平特五不中

The hottest point on a gaseous planet near a distant star isn鈥檛 where astrophysicists expected it to be 鈥� a discovery that challenges scientists鈥� understanding of the many planets of this type found in solar systems outside our own.

Unlike our familiar planet Jupiter, so-called hot Jupiters circle astonishingly close to their host star -- so close that it typically takes fewer than three days to complete an orbit.听 And one hemisphere of these planets always faces its host star, while the other faces permanently out into the dark.

Not surprisingly, the 鈥渄ay鈥� side of the planets gets vastly hotter than the night side, and the hottest point of all tends to be the spot closest to the star. Astrophysicists theorize and observe that these planets also experience strong winds blowing eastward near their equators, which can sometimes displace the hot spot toward the east.

In the mysterious case of exoplanet CoRoT-2b, however, the hot spot turns out to lie in the opposite direction: west of center.听 A research team led by astronomers at 平特五不中鈥檚 平特五不中 Space Institute (MSI) and the Institute for research on exoplanets (iREx) in Montreal made the discovery using NASA鈥檚 Spitzer Space Telescope. Their findings are reported Jan. 22 in the journal Nature Astronomy.

Wrong-way wind

鈥淲e鈥檝e previously studied nine other hot Jupiter, giant planets orbiting super close to their star. In every case, they have had winds blowing to the east, as theory would predict,鈥� says 平特五不中 astronomer Nicolas Cowan, a co-author on the study and researcher at MSI and iREx. 鈥淏ut now, nature has thrown us a curveball. On this planet, the wind blows the wrong way. Since it鈥檚 often the exceptions that prove the rule, we are hoping that studying this planet will help us understand what makes hot Jupiters tick."

CoRoT-2b, discovered a decade ago by a French-led space observatory mission, is 930 light years from Earth. While many other hot Jupiters have been detected in recent years, CoRoT-2b has continued to intrigue astronomers because of two factors: its inflated size and the puzzling spectrum of light emissions from its surface.

鈥淏oth of these factors suggest there is something unusual happening in the atmosphere of this hot Jupiter,鈥� says Lisa Dang, a 平特五不中 PhD student and lead author of the new study. By using Spitzer's Infrared Array Camera to observe the planet while it completed an orbit around its host star, the researchers were able to map the planet鈥檚 surface brightness for the first time, revealing the westward hot spot.听

New questions

The researchers offer three possible explanations for the unexpected discovery 鈥� each of which raises new questions:

• The planet could be spinning so slowly that one rotation takes longer than a full orbit of its star; this could create winds blowing toward the west rather than the east 鈥� but it would also undercut theories about planet-star gravitational interaction in such tight orbits.
• The planet鈥檚 atmosphere could be interacting with the planet鈥檚 magnetic field to modify its wind pattern; this could provide a rare opportunity to study an exoplanet鈥檚 magnetic field.
• Large clouds covering the eastern side of the planet could make it appear darker than it would otherwise 鈥� but this would undercut current models of atmospheric circulation on such planets.

"We鈥檒l need better data to shed light on the questions raised by our finding,鈥� Dang says. 鈥淔ortunately, the James Webb Space Telescope, scheduled to launch next year, should be capable of tackling this problem. Armed with a mirror that has 100 times the collecting power of Spitzer鈥檚, it should provide us with exquisite data like never before."

Scientists from the University of Michigan, the California Institute of Technology, Arizona State University, New York University Abu Dhabi, the University of California, Santa Cruz, and Pennsylvania State University also contributed to the study.

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鈥淒etection of a westward hotspot offset in the atmosphere of hot gas giant CoRoT-2b,鈥� Lisa Dang, Nicolas B. Cowan, Joel C. Schwartz, et al. Nature Astronomy, Jan. 22, 2018.

Funding for the research was provided in part by the Natural Sciences and Engineering Research Council of Canada and the California Institute of Technology鈥檚 Infrared Processing and Analysis Center.

IMAGE:听Artist鈥檚 concept shows the gaseous exoplanet CoRoT-2b with a westward hot spot in orbit around its host star.
CREDIT:听NASA/JPL-Caltech/T. Pyle (IPAC)

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