DLR-Logo -> http://www.dlr.de
DLR Portal Home | Imprint | Contact | Deutsch
Fontsize: [-] Text [+]

“TNOs are Cool”: A survey of the trans-Neptunian region. VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects

Vilenius, E. and Kiss, C. and Mommert, M. and Müller, T. and Santos-Sanz, P. and Pal, A. and Stansberry, J. and Mueller, M. and Peixinho, N. and Fornasier, S. and Lellouch, E. and Delsanti, A. and Thirouin, A. and Ortiz, J. L. and Duffard, R. and Perna, D. and Szalai, N. and Protopapa, S. and Henry, F. and Hestroffer, D. and Rengel, M. and Dotto, E. and Hartogh, P. (2012) “TNOs are Cool”: A survey of the trans-Neptunian region. VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects. Astronomy and Astrophysics, 541, A94. DOI: 10.1051/0004-6361/201118743. ISSN 0004-6361.

Full text not available from this repository.

Official URL: http://dx.doi.org/10.1051/0004-6361/201118743


Context. Trans-Neptunian objects (TNO) represent the leftovers of the formation of the solar system. Their physical properties provide constraints to the models of formation and evolution of the various dynamical classes of objects in the outer solar system. Aims: Based on a sample of 19 classical TNOs we determine radiometric sizes, geometric albedos and beaming parameters. Our sample is composed of both dynamically hot and cold classicals. We study the correlations of diameter and albedo of these two subsamples with each other and with orbital parameters, spectral slopes and colors. Methods: We have done three-band photometric observations with Herschel/PACS and we use a consistent method for data reduction and aperture photometry of this sample to obtain monochromatic flux densities at 70.0, 100.0 and 160.0 μm. Additionally, we use Spitzer/MIPS flux densities at 23.68 and 71.42 μm when available, and we present new Spitzer flux densities of eight targets. We derive diameters and albedos with the near-Earth asteroid thermal model (NEATM). As auxiliary data we use reexamined absolute visual magnitudes from the literature and data bases, part of which have been obtained by ground based programs in support of our Herschel key program. Results: We have determined for the first time radiometric sizes and albedos of eight classical TNOs, and refined previous size and albedo estimates or limits of 11 other classicals. The new size estimates of 2002 MS4 and 120347 Salacia indicate that they are among the 10 largest TNOs known. Our new results confirm the recent findings that there are very diverse albedos among the classical TNOs and that cold classicals possess a high average albedo (0.17 ± 0.04). Diameters of classical TNOs strongly correlate with orbital inclination in our sample. We also determine the bulk densities of six binary TNOs. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

Document Type:Article
Title:“TNOs are Cool”: A survey of the trans-Neptunian region. VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
AuthorsInstitution or Email of AuthorsAuthors ORCID
Vilenius, E.MPE, GarchingUNSPECIFIED
Kiss, C.Konkoly ObservatoryUNSPECIFIED
Mommert, M.michael.mommert@dlr.deUNSPECIFIED
Müller, T.MPE, GarchingUNSPECIFIED
Santos-Sanz, P. Observatoire de Paris-Meudon, France UNSPECIFIED
Pal, A.Konkoly ObservatoryUNSPECIFIED
Stansberry, J.U. of ArizonaUNSPECIFIED
Mueller, M.SRON, NetherlandsUNSPECIFIED
Peixinho, N.Center for Geophysics of the University of CoimbraUNSPECIFIED
Fornasier, S. Observatoire de Paris-Meudon, France UNSPECIFIED
Lellouch, E. Observatoire de Paris-Meudon, France UNSPECIFIED
Delsanti, A.Lab. d'Astrophysique de Marseille, FranceUNSPECIFIED
Thirouin, A.IAA-CSIC Granada, SpainUNSPECIFIED
Ortiz, J. L.IAA-CSIC Granada, SpainUNSPECIFIED
Duffard, R.IAA-CSIC Granada, SpainUNSPECIFIED
Perna, D.INAF - Osservatorio Astronomico di RomaUNSPECIFIED
Szalai, N.Konkoly ObservatoryUNSPECIFIED
Protopapa, S.U. of MarylandUNSPECIFIED
Henry, F.Observatoire de Paris-Meudon, France UNSPECIFIED
Hestroffer, D.Observatoire de Paris, France UNSPECIFIED
Rengel, M.MPS, Lindau-KatlenburgUNSPECIFIED
Dotto, E.Osservatorio Astronomico di Roma, ItalyUNSPECIFIED
Hartogh, P.MPS, Lindau-KatlenburgUNSPECIFIED
Date:May 2012
Journal or Publication Title:Astronomy and Astrophysics
Refereed publication:Yes
In Open Access:No
In ISI Web of Science:Yes
Page Range:A94
Keywords:Kuiper belt: general, infrared: planetary systems, techniques: photometric
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Exploration des Sonnensystems (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Asteroids and Comets
Deposited By: Mommert, Michael
Deposited On:24 Oct 2012 08:29
Last Modified:19 Jul 2016 17:29

Repository Staff Only: item control page

Help & Contact
electronic library is running on EPrints 3.3.12
Copyright © 2008-2012 German Aerospace Center (DLR). All rights reserved.