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Planets with double suns are common

Date:
January 12, 2012
Source:
Harvard-Smithsonian Center for Astrophysics
Summary:
Astronomers have discovered two new circumbinary planet systems -- planets that orbit two stars, like Tatooine in the movie Star Wars. Their find, which brings the number of known circumbinary planets to three, shows that planets with two suns must be common, with many millions existing in our galaxy.
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This artist's conception shows Kepler-34b, a newfound gas-giant planet that orbits a double-star system. Its two suns are both yellow, G-type stars that swing around each other every 28 days. The planet circles them both in 289 days. The discovery of Kepler-34b and Kepler-35b shows that circumbinary planets are common in our Galaxy.
Credit: David A. Aguilar (CfA)

Astronomers using NASA's Kepler mission have discovered two new circumbinary planet systems -- planets that orbit two stars, like Tatooine in the movie Star Wars. Their find, which brings the number of known circumbinary planets to three, shows that planets with two suns must be common, with many millions existing in our Galaxy.

"Once again, we're seeing science fact catching up with science fiction," said co-author Josh Carter of the Harvard-Smithsonian Center for Astrophysics.

The work was published online in the journal Nature and presented by lead author William Welsh (San Diego State University) at a meeting of the American Astronomical Society.

The two new planets, named Kepler-34b and Kepler-35b, are both gaseous Saturn-size planets. Kepler-34b orbits its two Sun-like stars every 289 days, and the stars themselves orbit each other every 28 days. Kepler-35b revolves around a pair of smaller stars (80 and 89 percent of the Sun's mass) every 131 days, and the stars orbit one another every 21 days. Both systems reside in the constellation Cygnus the Swan, with Kepler-34 located 4,900 light-years from Earth and Kepler-35 at a distance of 5,400 light-years.

Circumbinary planets have two suns, not just one, and due to the orbital motion of the stars, the amount of energy the planet receives varies greatly. This changing energy flow could produce wildly varying climates.

"It would be like cycling through all four seasons many times per year, with huge temperature changes," explained Welsh. "The effects of these climate swings on the atmospheric dynamics, and ultimately on the evolution of life on habitable circumbinary planets, is a fascinating topic that we are just beginning to explore."

The Kepler team announced the first circumbinary planet, Kepler-16b, last September. Like Kepler-16b, these new planets also transit (eclipse) their host stars, which is how Kepler spotted them. When only Kepler-16b was known, many questions remained about the nature of circumbinary planets; most importantly, was it a fluke? With the discovery of these two new worlds, astronomers can now answer many of those questions as they begin to study an entirely new class of planets.

"It was once believed that the environment around a pair of stars would be too chaotic for a circumbinary planet to form, but now that we have confirmed three such planets, we know that it is possible, if not probable, that there are at least millions in the Galaxy," said Welsh.

"The search is on for more circumbinary planets," agreed Carter, "and we hope to use Kepler for years to come."


Story Source:

The above post is reprinted from materials provided by Harvard-Smithsonian Center for Astrophysics. Note: Materials may be edited for content and length.


Journal Reference:

  1. William F. Welsh, Jerome A. Orosz, Joshua A. Carter, Daniel C. Fabrycky, Eric B. Ford, Jack J. Lissauer, Andrej Prša, Samuel N. Quinn, Darin Ragozzine, Donald R. Short, Guillermo Torres, Joshua N. Winn, Laurance R. Doyle, Thomas Barclay, Natalie Batalha, Steven Bloemen, Erik Brugamyer, Lars A. Buchhave, Caroline Caldwell, Douglas A. Caldwell, Jessie L. Christiansen, David R. Ciardi, William D. Cochran, Michael Endl, Jonathan J. Fortney, Thomas N. Gautier III, Ronald L. Gilliland, Michael R. Haas, Jennifer R. Hall, Matthew J. Holman, Andrew W. Howard, Steve B. Howell, Howard Isaacson, Jon M. Jenkins, Todd C. Klaus, David W. Latham, Jie Li, Geoffrey W. Marcy, Tsevi Mazeh, Elisa V. Quintana, Paul Robertson, Avi Shporer, Jason H. Steffen, Gur Windmiller, David G. Koch, William J. Borucki. Transiting circumbinary planets Kepler-34 b and Kepler-35 b. Nature, 2012; DOI: 10.1038/nature10768

Cite This Page:

Harvard-Smithsonian Center for Astrophysics. "Planets with double suns are common." ScienceDaily. ScienceDaily, 12 January 2012. <www.sciencedaily.com/releases/2012/01/120111154035.htm>.
Harvard-Smithsonian Center for Astrophysics. (2012, January 12). Planets with double suns are common. ScienceDaily. Retrieved July 29, 2015 from www.sciencedaily.com/releases/2012/01/120111154035.htm
Harvard-Smithsonian Center for Astrophysics. "Planets with double suns are common." ScienceDaily. www.sciencedaily.com/releases/2012/01/120111154035.htm (accessed July 29, 2015).

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