Is (1) Ceres a Small Planet or a Large Comet?

Friday, 19 December 2014: 10:50 AM
Michael Küppers1, Laurence O'Rourke2, Dominique Bockelée-Morvan3, Vladimir Zakharov3, Seungwon Lee4, Paul Von Allmen4, Benoit Carry5, David Teyssier2, Anthony Marston2, Thomas Müller6, Jacques Crovisier3, M. Antonietta Barucci3 and Raphael Moreno3, (1)European Space Agency, Villanueva De La Can, Spain, (2)European Space Agency, Villanueva de la Canada, Spain, (3)Paris Observatory Meudon, Meudon, France, (4)Jet Propulsion Laboratory, Burbank, CA, United States, (5)Paris Observatory, Paris, France, (6)Max Planck Insitute for Extraterrestrial Physics, Garching, Germany
The snowline conventionally divides Solar System objects into dry bodies, ranging out to the main asteroid belt, and icy bodies beyond the belt. Recently, the detection of dust emission from "main-belt comets" and of hydration features and possible water ice absorption on some main-belt asteroids together with theories of migration of small bodies in the solar system cast some doubts on the classical picture.

Ceres, contributing about 30 % of the mass of the asteroid belt, is thought to be differentiated into an icy core and a silicate mantle and hydrated minerals were found on infrared spectra of its surface. A marginal detection of OH, a photodissociation product of water was reported in 1991, but questioned by later, more sensitive observations.. Observations of Ceres with the Heterodyne Instrument for the Far Infrared (HIFI) on the Herschel Space Observatory in the context of the MACH 11 guaranteed time program and with a follow up DDT program detected water vapour from Ceres on 3 occasions in 2012 and 2013. The production rate of water on Ceres is a few times 1026 s1.

The signal from the water vapour from Ceres was found to be linearly polarized during some of the observations, with the absorption being stronger in the horizontal branch. The measured line area ratio of up to 2.5 between H and V polarizations is so far unexplained.

The water signal varies on time scales of hours. Those variations are interpreted as localized sources on Ceres surface rotating into and out of the hemisphere visible by Herschel. The time variability is consistent with those sources being dark features known from ground-based adaptive optics observations.

The water vapour on Ceres may be either produced by near surface ice heated by sunlight (cometary activity) or by cryovolcanoes or geysers getting their energy from Ceres’ interior. In the first case the production rate is expected to peak around perihelion, while for volcanic the time variations are expected to be more stochastic. The existing observations appear consistent with the cometary hypothesis, but do not allow to clearly distinguish between those possibilities. Upon its arrival at Ceres in 2015, the DAWN spacecraft may provide insight into the sources and mechanisms of water production at Ceres.