0000000000134400

AUTHOR

Sylvain Bouley

showing 2 related works from this author

Cavezzo, the first Italian meteorite recovered by the PRISMA fireball network. Orbit, trajectory, and strewn-field

2020

ABSTRACT Two meteorite pieces have been recovered in Italy, near the town of Cavezzo (Modena), on 2020 January 4th. The associated fireball was observed on the evening of New Year’s Day 2020 by eight all-sky cameras of the PRISMA fireball network, a partner of FRIPON. The computed trajectory had an inclination angle of approximately 68° and a velocity at infinity of 12.8 km s−1. Together with the relatively low terminal height, estimated as 21.5 km, those values were indicating the significant possibility of a meteorite dropping event, as additionally confirmed by the non-zero residual total mass. The strewn-field was computed taking into account the presence of two bright light flashes, re…

meteoroids -methods: data analysis -techniques: image processing010502 geochemistry & geophysics01 natural sciencesStrewn fieldmeteorites0103 physical sciencesmeteorsmeteoroids010303 astronomy & astrophysicsmeteoroid0105 earth and related environmental sciencesPhysicsMeteoroidimage processing; meteorites; meteoroids; meteors; methods: data analysis; techniquesmeteorAstronomyAstronomy and Astrophysicsmethods: data analysismeteoriteimage processingMeteoriteSpace and Planetary Science[SDU]Sciences of the Universe [physics]data analysi [methods]TrajectoryOrbit (control theory)techniques
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Martian zeolites as a source of atmospheric methane

2016

The origin of the martian methane is still poorly understood. A plausible explanation is that methane could have been produced either by hydrothermal alteration of basaltic crust or by serpentinization of ultramafic rocks producing hydrogen and reducing crustal carbon into methane. Once formed, methane storage on Mars is commonly associated with the presence of hidden clathrate reservoirs. Here, we alternatively suggest that chabazite and clinoptilolite, which belong to the family of zeolites, may form a plausible storage reservoir of methane in the martian subsurface. Because of the existence of many volcanic terrains, zeolites are expected to be widespread on Mars and their Global Equival…

Chabazite010504 meteorology & atmospheric sciencesClathrate hydrateFOS: Physical sciences01 natural sciencesMethaneAstrobiologychemistry.chemical_compound0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)BasaltMartianAtmospheric methaneAstronomy and AstrophysicsMars Exploration ProgramAtmosphere of Marschemistry13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Environmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][ SDU ] Sciences of the Universe [physics]Astrophysics - Earth and Planetary Astrophysics
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