Researchers also find salt deposits in an impact crater on the dwarf planet.

© MPS, based on data from the Dawn mission: NASA/JPL-Caltech/UCLA/MPS/DLR/IDARugged surface: Numerous large, striking craters are found on the surface of dwarf planet Ceres.
The third-largest crater on the dwarf planet Ceres was geologically active at least once many millions of years after its formation. In a recent study published today in the journal
Nature Communications, researchers from the Max Planck Institute for Solar System Research (MPS) in Göttingen, the University of Münster (WWU) and the National Institute of Science Education and Research (NISER) in Bhubaneswar, India present the most detailed study of Urvara crater to date. For the first time, they evaluated camera images from the last phase of NASA's Dawn mission, which reveal geological structures only a few meters in size. The Dawn spacecraft entered orbit around the dwarf planet in 2015 and studied it up close for about three and a half years. Like Occator crater, Urvara crater may have been the scene of cryovolcanic activity, the researchers argue.
The study supports the picture that a global saline ocean extended beneath Ceres' crust, some of which may still be liquid today.Numerous large craters cover the surface of dwarf planet Ceres, the largest body in the asteroid belt at about 960 kilometers in diameter. Probably the most striking of these craters is Occator located in the northern hemisphere. The bright spots in its interior, which were already clearly visible during Dawn's approach phase, turned out to be saline remnants of a subsurface brine, which rose to the surface through cryovolcanic processes until recent geological times. In another large crater, called Ernutet, there is evidence of exposed organic compounds and thus very complex chemistry. In their latest publication, researchers led by the MPS now turn their attention to Urvara crater. Located in the southern hemisphere, it is Ceres' third largest crater, with a diameter of 170 kilometers. The impact that formed it about 250 million years ago is thought to have revealed material from depths of up to 50 kilometers.
"The large impact structures on Ceres give us access to the deeper layers of the dwarf planet," explains Andreas Nathues of the MPS, first author of the current study and Lead Investigator of Dawn's camera team. "As it turns out, the current topography and mineralogical composition of some of Ceres' large craters is the result of complex and long-lasting geological processes that have altered the dwarf planet's surface," he adds.
Comment: The following video is by one of the authors of the above paper, Melanie During, explaining the findings: See also:
- The Seven Destructive Earth Passes of Comet Venus
- Fossil jawbone from Alaska forces rethink of dinosaurs in the Arctic
- Dinosaurs appeared much earlier, then their numbers exploded during planetary upheaval and mass extinction event
And check out SOTT radio's: