A Generalized Exosphere Model Across the Solar System

We have embarked on a parametrical study of exospheres as a function of basic controlling parameters such as the mass of the primary object, mass of the exospheric species, heliocentric distance, rotation rate of the primary, and composition of the body. These parameters will be useful for mission planning as well as quick look data to determine the size and location of bodies likely to retain their exospheres, the observability of exospheric species, and differences among bodies based on size, composition, rotation rate and other parameters. We will also consider the sizes of small clusters of atoms, and small dust particles that may be gravitationally bound to low mass bodies such as Phobos and asteroids. In addition, it is of interest to be able to determine the extent of contamination of the pristine exosphere due to the spacecraft sent to make measurements, and the effect on the measurements of outgassing in the instruments.