拥有卫星的星球更易产生生命

Having a companion in old age is good for people -- and, it turns out, might extend the chance for life on certain Earth-sized planets in the cosmos¹ as well. Planets cool as they age. Over time their molten cores solidify² and inner heat-generating activity dwindles³, becoming less able to keep the world habitable by regulating carbon dioxide to prevent runaway⁴ heating or cooling.

 

But astronomers⁶ at the University of Washington and the University of Arizona have found that for certain planets about the size of our own, the gravitational pull of an outer companion planet could generate enough heat -- through a process called tidal heating -- to effectively prevent that internal cooling, and extend the inner world's chance at hosting life.

 

UW astronomer⁵ Rory Barnes is second author of a paper published in the July issue of the Monthly Notices of the Royal Astronomical⁷ Society. The lead authors are graduate student Christa Van Laerhoven and planetary scientist Richard Greenberg at the University of Arizona.

 

Tidal heating results from the gravitational push and pull of the outer companion planet on its closer-in neighbor, Barnes said. The effect happens locally, so to speak, on Jupiter's moons Io and Europa. The researchers showed that this phenomenon can take place on exoplanets -- those outside the solar system -- as well.

 

Using computer models, the researchers found the effect can occur on older Earth-sized planets in noncircular orbits in the habitable zone of low-mass stars, or those less than one-quarter the mass of the Sun. The habitable zone is that swath of space around a star just right to allow an orbiting rocky planet to sustain liquid water on its surface, thus giving life a chance.

 

"When the planet is closer to the star, the gravitational field is stronger and the planet is deformed⁸ into an American football shape. When farther from the star, the field is weaker and the planet relaxes into a more spherical⁹（球形的） shape," Barnes said. "This constant flexing¹⁰ causes layers inside the planet to rub against each other, producing frictional heating."

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