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Sökning: onr:"swepub:oai:DiVA.org:uu-295585" > The dust environmen...

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FältnamnIndikatorerMetadata
00009638naa a2200973 4500
001oai:DiVA.org:uu-295585
003SwePub
008160608s2016 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-2955852 URI
024a https://doi.org/10.1051/0004-6361/2015275642 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Moreno, F.u CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain.4 aut
2451 0a The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inbound
264 c 2016-03-07
264 1b EDP Sciences,c 2016
338 a print2 rdacarrier
520 a Context: The ESA Rosetta spacecraft, currently orbiting around cornet 67P/Churyumov-Gerasimenko, has already provided in situ measurements of the dust grain properties from several instruments, particularly OSIRIS and GIADA. We propose adding value to those measurements by combining them with ground-based observations of the dust tail to monitor the overall, time-dependent dust-production rate and size distribution.Aims: To constrain the dust grain properties, we take Rosetta OSIRIS and GIADA results into account, and combine OSIRIS data during the approach phase (from late April to early June 2014) with a large data set of ground-based images that were acquired with the ESO Very Large Telescope (VLT) from February to November 2014.Methods: A Monte Carlo dust tail code, which has already been used to characterise the dust environments of several comets and active asteroids, has been applied to retrieve the dust parameters. Key properties of the grains (density, velocity, and size distribution) were obtained from. Rosetta observations: these parameters were used as input of the code to considerably reduce the number of free parameters. In this way, the overall dust mass-loss rate and its dependence on the heliocentric distance could be obtained accurately.Results: The dust parameters derived from the inner coma measurements by OSIRIS and GIADA and from distant imaging using VLT data are consistent, except for the power index of the size-distribution function, which is alpha = -3, instead of alpha = -2, for grains smaller than 1 mm. This is possibly linked to the presence of fluffy aggregates in the coma. The onset of cometary activity occurs at approximately 4.3 AU, with a dust production rate of 0.5 kg/s, increasing up to 15 kg/s at 2.9 AU. This implies a dust-to-gas mass ratio varying between 3.8 and 6.5 for the best-fit model when combined with water-production rates from the MIRO experiment.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a comets: individual: 67P/Churyumov-Gerasimenko
653 a methods: data analysis
653 a techniques: photometric
700a Snodgrass, C.u Open Univ, Dept Phys Sci, Planetary & Space Sci, Walton Hall, Milton Keynes MK7 6AA, Bucks, England.4 aut
700a Hainaut, O.u European So Observ, Karl Schwarschild Str 2, D-85748 Garching, Germany.4 aut
700a Tubiana, C.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Sierks, H.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Barbieri, C.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy.;Univ Padua, Ctr Studies & Activ Space CISAS G Colombo, Via Venezia 15, I-35131 Padua, Italy.4 aut
700a Lamy, P. L.u Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.4 aut
700a Rodrigo, R.u European Space Agcy, European Space Astron Ctr, Ctr Astrobiol INTA CSIC, POB 78, Madrid 28691, Spain.;Int Space Sci Inst, Hallerstr 6, CH-3012 Bern, Switzerland.4 aut
700a Koschny, D.u European Space Agcy, Res & Sci Support Dept, NL-2201 Noordwijk, Netherlands.4 aut
700a Rickman, Hansu Uppsala universitet,Teoretisk astrofysik,PAS Space Res Ctr, Bartycka 18A, PL-00716 Warsaw, Poland.4 aut0 (Swepub:uu)hansrick
700a Keller, H. U.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany.4 aut
700a Agarwal, J.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a A'Hearn, M. F.u Univ Maryland, Dept Astron, College Pk, MD 20742 USA.4 aut
700a Barucci, M. A.u Univ Paris Diderot, UPMC, CNRS, Observ Paris,LESIA, 5 Pl J Janssen, F-92195 Meudon, France.4 aut
700a Bertaux, J-Lu CNRS UVSQ IPSL, LATMOS, 11 Bd Alembert, F-78280 Guyancourt, France.4 aut
700a Bertini, I.u Univ Padua, Ctr Studies & Activ Space CISAS G Colombo, Via Venezia 15, I-35131 Padua, Italy.4 aut
700a Besse, S.u European Space Agcy, Res & Sci Support Dept, NL-2201 Noordwijk, Netherlands.4 aut
700a Bodewits, D.u Univ Maryland, Dept Astron, College Pk, MD 20742 USA.4 aut
700a Cremonese, G.u Osserv Astron Padova, INAF, Vic Osservatorio 5, I-35122 Padua, Italy.4 aut
700a Da Deppo, V.u CNR IFN UOS Padova LUXOR, Via Trasea 7, I-35131 Padua, Italy.4 aut
700a Davidsson, Björnu Uppsala universitet,Teoretisk astrofysik4 aut0 (Swepub:uu)bjoda312
700a Debei, S.u Univ Padua, Dept Ind Engn, Via Venezia 1, I-35131 Padua, Italy.4 aut
700a De Cecco, M.u Univ Trento, Via Sommarive 9, I-38123 Trento, Italy.4 aut
700a Ferri, F.u Univ Padua, Ctr Studies & Activ Space CISAS G Colombo, Via Venezia 15, I-35131 Padua, Italy.4 aut
700a Fornasier, S.u Univ Paris Diderot, UPMC, CNRS, Observ Paris,LESIA, 5 Pl J Janssen, F-92195 Meudon, France.4 aut
700a Fulle, M.u Osserv Astron Trieste, INAF, Via Tiepolo 11, I-34143 Trieste, Italy.4 aut
700a Groussin, O.u Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.4 aut
700a Gutierrez, P. J.u CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain.4 aut
700a Gutierrez-Marques, P.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Guettler, C.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Hviid, S. F.u DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany.4 aut
700a Ip, W. -H4 aut
700a Jorda, L.u Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.4 aut
700a Knollenberg, J.u DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany.4 aut
700a Kovacs, G.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Kramm, J. -R4 aut
700a Kuehrt, E.u DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany.4 aut
700a Kueppers, M.u ESA ESAC, POB 78, Villanueva De La Canada 28691, Spain.4 aut
700a Lara, L. M.u CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain.4 aut
700a Lazzarin, M.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy.4 aut
700a Lopez-Moreno, J. J.u CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain.4 aut
700a Marzari, F.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy.4 aut
700a Mottola, S.u DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany.4 aut
700a Naletto, G.u Univ Padua, Ctr Studies & Activ Space CISAS G Colombo, Via Venezia 15, I-35131 Padua, Italy.;CNR IFN UOS Padova LUXOR, Via Trasea 7, I-35131 Padua, Italy.;Univ Padua, Dept Informat Engn, Via Gradenigo 6-B, I-35131 Padua, Italy.4 aut
700a Oklay, N.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Pajola, M.u Univ Padua, Ctr Studies & Activ Space CISAS G Colombo, Via Venezia 15, I-35131 Padua, Italy.4 aut
700a Thomas, N.u Univ Bern, Inst Phys, Sidlerstr 5, CH-3012 Bern, Switzerland.4 aut
700a Vincent, J. B.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany.4 aut
700a Della Corte, V.u INAF, IAPS, Via Foss Lavaliere 100, I-00133 Rome, Italy.4 aut
700a Fitzsimmons, A.u Queens Univ Belfast, Sch Phys & Astron, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland.4 aut
700a Faggi, S.u Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy.4 aut
700a Jehin, E.u Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium.4 aut
700a Opitom, C.u Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium.4 aut
700a Tozzi, G-P4 aut
710a CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain.b Open Univ, Dept Phys Sci, Planetary & Space Sci, Walton Hall, Milton Keynes MK7 6AA, Bucks, England.4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 587q 587x 0004-6361x 1432-0746
856u https://www.aanda.org/articles/aa/pdf/2016/03/aa27564-15.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-295585
8564 8u https://doi.org/10.1051/0004-6361/201527564

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