September 18, 2006
Jupiter-Sized Transiting Planet Found by Astronomers Using Novel Telescope Network
Our home solar system may be down by a planet with the recent demotion of Pluto, but the number of giant planets discovered in orbit around other stars continues to grow steadily. Now, an international team of astronomers has detected a planet slightly larger than Jupiter that orbits a star 500 light-years from Earth in the constellation Draco.
Unlike the mythological names associated with the solar system's planets, the newly discovered planet is known by "TrES-2" and passes in front of the star "GSC 03549-02811" every two and a half days.
The new planet is especially noteworthy because it was identified by astronomers looking for transiting planets (that is, planets that pass in front of their home star) with a network of small automated telescopes. The humble telescopes used in the discovery consist of mostly amateur-astronomy components and off-the-shelf 4-inch camera lenses. This is the third transiting planet found using telescopes similar to those used by many amateur astronomers.
By definition, a transiting planet passes directly between Earth and the star, causing a slight reduction in the light in a manner similar to that caused by the moon's passing between the sun and Earth during a solar eclipse. According to Francis O'Donovan, an Irish graduate student in astronomy at the California Institute of Technology, "When TrES-2 is in front of the star, it blocks off about one and a half percent of the star's light, an effect we can observe with our TrES telescopes.
"We know of about 200 planets around other stars," says O'Donovan, lead author of the paper announcing the discovery in an upcoming issue of the Astrophysical Journal, "but it is only for the nearby transiting planets that we can precisely measure the size and mass of the planet, and hence study its composition. That makes each new transiting planet an exciting find. And because TrES-2 is the most massive of the nearby transiting planets, it sets a new limit to our understanding of how these gas planets form around stars."
The planet TrES-2 is also noteworthy for being the first transiting planet in an area of the sky known as the "Kepler field," which has been singled out as the targeted field of view for the upcoming NASA Kepler mission. Using a satellite-based telescope, Kepler will stare at this patch of sky for four years, and should discover hundreds of giant planets and Earth-like planets. Finding a planet in the Kepler field with the current method allows astronomers to plan future observations with Kepler that include searching for moons around TrES-2.
And finally, the research team hails the discovery as the second transiting "hot Jupiter" found with the Trans-Atlantic Exoplanet Survey (TrES), an effort involving the "Sleuth" telescope at Caltech's Palomar Observatory in San Diego County, the Planet Search Survey Telescope (PSST) at Lowell Observatory near Flagstaff, Arizona, and the "STellar Astrophysics and Research on Exoplanets (Stare) telescope in the Canary Islands. The name of the planet, TrES-2, is derived from the name of the survey.
To look for transits, the small telescopes are automated to take wide-field timed exposures of the clear skies on as many nights as possible. When an observing run is completed for a particular field-usually over an approximate two-month period-the data are run through software that corrects for various sources of distortion and noise.
The end result is a "light curve" for each of thousands of stars in the field. If the software detects regular variations in the light curve for an individual star, then the astronomers do additional work to see if the source of the variation is indeed a transiting planet. One possible alternative is that the object passing in front of the star is another star, fainter and smaller.
In order to confirm they had found a planet, O'Donovan and his colleagues switched from the 10-centimeter TrES telescopes to one of the 10-meter telescopes at the W. M. Keck Observatory on the summit of Mauna Kea, Hawaii. Using this giant telescope, they confirmed that they had found a new planet. O'Donovan says, "Each of us had spent countless hours working on TrES at that point, and we had suffered many disappointments. All our hard work was made worthwhile when we saw the results from our first night's observations, and realized we had found our second transiting planet."
TrES-2 was first spotted by the Sleuth telescope, which was set up by David Charbonneau, formerly an astronomer at Caltech who is now at the Harvard-Smithsonian Center for Astrophysics and is a coauthor of the paper. The PSST, which is operated by Georgi Mandushev and Edward Dunham (coauthors from Lowell Observatory), also observed transits of TrES-2, confirming the initial detections.
The other authors of the paper are David Latham and Guillermo Torres of Harvard-Smithsonian; Alessandro Sozetti of Harvard-Smithsonian and the INAF-Osservatorio Astronomico di Torino; Timothy Brown of the Las Cumbres Observatory Global Telescope; John Trauger of the Jet Propulsion Laboratory; Markus Rabus, José Almenara, Juan Belmonte, and Hans Deeg of the Instituto de Astrofísica de Canarias; Roi Alonso of the Laboratoire d'Astrophysique de Marseille and the Institute de Astrofísica de Canarias; Gilbert Esquerdo of Harvard-Smithsonian and the Planetary Science Institute in Tucson; Emilio Falco of Harvard-Smithsonian; Lynne Hillenbrand of Caltech; Anna Roussanova of MIT; Robert Stefanik of Harvard-Smithsonian; and Joshua Winn of MIT.
Contact: Robert Tindol (626) 395-3631 email@example.com
The above is a reprint of a Caltech press release available at http://pr.caltech.edu/media/Press_Releases/PR12890.html.
The availability of the HPWREN network for data communications to the Calfornia Institute of Technology's Palomar Observatory was critical to this discovery. "Living in the modern age of astronomy has made observing much more efficient. Every night we transfer about 4 gigabytes of data via HPWREN from Sleuth to Caltech in Pasadena. It is on my computer and analyzed before I arrive at work in the morning," says Caltech graduate student Francis O'Donovan. "The ability to process the previous night's data enables us to quickly check the quality of that data. We can then ensure the telescope is operational before beginning the next night's observations."
W. Scott Kardel
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