Asteroid's troughs suggest stunted planet - 0 views
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Scientists have been trying to determine the origin of these unusual troughs since their discovery just last year
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new analysis supports the notion that the troughs are faults that formed when a fellow asteroid smacked into Vesta's south pole. The research reinforces the claim that Vesta has a layered interior, a quality normally reserved for larger bodies, such as planets and large moons.
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ggest of those troughs, named Divalia Fossa, surpasses the size of the Grand Canyon by spanning 465 kilometers (289 miles) long, 22 km (13.6 mi) wide and 5 km (3 mi) deep
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would only have been possible if the asteroid is differentiated – meaning that it has a core, mantle and crust
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previous research has found signs of igneous rock on Vesta, indicating that rock on Vesta's surface was once molten, a sign of differentiation
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If the troughs are made possible by differentiation, then the cracks aren't just troughs, they're graben
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graben is a dip in the surface that forms when two faults move apart from each other and the ground sinks into the widening gap
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observations indicate that Vesta is also unusually planet-like for an asteroid in that its mantle is ductile and can stretch under a lot of pressure
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unlike the larger asteroid Ceres, Vesta is not classified as a dwarf planet because the large collision at its south pole knocked it out of its spherical shape
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if Vesta has a mantle and core, that would mean it has qualities often reserved for planets, dwarf planets and moons—regardless of its shape
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believes the south pole collision knocked Vesta into its current speedy rate of rotation about its axis of about once per 5.35 hours
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may have caused the equator to bulge outward so far and so fast that the rotation caused the troughs, rather than the direct power of the impact
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scientists will continue to sort that data out and improve on computer simulations of Vesta's interior