Sylvain Bouley

ORCID: 0000-0003-0377-5517
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About
Contact & Profiles
Research Areas
  • Planetary Science and Exploration
  • Astro and Planetary Science
  • Geology and Paleoclimatology Research
  • Space Exploration and Technology
  • Marine and environmental studies
  • Stellar, planetary, and galactic studies
  • Solar and Space Plasma Dynamics
  • Space Science and Extraterrestrial Life
  • Image Processing and 3D Reconstruction
  • Advanced Photonic Communication Systems
  • History of Computing Technologies
  • Transboundary Water Resource Management
  • Methane Hydrates and Related Phenomena
  • Metallurgy and Cultural Artifacts
  • earthquake and tectonic studies
  • Geological and Geophysical Studies Worldwide
  • Isotope Analysis in Ecology
  • Geological and Geochemical Analysis
  • Ionosphere and magnetosphere dynamics
  • Gamma-ray bursts and supernovae
  • Astronomical Observations and Instrumentation
  • Space Satellite Systems and Control
  • History and Developments in Astronomy
  • GNSS positioning and interference
  • Geophysics and Gravity Measurements

Institut de Mécanique Céleste et de Calcul des Éphémérides
2015-2024

Geosciences Paris-Saclay
2015-2024

Université Paris-Saclay
2015-2024

Centre National de la Recherche Scientifique
2015-2024

Université Paris-Sud
2014-2023

Observatoire de Paris
2020-2023

Institut Universitaire de France
2022

Observatoire Midi-Pyrénées
2007-2021

Roche (France)
2012-2021

Université Paris Sciences et Lettres
2019-2021

Abstract The identification of lobate debris deposits in Arabia Terra, along the proposed paleoshoreline a former northern ocean, has renewed questions about existence and stability ocean‐sized body water early geologic history Mars. potential occurrence impact‐generated tsunamis ocean was investigated by comparing geomorphologic characteristics Martian with predictions well‐validated terrestrial models (scaled to Mars) tsunami wave height, propagation direction, runup elevation, distance...

10.1002/2016je005230 article EN Journal of Geophysical Research Planets 2017-03-01
A. J. King Luke Daly James B. Rowe K. H. Joy R. C. Greenwood and 95 more Hadrien A. R. Devillepoix Martin D. Suttle Q. H. S. Chan S. S. Russell H. C. Bates J. F. J. Bryson P. L. Clay Denis Vida Martin Lee Áine O’Brien L. J. Hallis N. R. Stephen Romain Tartèse Eleanor K. Sansom M. C. Towner Martin Cupák Patrick Shober P. A. Bland Ross Findlay I. A. Franchi A. B. Verchovsky F. A. J. Abernethy M. M. Grady Cameron J. Floyd Matthias Van Ginneken J. C. Bridges L. J. Hicks R. H. Jones Jennifer T. Mitchell M. J. Genge Laura E. Jenkins Pierre‐Etienne Martin Mark A. Sephton Jonathan S. Watson T. Salge K. A. Shirley R. J. Curtis T. Warren Neil E. Bowles Finlay M. Stuart Luigia Di Nicola Domokos Györe Adrian J. Boyce Kathryn M. M. Shaw Tim Elliott Robert C. Steele Pavel P. Povinec M. Laubenstein D.C.W. Sanderson A.J. Cresswell A. J. T. Jull I. Sýkora Sanjana Sridhar R. J. Harrison Francesca M. Willcocks Catherine S. Harrison Daniel Hallatt P. J. Wozniakiewicz M. J. Burchell Luke S. Alesbrook Aishling Dignam N. V. Almeida C. L. Smith Brett Clark Emma Humphreys‐Williams P. F. Schofield Luke T. Cornwell Vassilia Spathis Geraint Morgan Mark J. Perkins Richard Kacerek Peter Campbell‐Burns F. Colas B. Zanda P. Vernazza Sylvain Bouley Simon Jeanne Mike Hankey G. S. Collins J. S. Young Clive Shaw Jana Horák Dave Jones Nick James Steve Bosley Alan Shuttleworth Paul Dickinson Ian McMullan Derek Robson Andrew R. D. Smedley Ben Stanley Richard Bassom Mark McIntyre Adam Suttle Richard Fleet

Direct links between carbonaceous chondrites and their parent bodies in the solar system are rare. The Winchcombe meteorite is most accurately recorded chondrite fall. Its pre-atmospheric orbit cosmic-ray exposure age confirm that it arrived on Earth shortly after ejection from a primitive asteroid. Recovered only hours falling, composition of largely unmodified by terrestrial environment. It contains abundant hydrated silicates formed during fluid-rock reactions, carbon- nitrogen-bearing...

10.1126/sciadv.abq3925 article EN cc-by-nc Science Advances 2022-11-16

Context . The source regions of ordinary chondrites (~80% all falls) and large S-type near-Earth objects (NEOs; ~30%) have recently been identified with three young asteroid families (Karin, Koronis, Massalia) being at the origin most chondrite falls. Aims present work is a continuation our previous studies aims to determine remaining meteorite NEO classes, an emphasis on carbonaceous (CM, CI, CO, CV, CK, CR, CH, CB, or C-ungrouped). Methods We studied 38 individual families, including old...

10.1051/0004-6361/202450532 article EN cc-by Astronomy and Astrophysics 2024-07-25

Context. Asteroid modeling efforts in the last decade resulted a comprehensive dataset of almost 400 convex shape models and their rotation states. These already provided deep insight into physical properties main-belt asteroids or large collisional families. Going finer detail (e.g., smaller families, with sizes ≲20 km) requires knowledge parameters more objects.

10.1051/0004-6361/201527441 article EN Astronomy and Astrophysics 2015-11-09

In the eastern part of Arabia Terra cratered boundary, lobate deposits are observed on top north-sloping highland mesas. Our previous studies (Rodriguez et al., 2016; Costard 2017) suggest that most plausible origin for these morphologies tsunami associated with Lomonosov impact event in an Hesperian age ocean (Costard 2019). Tsunami Earth serve as valuable analogs interpreting possible tsunami-related features Mars, especially regarding hypothesized ancient oceans. this study, we examine...

10.5194/egusphere-egu25-9022 preprint EN 2025-03-14

Farside Explorer is a proposed Cosmic Vision medium-size mission to the farside of Moon consisting two landers and an instrumented relay satellite. The unique scientific platform in that it shielded from terrestrial radio-frequency interference, recorded primary differentiation evolution Moon, can be continuously monitored Earth–Moon L2 Lagrange point, there complete lack reflected solar illumination Earth. will exploit these properties make first radio-astronomy measurements most...

10.1007/s10686-011-9252-3 article EN cc-by-nc Experimental Astronomy 2011-10-26

Abstract The formation and differentiation of the crust Mars in first tens millions years after its accretion can only be deciphered from incredibly limited records. martian breccia NWA 7034 paired stones is one them. This meteorite contains oldest igneous material ever dated: ~4.5 Ga old. However, source geological context have so far remained unknown. Here, we show that was ejected 5–10 Ma ago north-east Terra Cimmeria—Sirenum province, southern hemisphere Mars. More specifically, belongs...

10.1038/s41467-022-31444-8 article EN cc-by Nature Communications 2022-07-12

What was the nature of Late Hesperian climate? Warm and wet or cold dry? Formulated this way question leads to an apparent paradox since both options seem implausible. A warm climate would have produced extensive fluvial erosion but few valley networks been observed at age late Hesperian. too kept any northern ocean frozen most time. moderate transferred water from land in form snow ice. But prevent tsunami formation, for which there is some evidence. Here, we provide new insights numerical...

10.1073/pnas.2112930118 article EN cc-by-nc-nd Proceedings of the National Academy of Sciences 2022-01-18

Abstract This work in Utopia Planitia is the first continuous regional mapping of ice‐related landforms integrated into an effort to study three main basins (Arcadia, Acidalia, and Planitiae) northern plains. The distribution morphotypes these landforms, SHAllow RADar detections, crater size‐frequency measurements (>50 m diameter) were used understand permafrost cryolithology its past evolution relation climate Planitia. Three assemblages identified based on their spatial correlation with...

10.1029/2018je005665 article EN Journal of Geophysical Research Planets 2018-09-13

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

10.1093/mnras/staa3646 article EN Monthly Notices of the Royal Astronomical Society 2020-11-20

Determining the source regions of meteorites is one major goals current research in planetary science. Whereas asteroid observations are currently unable to pinpoint most meteorite classes, meteors with camera networks and subsequent recovery may help make progress on this question. The main caveat such an approach, however, that rate falls low, implying meteoritic analogues at least 80% observed remain unknown. Aims: Spectroscopic bolides have potential mitigate problem by classifying...

10.1051/0004-6361/201732225 article EN cc-by Astronomy and Astrophysics 2018-02-05

Abstract Recent research suggests that major meteorite impact events into a Late Hesperian/Early Amazonian ocean likely produced mega‐tsunami would have resurfaced coastal areas in northwestern Arabia Terra. The orientations of the associated lobate deposits, conspicuous type landforms called Thumbprint Terrain, if an event triggered mega‐tsunami, most location source crater is within northern plains regions situated north This study focuses on identification craters impacted and are to...

10.1029/2019je006008 article EN publisher-specific-oa Journal of Geophysical Research Planets 2019-06-26
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