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    Home»Space»Rogue Planets Captured by Stars
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    Rogue Planets Captured by Stars

    By Harvard-Smithsonian Center for AstrophysicsApril 17, 2012No Comments4 Mins Read
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    world drifts at the outer edge of a distant star system
    In this artist’s conception, a captured world drifts at the outer edge of a distant star system, so far from its Sun-like host that the star’s disk is barely resolvable at the upper right. New research shows that one in 20 stars within our galaxy might have captured a free-floating planet. Credit: Christine Pulliam (CfA)

    According to a new study set to be published this week, rogue planets might not be alone forever. The study details how rogue planets are occasionally “snagged or grabbed” by stars and possibly by other planets.

    New research suggests that billions of stars in our galaxy have captured rogue planets that once roamed interstellar space. The nomad worlds, which were kicked out of the star systems in which they formed, occasionally find a new home with a different sun. This finding could explain the existence of some planets that orbit surprisingly far from their stars, and even the existence of a double-planet system.

    “Stars trade planets just like baseball teams trade players,” said Hagai Perets of the Harvard-Smithsonian Center for Astrophysics.

    The study, co-authored by Perets and Thijs Kouwenhoven of Peking University, China, will appear in the April 20th issue of The Astrophysical Journal.

    To reach their conclusion, Perets and Kouwenhoven simulated young star clusters containing free-floating planets. They found that if the number of rogue planets equaled the number of stars, then 3 to 6 percent of the stars would grab a planet over time. The more massive a star is, the more likely it is to snag a planet drifting by.

    They studied young star clusters because capture is more likely when stars and free-floating planets are crowded together in a small space. Over time, the clusters disperse due to close interactions between their stars, so any planet-star encounters have to happen early in the cluster’s history.

    Rogue planets are a natural consequence of star formation. Newborn star systems often contain multiple planets. If two planets interact, one can be ejected and become an interstellar traveler. If it later encounters a different star moving in the same direction at the same speed, it can hitch a ride.

    A captured planet tends to end up hundreds or thousands of times farther from its star than Earth is from the Sun. It’s also likely to have an orbit that’s tilted relative to any native planets, and may even revolve around its star backward.

    Astronomers haven’t detected any clear-cut cases of captured planets yet. Imposters can be difficult to rule out. Gravitational interactions within a planetary system can throw a planet into a wide, tilted orbit that mimics the signature of a captured world.

    Finding a planet in a distant orbit around a low-mass star would be a good sign of capture, because the star’s disk wouldn’t have had enough material to form the planet so far out.

    The best evidence to date in support of planetary capture comes from the European Southern Observatory, which announced in 2006 the discovery of two planets (weighing 14 and 7 times Jupiter) orbiting each other without a star.

    “The rogue double-planet system is the closest thing we have to a ‘smoking gun’ right now,” said Perets. “To get more proof, we’ll have to build up statistics by studying a lot of planetary systems.”

    Could our solar system harbor an alien world far beyond Pluto? Astronomers have looked, and haven’t found anything yet.

    “There’s no evidence that the Sun captured a planet,” said Perets. “We can rule out large planets. But there’s a non-zero chance that a small world might lurk on the fringes of our solar system.”

    Reference: “On the Origin of Planets at Very Wide Orbits From the Recapture of Free Floating Planets” by Hagai B. Perets and M. B. N. Kouwenhoven, 17 April 2012, The Astrophysical Journal.
    DOI: 10.1088/0004-637X/750/1/83

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