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ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey

Harris, A.W. und Mommert, M. und Hora, J.L. und Mueller, M. und Trilling, D.E. und Bhattacharya, B. und Bottke, W.F. und Chesley, S. und Delbo, M. und Emery, J.P. und Fazio, G. und Mainzer, A. und Penprase, B. und Smith, H.A. und Spahr, T.B. und Stansberry, J.A. und Thomas, C.A. (2011) ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey. Astronomical Journal, 141 (3), Seiten 1-10. Institute of Physics. DOI: 10.1088/0004-6256/141/3/75.

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Offizielle URL: http://iopscience.iop.org/1538-3881/141/3/75/pdf/1538-3881_141_3_75.pdf


We report on results of observations of near-Earth objects (NEOs) performed with the NASA Spitzer Space Telescope as part of our ongoing (2009–2011) Warm Spitzer NEO survey (“ExploreNEOs”), the primary aim of which is to provide sizes and albedos of some 700 NEOs. The emphasis of the work described here is an assessment of the overall accuracy of our survey results, which are based on a semi-empirical generalized model of asteroid thermal emission. The NASA Spitzer Space Telescope has been operated in the so-called Warm Spitzer mission phase since the cryogen was depleted in 2009 May, with the two shortest-wavelength channels, centered at 3.6 μm and 4.5 μm, of the Infrared Array Camera continuing to provide valuable data. The set of some 170 NEOs in our current Warm Spitzer results catalog contains 28 for which published taxonomic classifications are available, and 14 for which relatively reliable published diameters and albedos are available. A comparison of the Warm Spitzer results with previously published results (“ground truth”), complemented by a Monte Carlo error analysis, indicates that the rms Warm Spitzer diameter and albedo errors are ±20% and ±50%, respectively. Cases in which agreement with results from the literature is worse than expected are highlighted and discussed; these include the potential spacecraft target 138911 2001 AE2. We confirm that 1.4 appears to be an appropriate overall default value for the relative reflectance between the V band and the Warm Spitzer wavelengths, for use in correction of the Warm Spitzer fluxes for reflected solar radiation.

Zusätzliche Informationen:Article i.d: The Astronomical Journal, Volume 141, Issue 3, article id. 75 (2011)
Titel:ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey
AutorenInstitution oder E-Mail-Adresse der Autoren
Harris, A.W.alan.harris@dlr.de
Mommert, M.michael.mommert@dlr.de
Hora, J.L.Harvard-Smithsonian Center for Astrophysics, USA
Mueller, M.Universite de Nice Sophia Antipolis, France
Trilling, D.E.Northern Arizona University, USA
Bhattacharya, B.NASA Herschel Science Center Caltech, USA
Bottke, W.F.Southwest Research Institute, USA
Chesley, S.Jet Propulsion Laboratory, California Institute of Technology, USA
Delbo, M.Universite de Nice Sophia Antipolis, France
Emery, J.P.Department of Earth and Planetary Sciences, University of Tennessee, USA
Fazio, G.Harvard-Smithsonian Center for Astrophysics, USA
Mainzer, A.Jet Propulsion Laboratory, California Institute of Technology, USA
Penprase, B.Department of Physics and Astronomy, Pomona College, USA
Smith, H.A.Harvard-Smithsonian Center for Astrophysics, USA
Spahr, T.B.Harvard-Smithsonian Center for Astrophysics, USA
Stansberry, J.A.Steward Observatory, University of Arizona, USA
Thomas, C.A.Northern Arizona University, USA
Datum:März 2011
Erschienen in:Astronomical Journal
Referierte Publikation:Ja
In Open Access:Nein
In ISI Web of Science:Ja
DOI :10.1088/0004-6256/141/3/75
Seitenbereich:Seiten 1-10
Verlag:Institute of Physics
Stichwörter:Asteroids, Near-Earth objects, Spitzer Space telescope
HGF - Forschungsbereich:Verkehr und Weltraum (alt)
HGF - Programm:Weltraum (alt)
HGF - Programmthema:W EW - Erforschung des Weltraums
DLR - Schwerpunkt:Weltraum
DLR - Forschungsgebiet:W EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):W - Vorhaben Asteroiden und Kometen (alt)
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Asteroiden und Kometen
Hinterlegt von: Prof. Alan Harris
Hinterlegt am:11 Mai 2011 14:09
Letzte Änderung:20 Mär 2013 19:44

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