The mysterious dark streaks on Vesta

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dark material on Vesta

In a preprint paper published today at the Los Alamos astro-ph website, scientists have taken a detailed look at the mysterious dark streaks seen by Dawn on the surface of the asteroid Vesta and have concluded that the material comes from impacts, not from volcanic activity.

The scientists also concluded that

the majority of the spectra of [dark material] are similar to carbonaceous chondrite meteorites mixed with materials indigenous to Vesta.

Carbonaceous chondrite meteorites are considered to be the most primeval material in the solar system. This means that Vesta has the potential to give scientists a convenient laboratory for studying that primeval material and the early formation of the solar system. Ideally, the best way to do this would of course be to go there.

The scientists also theorize that much of this material was brought to Vesta by a single large impact.

Our modeling efforts using impact crater scaling laws and numerical models of ejecta re-accretion suggest the delivery and emplacement of this [dark material] on Vesta during the formation of the ~400 km Veneneia basin by a low-velocity (<2 km/sec) carbonaceous impactor.

The Veneneia basin is one of the largest impact basins on Vesta and is thought to be about two billion years old.

Later impacts further distributed the dark material about the surface of Vesta, while also burying much of this material.

The image above shows the global distribution of geologic features associated with the dark material. Blue corresponds to lowest elevation and red the highest. Dark material is indicated by the white and black spots, with the black spots cases where the dark material is associated with craters. The black line indicates the approximate outline of the rim of the Rheasilvia basin, the largest such impact basin on Vesta and thought to be about one billion years old, while the broken red line indicates the rim of the older Veneneia basin.

As you can see, the dark material seems to cluster around the rim of the Veneneia basin. It mostly disappears inside the Rheasilvia Basin, which was created by an impact after Veneneia and wiped it away. The only evidence of dark material in the Rheasilvia Basin are newer crater impacts, which would have is drilled into the surface and exposed older material.

You can download and read the full paper here. [pdf]


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