infrared glows of two other previously detected "Hot Jupiter" planets,
designated HD 209458b and TrES-1.
Infrared light is invisible to the human eye, but detectable by special
instruments. Some infrared light is perceived as heat. Hot Jupiter planets
are alien gas giants that zip closely around their parent stars, like HD
189733b. From their close orbits, they soak up ample starlight and shine
brightly in infrared wavelengths.
Deming's team used the same method to observe HD 189733b. To distinguish
the planet's glow from its hot parent star, the astronomers used an
elegant method. First, they used Spitzer to collect the total infrared
light from both the star and its planet. Then, when the planet dipped
behind the star as part of its regular orbit, the astronomers measured the
infrared light coming from just the star. This pinpointed exactly how much
infrared light belonged to the planet. Under optimal circumstances this
same method can be used to make a crude temperature map of the planet
itself.
"The heat signal from this planet is so strong that Spitzer was able to
resolve its disk, in the sense that our team could tell we were seeing a
round object in the data, not a mere point of light," said Deming. "The
current Spitzer observations cannot yet make a temperature map of this
world, but more observations by Spitzer or future infrared telescopes in
space may be able to do that."
Deming's team includes Joseph Harrington, Cornell University, Ithaca,
N.Y.; Sara Seager, Carnegie Institution of Washington; and Jeremy
Richardson, NASA Postdoctoral Fellow at Goddard, in the Exoplanets and
Stellar Astrophysics Laboratory.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer
Space Telescope mission for the agency's Science Mission Directorate.
Science operations are conducted at the Spitzer Science Center at Caltech.
JPL is a division of Caltech.
Bill Steigerwald (301) 286-5017
Goddard Space Flight Center, Greenbelt, Md.
Whitney Clavin (818) 354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
For Release: February 21, 2006
ssc2006-07
NASA's Spitzer Makes Hot Alien World the Closest Directly Detected
A NASA-led team of astronomers have used NASA's Spitzer Space Telescope to
detect a strong flow of heat radiation from a toasty planet orbiting a
nearby star. The findings allowed the team to "take the temperature" of
the planet.
"This is the closest extrasolar planet to Earth that has ever been
detected directly, and it presents the strongest heat emission ever seen
from an exoplanet," said Drake Deming of NASA's Goddard Space Flight
Center, Greenbelt, Md. Deming is the lead author of a paper on this
observation to be published in the Astrophysical Journal on June 10. An
advance copy of the paper will be posted on the astro-ph website on Feb.
22 [http://arxiv.org/abs/astro-ph/0602443].
The planet "HD 189733b" orbits a star that is a near cosmic neighbor to
our sun, at a distance of 63 light years in the direction of the Dumbbell
Nebula. It orbits the star very closely, just slightly more than three
percent of the distance between Earth and the sun. Such close proximity
keeps the planet roasting at about 844 Celsius (about 1,551 Fahrenheit),
according to the team's measurement.
The planet was discovered last year by François Bouchy of the Marseille
Astrophysics Laboratory, France, and his team. The discovery observations
allowed Bouchy's team to determine the planet's size (about 1.26 times
Jupiter's diameter), mass (1.15 times Jupiter), and density (about 0.75
grams per cubic centimeter). The low density indicates the planet is a gas
giant like Jupiter.
The observations also revealed the orbital period (2.219 days) and the
distance from the parent star. From this distance and the temperature of
the parent star, Bouchy's team estimated the planet's temperature was at
least several hundred degrees Celsius, but they were not able to measure
heat or light emitted directly from the planet.
"Our direct measurement confirms this estimate," said Deming. This
temperature is too high for liquid water to exist on the planet or any
moons it might have. Since known forms of life require liquid water, it is
unlikely to have emerged there.
Last year, Deming's team and another group based at the
Harvard-Smithsonian Center for Astrophysics used Spitzer to make the first
direct detection of light from alien worlds, by observing the warm
infrared glows of two other previously detected "Hot Jupiter" planets,
designated HD 209458b and TrES-1.
Infrared light is invisible to the human eye, but detectable by special
instruments. Some infrared light is perceived as heat. Hot Jupiter planets
are alien gas giants that zip closely around their parent stars, like HD
189733b. From their close orbits, they soak up ample starlight and shine
brightly in infrared wavelengths.
Deming's team used the same method to observe HD 189733b. To distinguish
the planet's glow from its hot parent star, the astronomers used an
elegant method. First, they used Spitzer to collect the total infrared
light from both the star and its planet. Then, when the planet dipped
behind the star as part of its regular orbit, the astronomers measured the
infrared light coming from just the star. This pinpointed exactly how much
infrared light belonged to the planet. Under optimal circumstances this
same method can be used to make a crude temperature map of the planet
itself.
"The heat signal from this planet is so strong that Spitzer was able to
resolve its disk, in the sense that our team could tell we were seeing a
round object in the data, not a mere point of light," said Deming. "The
current Spitzer observations cannot yet make a temperature map of this
world, but more observations by Spitzer or future infrared telescopes in
space may be able to do that."
Deming's team includes Joseph Harrington, Cornell University, Ithaca,
N.Y.; Sara Seager, Carnegie Institution of Washington; and Jeremy
Richardson, NASA Postdoctoral Fellow at Goddard, in the Exoplanets and
Stellar Astrophysics Laboratory.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer
Space Telescope mission for the agency's Science Mission Directorate.
Science operations are conducted at the Spitzer Science Center at Caltech.
JPL is a division of Caltech.