
Most of the planets astronomers have found orbit only one star – a few orbit two, but so far we’ve never spotted an exoplanet that orbits three stars simultaneously. Now, researchers have spotted hints of a young world with three host stars.
These hints come from a stellar system called GW Orionis, which consists of two stars orbiting one another at about the same distance that Earth sits from the sun, and a third circling those two about eight times further away. Encircling this system is a disc of dust and gas separated into three rings.
There is a huge gap – about 15 billion kilometres across – between the innermost ring and the other two. Some astronomers have interpreted this gap as having formed when the torque from the three stars’ gravity ripped the disc apart, but through a series of simulations, at the University of Nevada, Las Vegas, and his colleagues have determined that it’s more likely a planet carved it out.
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They performed a set of 11 simulations of the stars, including the gas in the disc – the dust in the disc is expected to follow the structure of the gas. Without a giant planet, torque from the stars didn’t rip the disc apart into separate rings, but inserting a planet about the size of Jupiter reproduced the observed gap. When the gap filled in over time, the planet simply carved a new one.
“We haven’t observed the planet directly, but there is some evidence that a planet is shaping this gap,” says Smallwood. If it is there, this would be the first world ever found that orbits three stars, and there may even be a second, smaller planet between the outer two rings.
However, confirming this will be difficult, he says. The larger purported world would be far away from the stars and have a tilted orbit, making it hard to detect using the usual method, which relies on a planet passing in front of a star and blocking out some of its light. The best way to confirm the planet’s existence would be taking a direct image of it, but the system is more than 1000 light years from Earth, so that would be tough, too.
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