Fifteen years ago, Geneva Observatory researchers Michel Mayor and Didier Queloz discovered a planet more massive than Jupiter circling a mere 5 million miles (8 million km) from the Sunlike star 51 Pegasi.
Dynamicists have struggled to understand how this and the many other “hot Jupiters” found since then managed to orbit so tightly without being gobbled up. Some were perhaps flung into their star-skirting orbits after losing tugs-of-war with other massive planets in their systems, and some were probably dragged inward along with the natal disks of matter around their young Suns. After the disks dissipated, these massive worlds were deposited in precarious but seemingly stable orbits
There they might remain, roasting for eons, were it not for the tides these close-in planets incite in their stars. For some, long-term survival is not in the cards.
Why so? Consider how the Moon raises tides in Earth’s oceans. Because our satellite takes a month to complete one orbit, whereas Earth spins in just 24 hours, the exchange of tidal energy is a net gain for the Moon, which is edging ever farther from Earth.
But a hot Jupiter completes its orbit in a few days — sometimes in less than 24 hours — creating stellar tides that have the opposite effect. Slowly, inexorably, the planet is dragged to its doom.
That’s the fate of OGLE-TR-113b, a hottie with 1.3 times Jupiter’s mass crowding a Sunlike star 1,800 light-yeas away in Carina. Because it transits, or passes directly in front of its star, astronomers can time the planet’s orbital period exactly. (TR in its designation is for transit; OGLE stands for Optical Gravitational Lensing Experiment.)
As Elisabeth Adams told a meeting of planetary scientists on Friday, precise timing of six such transits over the past few years reveals that OGLE-TR-113b’s 34⅓-hour orbital period does seem to be very gradually shrinking. Using the timings she and her observing team made with the 6.5-m Magellan Telescopes in 2007-09, Adams finds that OGLE-TR-113b shaves about 60 milliseconds off its period each year.
It’s possible, she notes, that the system contains a massive but as-yet unseen companion that’s yanking the planet around. Some kind of librating resonance with a second planet isn’t out of the question either, though the perturber couldn’t have more than twice Earth’s mass. Instead, the simplest explanation is that astronomers have, for the first time, captured a hot Jupiter in its death spiral.
So when might we kiss OGLE-TR-113b good-bye? Adams emphasizes that it’ll happen long before the planet actually reaches the star’s surface. Rather, the point of no return occurs when the orbital period shrinks to 10.8 hours. By then the planet will be close enough for tidal forces to rip it apart. Depending on assumptions about how strongly the star and planet are interacting, the end could come only 1½ to 2 million years from now.
“This detection is still quite tentative,” writes the team in a paper submitted to the Astrophysical Journal, in part because there’s a less-than-perfect fit to other timings made in 2002 and 2006. Clarity should come early next year, when OGLE-TR-113b again becomes observable and more transits can be clocked.
“Other people have been on this trail,” Adams adds, with the hot Jupiter OGLE-TR-56b also getting special attention. Discovered in 2002 and orbiting just 2.1 million miles (3.4 million km) from its stellar host, it might meet its doom in as little as a million years.