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Surface characterization of 28978 Ixion (2001 KX76)

Authors :
Boehnhardt, Hermann
Bagnulo, Stefano
Muinonen, Karri
Barucci, Maria Antonella
Kolokolova, L.
Dotto, Elisabetta
Tozzi, Gian Paolo
Max-Planck-Institut für Astronomie (MPIA)
European Southern Observatory
Jakokoski Observatory, University of Helsinki
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Pôle Planétologie du LESIA
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Department of Astronomy, University of Florida
INAF-Osservatorio Astronomico di Roma (INAF-OAR)
INAF-Osservatorio Astrofisico di Arcetri (INAF-OAA)
Source :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2004, 415, pp.L21-L25
Publication Year :
2004
Publisher :
HAL CCSD, 2004.

Abstract

International audience; The Plutino 28978 Ixion, one of the largest objects in the Kuiper Belt, is measured by R filter photometry and linear polarimetry over the phase angle range as well as by BVRI colours and visible spectroscopy. Ixion is a medium red object with spectral slope of 17.7%/100 nm (400-900 nm). While its opposition phase curve surge (0.2 mag/deg) is within the typical range found for other solar system objects, it displays unusually high negative polarization (min. -1.3%). Comparison with model spectra and numerical modeling of the opposition brightening and polarization effects suggest an areal mixture of absorbing (dark) and icy (bright) compounds on its surface: the mixing ratio is about 6:1 for dark and bright material of 0.21 and 0.79 single-scattering albedo and of 250 and 33 dimensionless mean free path (length multiplied by wave number), respectively.

Details

Language :
English
ISSN :
00046361
Database :
OpenAIRE
Journal :
Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2004, 415, pp.L21-L25
Accession number :
edsair.od......2417..1c13f70245dfece4d03e0c8416da86c3