'Hot Jupiters' provoke their own host suns to wobble

'Hot Jupiters' provoke their own host suns to wobble
Credit: Cornell University

Blame the "hot Jupiters." These large, gaseous exoplanets (planets outside our solar system) can make their suns wobble when they wend their way through their own solar systems to snuggle up against their suns, according to new Cornell University research to be published in Science, Sept. 11.

"Although the planet's mass is only one-thousandth of the mass of the sun, the stars in these other solar systems are being affected by these and making the stars themselves act in a crazy way," said Dong Lai, Cornell professor of astronomy and senior author on the research, "Chaotic Dynamics of Stellar Spin in Binaries and the Production of Misaligned Hot Jupiters." Physics graduate student Natalia I. Storch (lead author) and astronomy graduate student Kassandra R. Anderson are co-authors.

In our , the sun's rotation axis is approximately aligned with the orbital axis of all the planets. The orbital axis is perpendicular to the flat plane in which the planets revolve around the sun. In solar systems with hot Jupiters, recent observations have revealed that the orbital axis of these planets is misaligned with the of their host star. In the last few years, astronomers have been puzzled by spin-orbit misalignment between the star and the planets.

Roasting like marshmallows on an open fire, hot Jupiters – large gaseous planets dispensed throughout the universe in other solar systems – wander from distant places to orbit extraordinarily close to their own suns. Partner binary stars, some as far as hundreds of astronomical units (an astronomical unit is 93 million miles, the distance between Earth and the sun,) influence through gravity the giant Jupiter-like planets and cause them to falter into uncommon orbits; that, in turn, causes them to migrate inward close to their sun, Lai said.

"When exoplanets were first found in the 1990s, it was large planets like Jupiter that were discovered. It was surprising that such can be so close to parent star," Lai said. "Our own planet Mercury is very close to our sun. But these hot Jupiters are much closer to their suns than Mercury."

By simulating the dynamics of these exotic planetary systems, the Cornell astronomers showed that when the Jupiter-like planet approaches its host star, the planet can force the star's spin axis to precess (that is, change the orientation of their rotational axis), much like a wobbling, spinning top.

"Also, it can make the star's change direction in a rather complex – or even a chaotic – way," said Lai. "This provides a possible explanation to the observed spin-orbit misalignments, and will be helpful for understanding the origin of these enigmatic planets."

Another interesting feature of the Cornell work is that the chaotic variation of the star's spin resembles other chaotic phenomena found in nature, such as weather and climate.


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More information: "Chaotic dynamics of stellar spin in binaries and the production of misaligned hot Jupiters" Science, 2014. www.sciencemag.org/lookup/doi/ … 1126/science.1254358
Journal information: Science

Provided by Cornell University
Citation: 'Hot Jupiters' provoke their own host suns to wobble (2014, September 11) retrieved 27 May 2019 from https://phys.org/news/2014-09-hot-jupiters-provoke-host-suns.html
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Sep 12, 2014
Yeah... that's how we find'em, thank you. Great news...

Sep 12, 2014
Most likely these planets in highly elliptical and inclined orbits were not formed from the same cloud as the stars they orbit. A random encounter resulting in an inelastic gravitational interaction (tidal forces created that dissipate orbital energy) that allows the star to capture the planet could easily account for the uncorrelated axes of rotation/revolution.

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