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Thermal Emission of the Eris — Dysnomia System as Observed by Herschel/PACS

Kiss, C. and Vilenius, E. and Müller, T. G. and Pál, A. and Rengel, M. and Mommert, M. and Szalai, N. and Santos-Sanz, P. and Lellouch, E. and Stansberry, J. A. (2012) Thermal Emission of the Eris — Dysnomia System as Observed by Herschel/PACS. Asteroids, Comets, Meteors 2012, May 16-20, 2012, Niigata, Japan.

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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.

Document Type:Conference or Workshop Item (Speech)
Title:Thermal Emission of the Eris — Dysnomia System as Observed by Herschel/PACS
AuthorsInstitution or Email of Authors
Kiss, C.Konkoly Observatory
Vilenius, E.MPE Garching
Müller, T. G.MPE Garching
Pál, A.Konkoly Observatory
Rengel, M.MPS, Lindau-Katlenburg
Mommert, M.michael.mommert@dlr.de
Szalai, N.Konkoly Observatory
Santos-Sanz, P.IAA, Spain
Lellouch, E.Observatoire de Paris-Meudon, France
Stansberry, J. A.U of Arizona
Keywords:Herschel, Eris, TNOs
Event Title:Asteroids, Comets, Meteors 2012
Event Location:Niigata, Japan
Event Type:international Conference
Event Dates:May 16-20, 2012
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Vorhaben Exploration des Sonnensystems
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Asteroids and Comets
Deposited By: Michael Mommert
Deposited On:09 Nov 2012 10:33
Last Modified:09 Nov 2012 10:33

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