
One  of the largest alien worlds yet discovered may create a huge  shock  wave as it plows through the wind blowing off its host star,   astronomers have found. That may mean the planet has a magnetic field   that protects it in its perilously close orbit. The discovery may help   astronomers understand the atmospheres, and ultimately the   life-supporting potential, of worlds beyond our solar system. 
  Scientists  identified the first alien world, or exoplanet, in 1992,  and since  then the number has ballooned to 531. In 2008, astronomers  added a  planet named WASP-12b to the roster. WASP-12b is a “hot  Jupiter,” a  gaseous planet similar in size to our own gas giant but with  a blisteringly hot surface temperature of more than 2000°C.   It whips around its host star at a distance of less than 1/16th the   distance from the sun to Mercury, completing its orbit once every 26   hours. In 2010, scientists at the Open University in the United Kingdom   used the Hubble Space Telescope to view WASP-12b’s transit and noticed   that as it crossed its star, its "shadows" appeared first in the   ultraviolet (UV) wavelengths before the rest of the planet blocked the   sun.
Aline  Vidotto and her team at the University of St. Andrews in the  United  Kingdom theorized that the out-of-sync dimming could be explained  by a  shock wave in the stellar wind, the stream of charged gas  particles  flowing off the star and immersing the planet. The shock wave  is  similar to that created by a supersonic jet aircraft as it travels   through air, building up pressure waves around its nose that merge   together. The planet’s shock wave would be pushed in front of it as it   orbits at supersonic speeds, and the wave would absorb some of the UV   light emitted from the star. Earth and Saturn exhibit similar “bow   shocks,” but this is the first evidence of a shock surrounding an   exoplanet. 
  Vidotto  and her team calculated the distance from the planet’s  surface to the  front of the apparent bow shock and were surprised that  it was more  than four times the planet’s radius. The team reasoned that strong magnetic forces were repelling the stellar wind   because gaseous pressures alone would not be enough to hold it off at   such a distance, says Vidotto, who presented the findings at this  week’s  meeting of the Royal Astronomical Society in Llandudno in the  United  Kingdom. 
Earth’s  magnetic field shields our atmosphere from the destructive  powers of  the solar wind, and many scientists believe a magnetic field  may be a  prerequisite for a habitable planet. “While WASP-12b is far too  hot to  support life, being able to detect planetary magnetic fields  will help  with our understanding of and identifying the habitable zones  around  exoplanets," says Joseph Llama, a Ph.D. student on Vidotto’s  team. 
  To  further explore exoplanet magnetism, the team has put together a  list  of potential planets that they believe offer the most promising  chances  to glimpse similar bow shocks. “It’s very competitive to get  [Hubble]  time, so we cannot ask to look at all the transiting planets,”  Vidotto  says. 
  Alan  Aylward, an astrophysicist at University College London,  cautions that  a magnetic field may not be the only plausible explanation  for the  observed bow shock, noting that normal assumptions about  atmospheric  dynamics may not apply in such exotic environments. Still,  he says, the  possibility of such a field leads to many interesting lines  of  inquiry, including questions about how planets produce magnetic  fields.  
  Heather  Knutson, an astronomer at the University of California,  Berkeley, says  the findings could help scientists know where to  concentrate their  observing efforts to spot new astronomical phenomena.  “A consistent  story with exoplanets is that they are almost never what  we expect them  to be,” she says. 
 
 
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