Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun

Alessra Rotundi; Holger Sierks; Vincenzo Della Corte; Marco Fulle; Pedro J. Gutierrez; Luisa Lara; Cesare Barbieri; Philippe L. Lamy; Rafael Rodrigo; Detlef Koschny; Hans Rickman; Horst Uwe Keller; José J. López-Moreno; Mario Accolla; Jessica Agarwal; Michael F. A'Hearn; Nicolas Altobelli; Francesco Angrilli; M. Antonietta Barucci; Jean Loup Bertaux; Ivano Bertini; Dennis Bodewits; Ezio Bussoletti; Luigi Colangeli; Massimo Cosi; Gabriele Cremonese; Jean Francois Crifo; Vania Da Deppo; Björn Davidsson; Stefano Debei; Mariolino De Cecco; Francesca Esposito; Marco Ferrari; Sonia Fornasier; Frank Giovane; Bo Gustafson; Simon F. Green; Olivier Groussin; Eberhard Grün; Carsten Güttler; Miguel L. Herranz; Stubbe F. Hviid; Wing Ip; Stavro Ivanovski; José M. Jerónimo; Laurent Jorda; Joerg Knollenberg; Rainer Kramm; Ekkehard Kührt; Michael Küppers; Monica Lazzarin; Mark R. Leese; Antonio C. López-Jiménez; Francesca Lucarelli; Stephen C. Lowry; Francesco Marzari; Elena Mazzotta Epifani; J. Anthony M. McDonnell; Vito Mennella; Harald Michalik; Antonio Molina; Rafael Morales; Ferno Moreno; Stefano Mottola; Giampiero Naletto; Nilda Oklay; José L. Ortiz; Ernesto Palomba; Pasquale Palumbo; Jean Marie Perrin; Julio Rodríguez; Lola Sabau; Colin Snodgrass; Roberto Sordini; Nicolas Thomas; Cecilia Tubiana; Jean Baptiste Vincent; Paul Weissman; Klaus Peter Wenzel; Vladimir Zakharov; John C. Zarnecki

doi:10.1126/science.aaa3905

Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun

Alessra Rotundi, Holger Sierks, Vincenzo Della Corte, Marco Fulle, Pedro J. Gutierrez, Luisa Lara, Cesare Barbieri, Philippe L. Lamy, Rafael Rodrigo, Detlef Koschny, Hans Rickman, Horst Uwe Keller, José J. López-Moreno, Mario Accolla, Jessica Agarwal, Michael F. A'Hearn, Nicolas Altobelli, Francesco Angrilli, M. Antonietta Barucci, Jean Loup BertauxIvano Bertini, Dennis Bodewits, Ezio Bussoletti, Luigi Colangeli, Massimo Cosi, Gabriele Cremonese, Jean Francois Crifo, Vania Da Deppo, Björn Davidsson, Stefano Debei, Mariolino De Cecco, Francesca Esposito, Marco Ferrari, Sonia Fornasier, Frank Giovane, Bo Gustafson, Simon F. Green, Olivier Groussin, Eberhard Grün, Carsten Güttler, Miguel L. Herranz, Stubbe F. Hviid, Wing Ip, Stavro Ivanovski, José M. Jerónimo, Laurent Jorda, Joerg Knollenberg, Rainer Kramm, Ekkehard Kührt, Michael Küppers, Monica Lazzarin, Mark R. Leese, Antonio C. López-Jiménez, Francesca Lucarelli, Stephen C. Lowry, Francesco Marzari, Elena Mazzotta Epifani, J. Anthony M. McDonnell, Vito Mennella, Harald Michalik, Antonio Molina, Rafael Morales, Ferno Moreno, Stefano Mottola, Giampiero Naletto, Nilda Oklay, José L. Ortiz, Ernesto Palomba, Pasquale Palumbo, Jean Marie Perrin, Julio Rodríguez, Lola Sabau, Colin Snodgrass, Roberto Sordini, Nicolas Thomas, Cecilia Tubiana, Jean Baptiste Vincent, Paul Weissman, Klaus Peter Wenzel, Vladimir Zakharov, John C. Zarnecki

Graduate Institute of Astronomy

Research output: Contribution to journal › Article › peer-review

296 Scopus citations

Abstract

Critical measurements for understanding accretion and the dust/gas ratio in the solar nebula, where planets were forming 4.5 billion years ago, are being obtained by the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko. Between 3.6 and 3.4 astronomical units inbound, GIADA and OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) detected 35 outflowing grains of mass 10^-10 to 10^-7 kilograms, and 48 grains of mass 10^-5 to 10^-2 kilograms, respectively. Combined with gas data from the MIRO (Microwave Instrument for the Rosetta Orbiter) and ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) instruments, we find a dust/gas mass ratio of 4 ± 2 averaged over the sunlit nucleus surface. A cloud of larger grains also encircles the nucleus in bound orbits from the previous perihelion. The largest orbiting clumps are meter-sized, confirming the dust/gas ratio of 3 inferred at perihelion from models of dust comae and trails.

Original language	English
Article number	aaa3905
Journal	Science
Volume	347
Issue number	6220
DOIs	https://doi.org/10.1126/science.aaa3905
State	Published - 23 Jan 2015

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Rotundi, A., Sierks, H., Della Corte, V., Fulle, M., Gutierrez, P. J., Lara, L., Barbieri, C., Lamy, P. L., Rodrigo, R., Koschny, D., Rickman, H., Keller, H. U., López-Moreno, J. J., Accolla, M., Agarwal, J., A'Hearn, M. F., Altobelli, N., Angrilli, F., Barucci, M. A., ... Zarnecki, J. C. (2015). Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun. Science, 347(6220), [aaa3905]. https://doi.org/10.1126/science.aaa3905

@article{09a95353ebdd4c5892c824573a13bc92,

title = "Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun",

abstract = "Critical measurements for understanding accretion and the dust/gas ratio in the solar nebula, where planets were forming 4.5 billion years ago, are being obtained by the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko. Between 3.6 and 3.4 astronomical units inbound, GIADA and OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) detected 35 outflowing grains of mass 10-10 to 10-7 kilograms, and 48 grains of mass 10-5 to 10-2 kilograms, respectively. Combined with gas data from the MIRO (Microwave Instrument for the Rosetta Orbiter) and ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) instruments, we find a dust/gas mass ratio of 4 ± 2 averaged over the sunlit nucleus surface. A cloud of larger grains also encircles the nucleus in bound orbits from the previous perihelion. The largest orbiting clumps are meter-sized, confirming the dust/gas ratio of 3 inferred at perihelion from models of dust comae and trails.",

author = "Alessra Rotundi and Holger Sierks and {Della Corte}, Vincenzo and Marco Fulle and Gutierrez, {Pedro J.} and Luisa Lara and Cesare Barbieri and Lamy, {Philippe L.} and Rafael Rodrigo and Detlef Koschny and Hans Rickman and Keller, {Horst Uwe} and L{\'o}pez-Moreno, {Jos{\'e} J.} and Mario Accolla and Jessica Agarwal and A'Hearn, {Michael F.} and Nicolas Altobelli and Francesco Angrilli and Barucci, {M. Antonietta} and Bertaux, {Jean Loup} and Ivano Bertini and Dennis Bodewits and Ezio Bussoletti and Luigi Colangeli and Massimo Cosi and Gabriele Cremonese and Crifo, {Jean Francois} and {Da Deppo}, Vania and Bj{\"o}rn Davidsson and Stefano Debei and {De Cecco}, Mariolino and Francesca Esposito and Marco Ferrari and Sonia Fornasier and Frank Giovane and Bo Gustafson and Green, {Simon F.} and Olivier Groussin and Eberhard Gr{\"u}n and Carsten G{\"u}ttler and Herranz, {Miguel L.} and Hviid, {Stubbe F.} and Wing Ip and Stavro Ivanovski and Jer{\'o}nimo, {Jos{\'e} M.} and Laurent Jorda and Joerg Knollenberg and Rainer Kramm and Ekkehard K{\"u}hrt and Michael K{\"u}ppers and Monica Lazzarin and Leese, {Mark R.} and L{\'o}pez-Jim{\'e}nez, {Antonio C.} and Francesca Lucarelli and Lowry, {Stephen C.} and Francesco Marzari and Epifani, {Elena Mazzotta} and McDonnell, {J. Anthony M.} and Vito Mennella and Harald Michalik and Antonio Molina and Rafael Morales and Ferno Moreno and Stefano Mottola and Giampiero Naletto and Nilda Oklay and Ortiz, {Jos{\'e} L.} and Ernesto Palomba and Pasquale Palumbo and Perrin, {Jean Marie} and Julio Rodr{\'i}guez and Lola Sabau and Colin Snodgrass and Roberto Sordini and Nicolas Thomas and Cecilia Tubiana and Vincent, {Jean Baptiste} and Paul Weissman and Wenzel, {Klaus Peter} and Vladimir Zakharov and Zarnecki, {John C.}",

year = "2015",

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doi = "10.1126/science.aaa3905",

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volume = "347",

journal = "Science",

issn = "0036-8075",

number = "6220",

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Rotundi, A, Sierks, H, Della Corte, V, Fulle, M, Gutierrez, PJ, Lara, L, Barbieri, C, Lamy, PL, Rodrigo, R, Koschny, D, Rickman, H, Keller, HU, López-Moreno, JJ, Accolla, M, Agarwal, J, A'Hearn, MF, Altobelli, N, Angrilli, F, Barucci, MA, Bertaux, JL, Bertini, I, Bodewits, D, Bussoletti, E, Colangeli, L, Cosi, M, Cremonese, G, Crifo, JF, Da Deppo, V, Davidsson, B, Debei, S, De Cecco, M, Esposito, F, Ferrari, M, Fornasier, S, Giovane, F, Gustafson, B, Green, SF, Groussin, O, Grün, E, Güttler, C, Herranz, ML, Hviid, SF, Ip, W, Ivanovski, S, Jerónimo, JM, Jorda, L, Knollenberg, J, Kramm, R, Kührt, E, Küppers, M, Lazzarin, M, Leese, MR, López-Jiménez, AC, Lucarelli, F, Lowry, SC, Marzari, F, Epifani, EM, McDonnell, JAM, Mennella, V, Michalik, H, Molina, A, Morales, R, Moreno, F, Mottola, S, Naletto, G, Oklay, N, Ortiz, JL, Palomba, E, Palumbo, P, Perrin, JM, Rodríguez, J, Sabau, L, Snodgrass, C, Sordini, R, Thomas, N, Tubiana, C, Vincent, JB, Weissman, P, Wenzel, KP, Zakharov, V & Zarnecki, JC 2015, 'Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun', Science, vol. 347, no. 6220, aaa3905. https://doi.org/10.1126/science.aaa3905

TY - JOUR

T1 - Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun

AU - Rotundi, Alessra

AU - Sierks, Holger

AU - Della Corte, Vincenzo

AU - Fulle, Marco

AU - Gutierrez, Pedro J.

AU - Lara, Luisa

AU - Barbieri, Cesare

AU - Lamy, Philippe L.

AU - Rodrigo, Rafael

AU - Koschny, Detlef

AU - Rickman, Hans

AU - Keller, Horst Uwe

AU - López-Moreno, José J.

AU - Accolla, Mario

AU - Agarwal, Jessica

AU - A'Hearn, Michael F.

AU - Altobelli, Nicolas

AU - Angrilli, Francesco

AU - Barucci, M. Antonietta

AU - Bertaux, Jean Loup

AU - Bertini, Ivano

AU - Bodewits, Dennis

AU - Bussoletti, Ezio

AU - Colangeli, Luigi

AU - Cosi, Massimo

AU - Cremonese, Gabriele

AU - Crifo, Jean Francois

AU - Da Deppo, Vania

AU - Davidsson, Björn

AU - Debei, Stefano

AU - De Cecco, Mariolino

AU - Esposito, Francesca

AU - Ferrari, Marco

AU - Fornasier, Sonia

AU - Giovane, Frank

AU - Gustafson, Bo

AU - Green, Simon F.

AU - Groussin, Olivier

AU - Grün, Eberhard

AU - Güttler, Carsten

AU - Herranz, Miguel L.

AU - Hviid, Stubbe F.

AU - Ip, Wing

AU - Ivanovski, Stavro

AU - Jerónimo, José M.

AU - Jorda, Laurent

AU - Knollenberg, Joerg

AU - Kramm, Rainer

AU - Kührt, Ekkehard

AU - Küppers, Michael

AU - Lazzarin, Monica

AU - Leese, Mark R.

AU - López-Jiménez, Antonio C.

AU - Lucarelli, Francesca

AU - Lowry, Stephen C.

AU - Marzari, Francesco

AU - Epifani, Elena Mazzotta

AU - McDonnell, J. Anthony M.

AU - Mennella, Vito

AU - Michalik, Harald

AU - Molina, Antonio

AU - Morales, Rafael

AU - Moreno, Ferno

AU - Mottola, Stefano

AU - Naletto, Giampiero

AU - Oklay, Nilda

AU - Ortiz, José L.

AU - Palomba, Ernesto

AU - Palumbo, Pasquale

AU - Perrin, Jean Marie

AU - Rodríguez, Julio

AU - Sabau, Lola

AU - Snodgrass, Colin

AU - Sordini, Roberto

AU - Thomas, Nicolas

AU - Tubiana, Cecilia

AU - Vincent, Jean Baptiste

AU - Weissman, Paul

AU - Wenzel, Klaus Peter

AU - Zakharov, Vladimir

AU - Zarnecki, John C.

PY - 2015/1/23

Y1 - 2015/1/23

N2 - Critical measurements for understanding accretion and the dust/gas ratio in the solar nebula, where planets were forming 4.5 billion years ago, are being obtained by the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko. Between 3.6 and 3.4 astronomical units inbound, GIADA and OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) detected 35 outflowing grains of mass 10-10 to 10-7 kilograms, and 48 grains of mass 10-5 to 10-2 kilograms, respectively. Combined with gas data from the MIRO (Microwave Instrument for the Rosetta Orbiter) and ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) instruments, we find a dust/gas mass ratio of 4 ± 2 averaged over the sunlit nucleus surface. A cloud of larger grains also encircles the nucleus in bound orbits from the previous perihelion. The largest orbiting clumps are meter-sized, confirming the dust/gas ratio of 3 inferred at perihelion from models of dust comae and trails.

AB - Critical measurements for understanding accretion and the dust/gas ratio in the solar nebula, where planets were forming 4.5 billion years ago, are being obtained by the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko. Between 3.6 and 3.4 astronomical units inbound, GIADA and OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) detected 35 outflowing grains of mass 10-10 to 10-7 kilograms, and 48 grains of mass 10-5 to 10-2 kilograms, respectively. Combined with gas data from the MIRO (Microwave Instrument for the Rosetta Orbiter) and ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) instruments, we find a dust/gas mass ratio of 4 ± 2 averaged over the sunlit nucleus surface. A cloud of larger grains also encircles the nucleus in bound orbits from the previous perihelion. The largest orbiting clumps are meter-sized, confirming the dust/gas ratio of 3 inferred at perihelion from models of dust comae and trails.

UR - http://www.scopus.com/inward/record.url?scp=84922021901&partnerID=8YFLogxK

U2 - 10.1126/science.aaa3905

DO - 10.1126/science.aaa3905

M3 - 期刊論文

AN - SCOPUS:84922021901

SN - 0036-8075

VL - 347

JO - Science

JF - Science

IS - 6220

M1 - aaa3905

ER -

Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the sun

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