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    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/101704


    Title: Redistribution of particles across the nucleus of comet 67P/Churyumov-Gerasimenko
    Authors: 葉永烜;Thomas, N.;Davidsson, B.;El-Maarry, M. R.;Fornasier, S.;Giacomini, L.;Gracia-Berná, A. G.;Hviid, S. F.;Ip, W.-H.;Jorda, L.;Keller, H. U.;Knollenberg, J.;Kührt, E.;La Forgia, F.;Lai, I. L.;Liao, Y.;Marschall, R.;Massironi, M.;Mottola, S.;Pajola, M.;Poch, O.;Pommerol, A.;Preusker, F.;Scholten, F.;Su, C. C.;Wu, J. S.;Vincent, J.-B.;Sierks, H.;Barbieri, C.;Lamy, P. L.;Rodrigo, R.;Koschny, D.;Rickman, H.;A’Hearn, M. F.;Barucci, M. A.;Bertaux, J.-L.;Bertini, I.;Cremonese, G.;Da Deppo, V.;Debei, S.;de Cecco, M.;Fulle, M.;Groussin, O.;Gutierrez, P. J.;Kramm, J.-R.;Küppers, M.;Lara, L. M.;Lazzarin, M.;Lopez Moreno, J. J.;Marzari, F.;Michalik, H.;Naletto, G.;Agarwal, J.;Güttler, C.;Oklay, N.;Tubiana, C.
    Contributors: 理學院天文研究所
    Keywords: Astrophysics;Comet nuclei;comets: individual: 67P/Churyumov-Gerasimenko;Earth and Planetary Astrophysics;Gas density;hydrodynamics;Imaging;Mathematical models;Nuclei;Ripples;Sciences of the Universe;space vehicles: instruments;techniques: image processing;Thermal properties;Transport
    Date: 2015-11-01
    Issue Date: 2026-04-21 14:41:17 (UTC+8)
    Publisher: EDP Sciences
    Abstract: 摘要: Context. We present an investigation of the surface properties of areas on the nucleus of comet 67P/Churyumov-Gerasimenko. Aims. We aim to show that transport of material from one part of the cometary nucleus to another is a significant mechanism that influences the appearance of the nucleus and the surface thermal properties. Methods. We used data from the OSIRIS imaging system onboard the Rosetta spacecraft to identify surface features on the nucleus that can be produced by various transport mechanisms. We used simple calculations based on previous works to establish the plausibility of dust transport from one part of the nucleus to another. Results. We show by observation and modeling that “airfall” as a consequence of non-escaping large particles emitted from the neck region of the nucleus is a plausible explanation for the smooth thin deposits in the northern hemisphere of the nucleus. The consequences are also discussed. We also present observations of aeolian ripples and ventifacts. We show by numerical modeling that a type of saltation is plausible even under the rarified gas densities seen at the surface of the nucleus. However, interparticle cohesive forces present difficulties for this model, and an alternative mechanism for the initiation of reptation and creep may result from the airfall mechanism. The requirements on gas density and other parameters of this alternative make it a more attractive explanation for the observations. The uncertainties and implications are discussed.
    出版者: EDP Sciences
    出版日期: 2015-11-01
    出處: Astronomy & Astrophysics, 2015-11, Vol.583, p.A17-
    資源來源: EDP Sciences
    版權: CC0 1.0 - Universal
    識別號: ISSN: 0004-6361
    識別號: ISSN: 1432-0746
    識別號: EISSN: 1432-0746
    識別號: DOI: 10.1051/0004-6361/201526049
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

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