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Alexis Bouquet
Researcher at Aix-Marseille University
Publications - 38
Citations - 1180
Alexis Bouquet is an academic researcher from Aix-Marseille University. The author has contributed to research in topics: Enceladus & Comet. The author has an hindex of 15, co-authored 35 publications receiving 878 citations. Previous affiliations of Alexis Bouquet include University of Toulouse & Southwest Research Institute.
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Journal ArticleDOI
Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes.
J. Hunter Waite,Christopher R. Glein,Rebecca Perryman,Ben Teolis,Brian Magee,Greg Miller,J. Grimes,Mark E. Perry,Kelly E. Miller,Alexis Bouquet,Jonathan I. Lunine,Tim Brockwell,Scott Bolton +12 more
TL;DR: The Ion Neutral Mass Spectrometer onboard the Cassini spacecraft is used to detect molecular hydrogen in the plume of escaping material on Enceladus, finding that the most plausible source of this hydrogen is ongoing hydrothermal reactions of rock containing reduced minerals and organic materials.
Journal ArticleDOI
Instrumental methods for professional and amateur collaborations in planetary astronomy
Olivier Mousis,Ricardo Hueso,J.-P. Beaulieu,Sylvain Bouley,Benoit Carry,F. Colas,Alain Klotz,C. Pellier,J.-M. Petit,Philippe Rousselot,Mohamad Ali-Dib,W. Beisker,Mirel Birlan,C. Buil,A. Delsanti,E. Frappa,H. B. Hammel,Anny Chantal Levasseur-Regourd,G. S. Orton,Agustín Sánchez-Lavega,Alexandre Santerne,Paolo Tanga,Jeremie Vaubaillon,Brigitte Zanda,David Baratoux,T. Böhm,Vincent Boudon,Alexis Bouquet,L. Buzzi,Jean-Luc Dauvergne,Alice Decock,M. Delcroix,P. Drossart,N. Esseiva,Georg Fischer,Leigh N. Fletcher,S. Foglia,J. M. Gómez-Forrellad,J. Guarro-Flo,D. Herald,Emmanuel Jehin,F. Kugel,Jean-Pierre Lebreton,J. Lecacheux,A. Leroy,Laurent Maquet,G. Masi,Alain Maury,Fanny Meyer,Santiago Pérez-Hoyos,A. S. Rajpurohit,C. Rinner,John H. Rogers,F. Roques,R. W. Schmude,B. Sicardy,B. Tregon,M. Vanhuysse,A. Wesley,Thomas Widemann +59 more
TL;DR: Amateur contributions to professional publications have increased exponentially over the last decades in the field of planetary astronomy as discussed by the authors, and amateur contributions to the monitoring of planets and interplanetary matter, characterization of asteroids and comets, as well as the determination of the physical properties of Kuiper Belt Objects and exoplanets are discussed.
Journal ArticleDOI
Scientific rationale for Saturn's in situ exploration
O. Mousis,Leigh N. Fletcher,Jean-Pierre Lebreton,Peter Wurz,Thibault Cavalié,A. Coustenis,Régis Courtin,D. Gautier,Ravit Helled,Pgj Irwin,Andrew Morse,Nadine Nettelmann,Bernard Marty,Philippe Rousselot,Olivia Venot,David H. Atkinson,David H. Atkinson,J. H. Waite,K. Reh,Amy Simon,Sushil K. Atreya,N. André,Michel Blanc,Ioannis A. Daglis,Georg Fischer,W. D Geppertt,Tristan Guillot,Matthew M. Hedman,Ricardo Hueso,Emmanuel Lellouch,Jonathan I. Lunine,Carl D. Murray,James O'Donoghue,Miriam Rengel,Agustín Sánchez-Lavega,François-Xavier Schmider,Aymeric Spiga,T. R. Spilker,J. M. Petit,Matthew S. Tiscareno,Mohamad Ali-Dib,Kathrin Altwegg,Scott Bolton,Alexis Bouquet,C. Briois,Thierry Fouchet,S. Guerlet,T. Kostiuk,D Lebleu,R. Moreno,G. S. Orton,J. Poncy +51 more
TL;DR: In this paper, the main scientific goals to be addressed by the future in situ exploration of Saturn placing the Galileo probe exploration of Jupiter in a broader context and before the future Pluto exploration of the more remote ice giants.
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Possible evidence for a methane source in Enceladus' ocean
TL;DR: In this paper, the authors used a statistical thermodynamic model to assess which species detected in the plumes by the Cassini-Ion and Neutral Mass Spectrometer experiment are trapped in clathrates and found that the conditions for clathrate formation are met in this ocean, except above 20km or in hypothetical hot spots.
Journal ArticleDOI
Methane clathrates in the solar system.
Olivier Mousis,Eric Chassefière,Nils G. Holm,Alexis Bouquet,Jack H. Waite,Wolf D. Geppert,Sylvain Picaud,Yuri Aikawa,Mohamad Ali-Dib,Jean Luc Charlou,Philippe Rousselot +10 more
TL;DR: Thermodynamic equilibrium calculations show that methane-rich clathrate layers may exist on Pluto as well, and their presence is invoked in the satellite's subsurface as a means of replenishing its atmosphere with methane via outgassing episodes.