New research indicates that cracks in the moon's crust have formed as the interior has cooled and shrunk over the past billion years or so. That means the surface has shrunk, too, though not so much you'd notice from gazing at it.
Scientists have identified 14 clifflike landforms called lobate scarps scattered over the surface of the moon, said Thomas R. Watters of the Center for Earth and Planetary Studies at the Smithsonian's National Air and Space Museum. Watters and colleagues describe their find in Friday's edition of the journal Science.
The scarps had previously been noted at the moon's equator, but this is the first evidence in other areas, indicating they result from a global process.
The study calls the scarps "evidence of recent thrust faulting on the moon." But this is planetary science, where "recent" can mean a billion years ago.
The scarps, or cliffs, extend across some small craters, and small craters tend to be obliterated over time, Watters said in a telephone interview. In addition, there are no large craters imposed on top of the scarps, another indication they are relatively recent, in planetary terms, he said.
"One of the really cool parts of this . . . the faults are so young-looking that you can't escape the possibility that this contraction occurred recently, and could indicate that the moon is still active," Watters said.
The size of the scarps indicates a shrinkage in the size of the moon of about 100 meters, or 328 feet, the researchers said. The moon is about one-fourth the size of Earth in diameter.
The scarps are up to 10 meters high and a few kilometers long, Watters said. By comparison, Mercury has much larger scarps indicating considerably more shrinkage over time.
The moon's not going to disappear and its shrinkage won't affect Earth, Watters said.
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