Astronomy

AN EXOPLANET ORBITING THREE STARS?

Astronomer­s may have found the first planet that orbits a trio of suns.

- — ALISON KLESMAN

Some 1,300 light-years away in the constellat­ion Orion the Hunter is the triple-star system GW Orionis. This trio of young stars is only about 1 million years old and still surrounded by a disk of dust and gas left over from their formation. This socalled protoplane­tary disk is organized into three concentric rings, none of which are aligned with any of the orbits of the three stars. Additional­ly, the innermost ring is out of alignment with the outer two rings; it also tilts and wobbles as it orbits. And there’s a large gap between the inner and middle rings, indicating the material there has been cleared out.

A paper published Sept. 17 in Monthly Notices of the Royal Astronomic­al Society suggests the reason for that last oddity is a so-called circumtrip­le planet (or planets) forming within the disk, orbiting all three stars at once and clearing out material to form the gap.

MAKING SPACE

Gaps in protoplane­tary disks often indicate where planets are forming within them. As a planet pulls in nearby gas and dust to grow, it clears out its surroundin­gs. But in this case, researcher­s weren’t sure whether the disk’s behavior should be attributed to a fledgling planet or the three stars whirling in a complex dance at its center.

They found, based on 3D modeling, that the stars’ gravity can’t produce enough torque to create the observed gap. Instead, the researcher­s say, it is likely due to at least one Jupiter-sized planet forming there. If confirmed, it would be the first exoplanet found orbiting three stars. (Although planets have been found in nearly 30 triple systems to date, none of these other worlds orbit all three stars.)

The supposed planet orbits about

100 astronomic­al units (AU) from the center, where 1 AU is the average EarthSun distance. The stars themselves are much closer: Two orbit each other separated by just 1 AU, while the third orbits both of these some 8 AU from the system’s center.

Because this research only provides indirect evidence for the planet, the next step is actually spotting the strange world. Unfortunat­ely, the authors conclude, that’s tricky in a system this complex. Still, more observatio­ns are coming down the pike, which may yet reveal a glimpse of a truly unique young world.

 ?? ALMA (ESO/NAOJ/NRAO), ESO/EXETER/KRAUS ET AL. ?? COMPLEX RINGS. The image at left, taken with the ALMA radio array, shows rings and gaps in the massive disk around GW Orionis. At right, a SPHERE image shows how the disk’s inner region is warped and twisted; the dark spot at center is the shadow of the inner ring.
ALMA (ESO/NAOJ/NRAO), ESO/EXETER/KRAUS ET AL. COMPLEX RINGS. The image at left, taken with the ALMA radio array, shows rings and gaps in the massive disk around GW Orionis. At right, a SPHERE image shows how the disk’s inner region is warped and twisted; the dark spot at center is the shadow of the inner ring.

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