NASA’s Dawn mission continues to reveal the intriguing past of Ceres, the Texas-sized dwarf planet residing in the main asteroid belt. Now, two new studies are delving even deeper into the world’s potentially water-rich history. One study found that Ceres’ crust contains materials such as ice and salts that have undergone past and possibly recent geologic activity; another identified a relatively soft, malleable layer of material just below the hard outer crust. Both point to the possibility of a global ocean in Ceres’ past, and even the remnants of that ocean beneath the surface today.
“More and more, we are learning that Ceres is a complex, dynamic world that may have hosted a lot of liquid water in the past, and may still have some underground,” said Julie Castillo-Rogez of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, in a
press release. Castillo-Rogez is both a Dawn project scientist and co-author of the recent studies.
Gravity anomalies
Gathering data on Ceres’ composition is difficult — the Dawn spacecraft is not designed to land on the dwarf planet, so measurements of its gravity are instead translated into compositional information. This is achieved by studying tiny variations in Dawn’s orbit as it circles the world; these variations can then be associated with specific features on or below Ceres’ surface: “gravity anomalies.”
The first recent study of Ceres, published in the
Journal of Geophysical Research and led by Anton Ermakov of JPL, found that “Ceres has an abundance of gravity anomalies associated with outstanding geologic features,” he said. Many of these features, such as Occator, Kerwan and Yalode craters and the mountain Ahuna Mons, are associated with cryovolcanism and its effects, highlighting the importance of such geologic activity in shaping the small world.
Additionally, the data indicate that Ceres’ crust has a low density more similar to ice than rock. However, Ceres’ crust is also relatively hard — so it raises the question, how can it be both?