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De la tectonique des plaques sur Vénus ? Un nouveau rebondissement !

De la tectonique des plaques sur Vénus ? Un nouveau rebondissement !
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Thick lithosphere casts doubt on plate tectonics in Venus s recent past

Date Time Thick lithosphere casts doubt on plate tectonics in Venus’s recent past A study of a giant impact crater on Venus suggests that its lithosphere was too thick to have had Earth-like plate tectonics, at least for much of the past billion years. PROVIDENCE, R.I. [Brown University] – At some point between 300 million and 1 billion years ago, a large cosmic object smashed into the planet Venus, leaving a crater more than 170 miles in diameter. A team of Brown University researchers has used that ancient impact scar to explore the possibility that Venus once had Earth-like plate tectonics. For a study published in Nature Astronomy, the researchers used computer models to recreate the impact that carved out Mead crater, Venus’s largest impact basin. Mead is surrounded by two clifflike faults – rocky ripples frozen in time after the basin-forming impact. The models showed that for those rings to be where they are in relation to the central crater, Venus’s lithosphere

Thick lithosphere casts doubt on plate tectonics in Venus s geologically recent past

 E-Mail IMAGE: Mead crater, the largest impact basin on Venus, is encircled by two rocky rings, which provide valuable information about the planet s lithosphere. view more  Credit: NASA PROVIDENCE, R.I. [Brown University] At some point between 300 million and 1 billion years ago, a large cosmic object smashed into the planet Venus, leaving a crater more than 170 miles in diameter. A team of Brown University researchers has used that ancient impact scar to explore the possibility that Venus once had Earth-like plate tectonics. For a study published in Nature Astronomy, the researchers used computer models to recreate the impact that carved out Mead crater, Venus s largest impact basin. Mead is surrounded by two clifflike faults rocky ripples frozen in time after the basin-forming impact. The models showed that for those rings to be where they are in relation to the central crater, Venus s lithosphere its rocky outer shell must have been quite thick, far thick

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