Originally Posted by
Dreamwoven
Society for Popular Astronomy:
BRIGHT AREAS ON CERES SUGGEST 'GEO'LOGICAL ACTIVITY
NASA
Since Dawn arrived in orbit around Ceres in 2015 March, scientists have located more than 300 bright areas on Ceres' surface. A new study divides the features into four categories. The first group of bright spots contains the most reflective material on Ceres, which is found on crater floors. The most iconic examples are in Occator Crater, which hosts two prominent bright areas. Cerealia Facula, in the centre of the crater, consists of bright material covering a 10-km-wide pit, within which sits a small dome. East of the centre is a collection of slightly less reflective and more diffuse features called Vinalia Faculae. All the bright areas in Occator Crater are made of salt-rich material, which was probably once mixed in water. Although Cerealia Facula is the brightest area on all of Ceres, it would resemble dirty snow to the human eye. More commonly, in the second category, bright material is found on the rims of craters, streaking down toward the floors. Impacting bodies probably exposed bright material that was already in the sub-surface or had formed in a previous impact event.Separately, in the third category, bright material can be found in the material ejected when craters were formed. The mountain Ahuna Mons gets its own fourth category -- the one instance on Ceres where bright material is not associated with any impact crater. It is probably a cryovolcano, a volcano formed by the gradual accumulation of thick, slowly flowing icy materials; it has prominent bright streaks on its flanks. Over hundreds of millions of years, bright material has mixed with the dark material that forms the bulk of Ceres' surface, as well as debris ejected by impacts. That means that billions of years ago, when Ceres experienced more impacts, the dwarf planet's surface would probably have been peppered with thousands of bright areas.
Why do the different bright areas of Occator seem so distinct from one another? The leading explanation for what happened is that Occator could have had, at least in the recent past, a reservoir of salty water beneath it. Vinalia Faculae, the diffuse bright regions to the northeast of the crater's central dome, could have formed from a fluid driven to the surface by a small amount of gas, similar to champagne surging out of its bottle when the cork is removed. In the case of the Vinalia Faculae, the dissolved gas could have been a volatile substance such as water vapour, carbon dioxide, methane or ammonia. Volatile-rich salty water could have been brought close to Ceres' surface through fractures that connected to the briny reservoir beneath Occator. The lower pressure at Ceres' surface would have caused the fluid to boil off as a vapour. Where fractures reached the surface, the vapour could escape energetically, carrying with it ice and salt particles and depositing them on the surface. Cerealia Facula must have formed by a somewhat different process, given that it is more elevated and brighter than Vinalia Faculae. The material at Cerealia may have been more like an icy lava, seeping up through the fractures and swelling into a dome. Intermittent phases of boiling, similar to what happened when Vinalia Faculae formed, may have occurred during that process, littering the surface with ice and salt particles that formed the Cerealia bright spot. The analyses do not depend on the initial impact that formed Occator. However, the current thinking among Dawn scientists is that when a large body slammed into Ceres, excavating the 92-kilometre-wide crater, the impact may also have created fractures through which liquid later emerged. As Dawn continues the final phase of its mission, in which it will descend to lower altitudes than ever before, scientists hope to continue learning about the origins of the bright material on Ceres and what gave rise to the enigmatic features in Occator.