Tuesday, July 23, 2019

Magnetic Activity in 'Hot Jupiter' Exoplanets Wildly Powerful, Twist and Shape Stars



Gas-giant planets orbiting close to other stars have powerful magnetic fields, many times stronger than our own Jupiter, according to a new study by a team of astrophysicists. It is the first time the strength of these fields has been calculated from observations.

The team, led by Wilson Cauley of the University of Colorado, also includes associate professor Evgenya Shkolnik of Arizona State University's School of Earth and Space Exploration. The other researchers are Joe Llama of Northern Arizona University and Antonino Lanza of the Astrophysical Observatory of Catania in Italy. Their report was published July 22 in Nature Astronomy.

This illustration shows a hot Jupiter orbiting so close to a red dwarf star that the magnetic fields of both interact, triggering activity on the star. Astrophysicists have for the first time used observations of such activity to calculate field strengths in four hot Jupiter star-and-planet systems.
 Image credit: NASA, ESA and A. Schaller (for STScI) 

"Our study is the first to use observed signals to derive exoplanet magnetic field strengths," said Shkolnik. "These signals appear to come from interactions between the magnetic fields of the star and the tightly orbiting planet."
Many worlds

More than 3,000 exoplanet systems containing over 4,000 planets have been discovered since 1988. Many of these star systems include what astronomers call "hot Jupiters." These are massive gaseous planets presumed to be like the sun's Jupiter but orbiting their stars at close distances, typically about five times the star's diameter, or roughly 20 times the moon's distance from Earth.

Such planets travel well inside their star's magnetic field, where interactions between the planetary field and the stellar one can be continual and strong.

Previous studies, the team says, have placed upper limits on exoplanet magnetic fields, for example from radio observations or derived purely from theory.

"We combined measurements of increased stellar emission from the magnetic star-planet interactions together with physics theory to calculate the magnetic field strengths for four hot Jupiters," lead author Cauley said.

The magnetic field strengths the team found range from 20 to 120 gauss. For comparison, Jupiter’s magnetic field is 4.3 gauss and Earth's field strength is only half a gauss, although that is strong enough to orient compasses worldwide.

Hot Jupiters (red dots) are large planets similar to our Jupiter, but orbiting close to their stars. Four hot Jupiters have magnetic field strengths much greater than that of Earth, Saturn, Uranus or Neptune — or even Jupiter itself. The left scale shows field strength in gauss, the bottom scale shows orbital distance from the star in astronomical units; Earth orbits the sun at 1 AU.


Credit: Wilson Cauley/University of Colorado

This simulation shows how a hot Jupiter's magnetic field would interact with its host star's magnetic field. The new study found such interactions are enhanced because at least four hot Jupiters have larger calculated magnetic field strengths than previously thought.

Triggering activity

The astrophysicists used telescopes in Hawaii and France to acquire high-resolution observations of emission from ionized calcium (Ca II) in the parent stars of the four hot Jupiters. The emission comes from a star's hot, magnetically heated chromosphere, a thin layer of gas above the cooler stellar surface. The observations let the team calculate how much energy was being released in the stars' calcium emission.

Said Shkolnik, "We used the power estimates to calculate magnetic field strengths for the planets using a theory for how the planets' magnetic fields interact with the stellar magnetic fields."

Cauley explained, "Magnetic fields like to be in a state of low energy. If you twist or stretch the field like a rubber band, this increases the energy stored in the magnetic field." Hot Jupiters orbit very close to their parent stars and so the planet's magnetic field can twist and stretch the star's magnetic field.

Credit: Antoine Strugarek/CEA Saclay/Université de Montréal



"When this happens," Cauley said, "energy can be released as the two fields reconnect, and this heats the star's atmosphere, increasing the calcium emission."
Probing deep

Astrophysicists have suspected that hot Jupiters would, like our own Jupiter, have magnetic fields produced deep inside them. The new observations provide the first probe of the internal dynamics of these massive planets.

"This is the first estimate of the magnetic field strengths for these planets based on observations, so it's a huge jump in our knowledge," Shkolnik noted. "It's giving us a better understanding of what is happening inside these planets."

She adds that it should also help researchers who model the internal dynamos of hot Jupiters. "We knew nothing about their magnetic fields — or any other exoplanet magnetic fields — and now we have estimates for four actual systems."

Surprisingly powerful

The field strengths, the team says, are larger than one would expect considering only the rotation and age of the planet. The standard dynamo theory of planetary magnetic fields predicts field strengths for the sampled planets that are much smaller than what the team found.

Instead, the observations support the idea that planetary magnetic fields depend on the amount of heat moving through the planet's interior. Because they are absorbing a lot of extra energy from their host stars, hot Jupiters should have larger magnetic fields than planets of similar mass and rotation rate.

"We are pleased to see how well the magnitude of the field values corresponded to those predicted by the internal heat flux theory," Shkolnik said. "This may also help us work toward a clearer understanding of magnetic fields around temperate rocky planets."




Contacts and sources:
Robert Burnham
Arizona State University

Citation: Magnetic field strengths of hot Jupiters from signals of star–planet interactions.
P. Wilson Cauley, Evgenya L. Shkolnik, Joe Llama, Antonino F. Lanza.Nature Astronomy, 2019; DOI: 10.1038/s41550-019-0840-x



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