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The Warm Spitzer NEO Survey: exploring the history of the inner Solar System and near Earth space

Trilling, D und Bhattacharya, B und Bottke, W und Chesley, S und Delbo, M und Emery, J und Fazio, G und Harris, A.W. und Hora, J und Mainzer, A und Mueller, M und Penprase, B und Smith, H und Spahr, T und Stansberry, J (2009) The Warm Spitzer NEO Survey: exploring the history of the inner Solar System and near Earth space. American Astronomical Society. American Astronomical Society, Meeting #214, 2009-06-07 - 2009-06-11, Pasadena, USA.

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Kurzfassung

The majority of Near Earth Objects (NEOs) originated in collisions between bodies in the main asteroid belt and have found their way into near-Earth space via complex and little understood dynamical interactions. This transport of material from the main belt into the inner Solar System has shaped the histories of the terrestrial planets. However, despite their scientific importance, key characteristics of the NEO population --‑ such as the size distribution, mix of albedos and mineralogies, and contributions from so-called dead or dormant comets --‑ remain largely unexplored; some 99% of all presently known NEOs are essentially uncharacterized. Recent evidence suggests that the size distribution of NEOs may undergo a transition at 1 km, and that the smaller bodies may record fundamental physical processes that are presently occurring in the Solar System but not understood. We will use the unique capability of Warm Spitzer to observe 700 NEOs. We will measure the size distribution of this population to understand fundamental physical processes that occur among the small bodies of our Solar System. We will measure the fraction of NEOs likely to be dead comets, with implications for the flux of organic material onto the Earth. We will measure the albedo distribution of NEOs, which indicates the compositional diversity among these small bodies. We will study properties of individual NEOs, including their surface properties and potentially their densities, and detailed properties of a subset of well-characterized objects. Our expert team and our previous experience in this field will allow us to complete a comprehensive study of the origin and evolution of the NEO population. Our work is nothing less than an exploration of the history of near-Earth space.

Dokumentart:Konferenzbeitrag (Paper)
Titel:The Warm Spitzer NEO Survey: exploring the history of the inner Solar System and near Earth space
Autoren:
AutorenInstitution oder E-Mail-Adresse der Autoren
Trilling, DNorthern Arizona University, USA
Bhattacharya, BNASA Herschel Science Center, California, USA
Bottke, WSWRI, Colorado, USA
Chesley, SJPL, California, USA
Delbo, MObservatoire de la Cote d'Azur, France
Emery, JU. Tennessee-Knoxville, USA
Fazio, GHarvard-Smithsonian, USA
Harris, A.W.NICHT SPEZIFIZIERT
Hora, JHarvard-Smithsonian, USA
Mainzer, AJPL, California, USA
Mueller, MUniv. Arizona, USA
Penprase, BPomona College, California, USA
Smith, HHarvard-Smithsonian, USA
Spahr, THarvard-Smithsonian, USA
Stansberry, JUniv. Arizona, USA
Datum:Mai 2009
Referierte Publikation:Nein
In SCOPUS:Nein
In ISI Web of Science:Nein
Band:41
Seitenbereich:Seite 716
Verlag:American Astronomical Society
Name der Reihe:Bulletin of the American Astronomical Society
Status:veröffentlicht
Stichwörter:Solar System; Near-Earth asteroids; Spitzer Space Telescope
Veranstaltungstitel:American Astronomical Society, Meeting #214
Veranstaltungsort:Pasadena, USA
Veranstaltungsart:internationale Konferenz
Veranstaltungsdatum:2009-06-07 - 2009-06-11
Veranstalter :American Astronomical Society
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:26 Aug 2009 11:58
Letzte Änderung:21 Jan 2010 10:11

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