Thermal Emission of the Eris — Dysnomia System as Observed by Herschel/PACS
Abstract
We will present the physical characteristics of Eris (size, albedo, thermal inertia, etc.) based on our recent Herschel/PACS data, and will discuss the influence of Dysnomia in our system-integrated thermal data and constrain its size and albedo.
- Publication:
-
Asteroids, Comets, Meteors 2012
- Pub Date:
- May 2012
- Bibcode:
- 2012LPICo1667.6357K