The Very Large Telescope detects first superstorm on exoplanet
The observations also allow another exciting "first" — measuring the orbital speed of the exoplanet itself.
June 23, 2010
Provided by ESO, Garching, Germany
June 23, 2010
This artist's impression shows the Jupiter-like transiting planet around its solar-like host star.
Photo by ESO/L. Calçada
Astronomers have measured a superstorm for the first time in the atmosphere of an exoplanet, "hot Jupiter" HD209458b. The high-precision observations of carbon monoxide gas show that it is streaming at enormous speed from the extremely hot dayside to the cooler nightside of the planet. The observations also allow another exciting "first" — measuring the orbital speed of the exoplanet itself, providing a direct determination of its mass.
"HD209458b is definitely not a place for the faint-hearted," said Ignas Snellen from Leiden Observatory in The Netherlands. "By studying the poisonous carbon monoxide gas with great accuracy, we found evidence for a super wind blowing at a speed of 3,100 to 6,200 mph (5,000 to 10,000 km/h)."
HD209458b is an exoplanet of about 60 percent the mass of Jupiter orbiting a solar-like star located 150 light-years from Earth toward the constellation Pegasus the Winged Horse. Circling at a distance of only one-twentieth the Sun-Earth distance, the planet is heated intensely by its parent star, and it has a surface temperature of about 1800° Fahrenheit (1000° Celsius) on the hot side. But as the planet always has the same side to its star, one side is very hot while the other is much cooler. "On Earth, big temperature differences inevitably lead to fierce winds, and as our new measurements reveal, the situation is no different on HD209458b," said Simon Albrecht from the Massachusetts Institute of Technology (MIT) in Cambridge.
HD209458b was the first exoplanet to be found transiting its sun — every 3.5 days, the planet moves in front of its host star, blocking a small portion of the starlight during a 3-hour period. During such an event, a tiny fraction of the starlight filters through the planet's atmosphere, leaving an imprint. A team of astronomers from Leiden University, the Netherlands Institute for Space Research (SRON), and MIT in the United States, have used the European Southern Observatory's (ESO) Very Large Telescope (VLT) and its powerful CRIRES spectrograph to detect and analyze these faint fingerprints, observing the planet for about 5 hours as it passed in front of its star. "CRIRES is the only instrument in the world that can deliver spectra that are sharp enough to determine the position of the carbon monoxide lines at a precision of 1 part in 100,000," said Remco de Kok from SRON in The Netherlands. "This high precision allows us to measure the velocity of the carbon monoxide gas for the first time using the Doppler effect."
The astronomers achieved several other firsts. They directly measured the velocity of the exoplanet as it orbits its home star. "In general, the mass of an exoplanet is determined by measuring the wobble of the star and assuming a mass for the star, according to theory," said Ernst de Mooij from Leiden Observatory in The Netherlands. "Here, we have been able to measure the motion of the planet as well, and thus determine both the mass of the star and of the planet."
Also for the first time, the astronomers measured how much carbon is present in the atmosphere of this planet. "It seems that H209458b is actually as carbon-rich as Jupiter and Saturn," said Snellen. "This could indicate that it was formed in the same way. In the future, astronomers may be able to use this type of observation to study the atmospheres of earthlike planets to determine whether life also exists elsewhere in the universe."