Cometary Comae

Comets are frozen left-overs from our Solar System's epoch of planetary formation. By studying their composition and evolution, we can help infer how the Solar System formed. However, we generally do not directly sense the composition of the cometary nucleus, the kilometer-sized solid body at the center of all comets, but instead study the coma.

The coma is created when the ices within the nucleus are warmed, sublimate, and drive erosion (mass loss). This process is known as cometary activity.

The composition of the coma reflects that of the surface of the nucleus. By studying cometary activity, and the evolution of the surface, we can infer the composition of the interior of the nucleus.

Copyright © Michael S. P. Kelley 2024