This false-color image from a sub-millimeter interferometric telescope shows the circumstellar disk of gas and dust that surrounds star CI Tau. Credit: Stephane Guilloteau/University of Bordeaux
Jupiter-like ‘CI Tau b’ orbits 2 million-year-old star in constellation Taurus. In contradiction to the long-standing idea that larger planets take longer to form, US astronomers today announced the discovery of a giant planet in close orbit around a star so young that it still retains a disk of circumstellar gas and dust.
“For decades, conventional wisdom held that large Jupiter-mass planets take a minimum of 10 million years to form,” said Christopher Johns-Krull. “That’s been called into question over the past decade” CI Tau b is at least 8X larger than Jupiter, ~450 light years from Earth. Earth and the sun are more than 4 billion years old, and while the 3,300-plus catalog of exoplanets includes some older and some younger than Earth, the obstacles to finding planets around newly formed stars are varied and daunting. There are relatively few candidate stars that are young enough, bright enough to view in sufficient detail with existing telescopes and still retain circumstellar disks of gas and dust from which planets form. Stars so young also are often active, with visual outbursts and dimmings, strong magnetic fields and enormous starspots that can make it appear that planets exist where they do not.
Astronomers used the Harlan J. Smith Telescope at the University of Texas at Austin’s McDonald Observatory near Fort Davis, Texas, to search for a planet around star CI Tau. (Image courtesy of Ethan Tweedie Photography) – See more at: http://news.rice.edu/2016/05/26/astronomers-find-giant-planet-around-very-young-star-2/#sthash.DwXT55r9.dpuf
CI Tau b orbits the star CI Tau once every 9 days. The planet was found with the radial velocity method, a planet-hunting technique that relies upon slight variations in the velocity of a star to determine the gravitational pull exerted by nearby planets that are too faint to observe directly with a telescope. The discovery resulted from a survey begun in 2004 of 140 candidate stars in the star-forming region Taurus-Auriga.
“This result is unique because it demonstrates that a giant planet can form so rapidly that the remnant gas and dust from which the young star formed, surrounding the system in a Frisbee-like disk, is still present,” said Lisa Prato of Lowell Observatory. “Giant planet formation in the inner part of this disk, where CI Tau b is located, will have a profound impact on the region where smaller terrestrial planets are also potentially forming.”
Initial optical radial velocity data from McDonald Observatory confirmed that a planet might be present, and the team added photometry measurements from Lowell and 5 years of infrared observations from Hawaii, Kitt Peak and McDonald to rule out the possibility that the optical signal resulted from starspots or another masking phenomenon. The team has examined about half of the young stars in the Taurus-Auriga survey sample, and the data suggests that more planets may be found.
Ours isn’t the only group looking for planets around young stars, and my hope is that astronomers can find enough of them to shed light on some of the nagging questions about planet formation,” Johns-Krull said.”For instance, the ‘brown dwarf desert,’ an unexplained paucity of objects that are larger than giant planets but smaller than stars. If close investigation of young stars reveals more brown dwarfs in short-period orbits than elsewhere, that could confirm the theory that they tend to merge with their central stars within a few million years of forming.” http://news.rice.edu/2016/05/26/astronomers-find-giant-planet-around-very-young-star-2/
Recent Comments