Search Results - "Raymond, S. N"

Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1 by Bolmont, E, Selsis, F, Owen, J E, Ribas, I, Raymond, S N, Leconte, J, Gillon, M

“…Ultracool dwarfs (UCD; T^sub eff^ < ~3000 K) cool to settle on the main sequence after ~1 Gyr. For brown dwarfs, this cooling never stops. Their habitable…”
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Populating the asteroid belt from two parent source regions due to the migration of giant planets-"The Grand Tack" by WALSH, Kevin J., MORBIDELLI, A., RAYMOND, S. N., O'BRIEN, D. P., MANDELL, A. M.

“…– The asteroid belt is found today in a dramatically different state than that immediately following its formation. It is estimated that it has been depleted…”
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Dry late accretion inferred from Venus’s coupled atmosphere and internal evolution by Gillmann, C., Golabek, G. J., Raymond, S. N., Schönbächler, M., Tackley, P. J., Dehant, V., Debaille, V.

“…It remains contentious whether the meteoritic material delivered to the terrestrial planets after the end of core formation was rich or poor in water and other…”
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Building Terrestrial Planets by Morbidelli, A, Lunine, J.I, O'Brien, D.P, Raymond, S.N, Walsh, K.J

“…This article reviews our current understanding of terrestrial planet formation. The focus is on computer simulations of the dynamical aspects of the accretion…”
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No evidence for interstellar planetesimals trapped in the Solar system by Morbidelli, A, Batygin, K, Brasser, R, Raymond, S N

“…ABSTRACT In two recent papers published in MNRAS, Namouni and Morais claimed evidence for the interstellar origin of some small Solar system bodies, including:…”
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A record of the final phase of giant planet migration fossilized in the asteroid belt’s orbital structure by Clement, Matthew S, Morbidelli, A, Raymond, S N, Kaib, N A

“…ABSTRACT The asteroid belt is characterized by an extreme low total mass of material on dynamically excited orbits. The Nice model explains many peculiar…”
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Vortex instabilities triggered by low-mass planets in pebble-rich, inviscid protoplanetary discs by Pierens, A, Lin, M-K, Raymond, S N

“…Abstract In the innermost regions of protoplanerary discs, the solid-to-gas ratio can be increased considerably by a number of processes, including…”
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Migration of Accreting Planets in Radiative Discs From Dynamical Torques by Pierens, A, Raymond, S N

“…We present the results of hydrodynamical simulations of the orbital evolution of planets undergoing runaway gas accretion in radiative discs. We consider…”
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Disruption of co-orbital (1:1) planetary resonances during gas-driven orbital migration by Pierens, A., Raymond, S. N.

“…Planets close to their stars are thought to form farther out and migrate inwards due to angular momentum exchange with gaseous protoplanetary discs. This…”
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Planetesimal-driven migration as an explanation for observations of high levels of warm, exozodiacal dust by Bonsor, Amy, Raymond, Sean N., Augereau, Jean-Charles, Ormel, Chris W.

“…High levels of exozodiacal dust have been observed in the inner regions of a large fraction of main-sequence stars. Given the short lifetime of the observed…”
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The extreme physical properties of the CoRoT-7b super-Earth by Léger, A., Grasset, O., Fegley, B., Codron, F., Albarede, A.F., Barge, P., Barnes, R., Cance, P., Carpy, S., Catalano, F., Cavarroc, C., Demangeon, O., Ferraz-Mello, S., Gabor, P., Grießmeier, J.-M., Leibacher, J., Libourel, G., Maurin, A.-S., Raymond, S.N., Rouan, D., Samuel, B., Schaefer, L., Schneider, J., Schuller, P.A., Selsis, F., Sotin, C.

“…► We discuss the extreme physical properties possible for CoRoT-7b and Kepler-10b. ► We make the working hypothesis that the planets are rocky, with no…”
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Making other earths: dynamical simulations of terrestrial planet formation and water delivery by Raymond, Sean N, Quinn, Thomas, Lunine, Jonathan I

“…We present results from 44 simulations of late stage planetary accretion, focusing on the delivery of volatiles (primarily water) to the terrestrial planets…”
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Terrestrial Planet Formation in Disks with Varying Surface Density Profiles by Raymond, Sean N, Quinn, Thomas, Lunine, Jonathan I

“…The minimum-mass solar nebula (MMSN) model estimates the surface density distribution of the protoplanetary disk by assuming the planets to have formed in…”
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Predicting Planets in Known Extrasolar Planetary Systems. I. Test Particle Simulations by Barnes, Rory, Raymond, Sean N

“…Recent work has suggested that many planetary systems lie near instability. If all systems are near instability, then at least one additional planet must exist…”
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Predicting Planets in Known Extrasolar Planetary Systems. II. Testing for Saturn Mass Planets by Raymond, Sean N, Barnes, Rory

“…Recent results have shown that many of the known extrasolar planetary systems contain regions that are stable for massless test particles. We examine the…”
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The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth by L, Allibert, J, Siebert, S, Charnoz, A, Jacobson S, N, Raymond S

“…Impact-induced erosion of the Earth's early crust during accretion of terrestrial bodies can significantly modify the primordial chemical composition of the…”
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Influence of planetary gas accretion on the shape and depth of gaps in protoplanetary discs by Bergez-Casalou, C, Bitsch, B, Pierens, A, Crida, A, Raymond, S. N

“…A&A 643, A133 (2020) It is widely known that giant planets have the capacity to open deep gaps in their natal gaseous protoplanetary discs. It is unclear,…”
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The effect of collisional erosion on the composition of Earth-analog planets in Grand Tack models: Implications for the formation of the Earth by Allibert, L., Siebert, J., Charnoz, S., Jacobson, S.A., Raymond, S.N.

“…Impact-induced erosion of the Earth’s early crust during accretion of terrestrial bodies can significantly modify the primordial chemical composition of the…”
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Dry Late Accretion inferred from Venus' coupled atmosphere and internal evolution by Gillmann, C, Golabek, G. J, Raymond, S. N, Schonbachler, M, Tackley, P. J, Dehant, V, Debaille, V

“…Nature Geoscience, 13(4), 265-269 (2020) The composition of meteoritic material delivered to the terrestrial planets after the end of core formation as late…”
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TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system by Timmermans, M, Dransfield, G, Gillon, M, Triaud, A. H. M. J, Rackham, B. V, Aganze, C, Barkaoui, K, Briceño, C, Burgasser, A. J, Collins, K. A, Cointepas, M, Dévora-Pajares, M, Ducrot, E, Zúñiga-Fernández, S, Howell, S. B, Kaltenegger, L, Murray, C. A, Pass, E. K, Quinn, S. N, Raymond, S. N, Sebastian, D, Stassun, K. G, Ziegler, C, Almenara, J. M, Benkhaldoun, Z, Bonfils, X, Christiansen, J. L, Davoudi, F, de Wit, J, Delrez, L, Demory, B. -O, Fong, W, Fűrész, G, Ghachoui, M, Garcia, L. J, Chew, Y. Gómez Maqueo, Hooton, M. J, Horne, K, Günther, M. N, Jehin, E, Jenkins, J. M, Law, N, Mann, A. W, Murgas, F, Pozuelos, F. J, Pedersen, P. P, Queloz, D, Ricker, G, Rowden, P, Schwarz, R. P, Seager, S, Smart, R. L, Srdoc, G, Striegel, S, Thompson, S, Vanderspek, R, Winn, J. N

“…A&A 687, A48 (2024) Small planets transiting bright nearby stars are essential to our understanding of the formation and evolution of exoplanetary systems…”
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