Asteroid Impact Delivered Carbon to Giant Asteroid Vesta

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PSI Staff

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Dark material seen on the giant asteroid Vesta by instruments on NASA’s Dawn spacecraft was likely emplaced by the low-speed impact of a carbon-based asteroid, according to research described in a new paper.

The mysterious dark material seen by Dawn’s framing camera has the same composition as carbonaceous chondrite meteorites, according to “Delivery of dark material to Vesta via carbonaceous chondritic impacts” published in Icarus. Vishnu Reddy of the Max Planck Institute for Solar System Research is lead author and Planetary Science Institute Research Scientist David P. O’Brien is a coauthor.

In the most comprehensive analysis of the dark material to date, Dawn scientists describe how this carbon-rich material tends to appear around the edge of two giant impact basins in Vesta’s southern hemisphere. The analysis suggests that the object that created the older of the two basins – known as Veneneia – about 2 to 3 billion years ago most likely delivered the dark material.  That material was later covered up by the impact that created the younger basin, Rheasilvia, and is now being exposed as impacts excavate subsurface material.

“Dawn results have shown that Vesta’s giant southern hemisphere impacts have had a profound influence on its evolution,” said PSI’s O’Brien, who performed the calculations to determine under what conditions significant amounts of carbonaceous material could be delivered to the surface of Vesta by impacts.  “This work provides yet another link between those impacts and the features we see on the surface.

“A possible history is that the impact that formed the Veneneia impact basin laid down ejecta containing the dark carbonaceous material, which was subsequently covered by ejecta from the younger Rheasilvia impact,” O’Brien said. “Finally, craters forming since then punch through to the dark material, leading to the exposures of dark material seen today, which are generally associated with impact craters.”

Impacts by similar asteroids in the early days of the formation of our solar system could have provided the inner planets, including Earth, with water, carbon, and other organic materials, essential ingredients for the development of life.

These mosaic images from NASA’s Dawn mission show how dark, carbon-rich materials tend to speckle the rims of smaller craters or their immediate surroundings on the giant asteroid Vesta. The image on the left is Numisia Crater and the image on the right is a shallow, unnamed crater in the Sextilia quadrangle. The left-hand image was obtained by Dawn’s framing camera during its low-altitude mapping orbit phase, about 130 miles (210) kilometers above the surface. The image on the right was obtained during Dawn’s high-altitude mapping orbit, about 420 miles (680 kilometers) above the surface. The images have been photometrically corrected. North is up. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
This composite-color view from NASA’s Dawn mission shows Cornelia Crater, streaked with dark materials, on the giant asteroid Vesta. The data were obtained by Dawn’s framing camera during the mission’s high-altitude mapping orbit, about 420 miles (680 kilometers) above the surface. The images were integrated into a mosaic and wrapped on a topographical model of Vesta’s surface. Scientists colorized the picture by assigning red to the 0.75-micron wavelength, green to the 0.92-micron wavelength and blue to the 0.98-micron wavelength. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDANASA/JPL-Caltech/UCLA/MPS/DLR/IDA

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Related Paper

Authors: V. Reddy, L. Le Corre, D. P. O’Brien, A. Nathues, E. A. Cloutis, D. D. Durda, W. F. Bottke, M. U. Bhatt, D. Nesvorny, D. Buczkowski, J. E. C. Scully, E. M. Palmer, H. Sierks, P. J. Mann, K. J. Becker, A. W. Beck, D. Mittlefehldt, J. Li, R. Gaskell, C. T. Russell, M. J. Gaffey, H. Y. McSween, T. B. McCord, J. P. Combe, D. Blewett
Journal: Icarus
Published: December 2012
DOI: 10.1016/j.icarus.2012.08.011
Ref: Reddy, V., Le Corre, L., O’Brien, D. P., et al. “Delivery of dark material to Vesta via carbonaceous chondritic impacts.” Icarus, 221.2 (2013).