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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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Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes.

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.
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Instrumental methods for professional and amateur collaborations in planetary astronomy

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.
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Scientific rationale for Saturn's in situ exploration

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.
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Methane clathrates in the solar system.

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.