Search Results - "Grasset, O."

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  1. 1

    Mass–radius curve for extrasolar Earth-like planets and ocean planets by Sotin, C., Grasset, O., Mocquet, A.

    Published in Icarus (New York, N.Y. 1962) (01-11-2007)
    “…By comparison with the Earth-like planets and the large icy satellites of the Solar System, one can model the internal structure of extrasolar planets. The…”
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  2. 2

    Mapping modern CO2 fluxes and mantle carbon content all along the mid-ocean ridge system by Chavrit, D., Humler, E., Grasset, O.

    Published in Earth and planetary science letters (01-02-2014)
    “…Quality criteria have been used to select ∼400 vesicularity measurements on zero-age mid-ocean ridge glasses from ∼600 data available in the literature…”
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  3. 3

    Heat transport in the high-pressure ice mantle of large icy moons by Choblet, G., Tobie, G., Sotin, C., Kalousová, K., Grasset, O.

    Published in Icarus (New York, N.Y. 1962) (15-03-2017)
    “…•3D convection simulations tailored to specific structure of high-pressure ice mantle of large icy moons.•Melting is introduced, melt extraction is assumed…”
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  4. 4

    Water and Volatiles in the Outer Solar System by Grasset, O., Castillo-Rogez, J., Guillot, T., Fletcher, L. N., Tosi, F.

    Published in Space science reviews (01-10-2017)
    “…Space exploration and ground-based observations have provided outstanding evidence of the diversity and the complexity of the outer solar system. This work…”
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  5. 5

    Very high-density planets: a possible remnant of gas giants by Mocquet, A., Grasset, O., Sotin, C.

    “…Data extracted from the Extrasolar Planets Encyclo- paedia (see http://exoplanet.eu) show the existence of planets that are more massive than iron cores that…”
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    What makes a planet habitable? by Lammer, H., Bredehöft, J. H., Coustenis, A., Khodachenko, M. L., Kaltenegger, L., Grasset, O., Prieur, D., Raulin, F., Ehrenfreund, P., Yamauchi, M., Wahlund, J.-E., Grießmeier, J.-M., Stangl, G., Cockell, C. S., Kulikov, Yu. N., Grenfell, J. L., Rauer, H.

    Published in The Astronomy and astrophysics review (01-06-2009)
    “…This work reviews factors which are important for the evolution of habitable Earth-like planets such as the effects of the host star dependent radiation and…”
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  8. 8

    Titan's internal structure inferred from a coupled thermal-orbital model by Tobie, Gabriel, Grasset, Olivier, Lunine, Jonathan I., Mocquet, Antoine, Sotin, Christophe

    Published in Icarus (New York, N.Y. 1962) (01-06-2005)
    “…Through coupled thermal and orbital calculations including a full description of tidal dissipation, heat transfer and the H 2O NH 3 phase diagram, we propose a…”
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  9. 9

    A Study of the Accuracy of Mass-Radius Relationships for Silicate-Rich and Ice-Rich Planets up to 100 Earth Masses by Grasset, O, Schneider, J, Sotin, C

    Published in The Astrophysical journal (01-03-2009)
    “…A mass-radius (M-R) relationship is proposed for solid planets and solid cores ranging from 1 to 100 Earth-mass planets. It relies on the assumption that solid…”
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  10. 10

    Experimental investigation of methane hydrates dissociation up to 5 GPa: Implications for Titan's interior by Bezacier, L, Le Menn, E, Grasset, O, Bollengier, O, Oancea, A, Mezouar, M, Tobie, G

    “…Methane may be present in significant amounts in the interior of Titan and other icy moons, as well as in water-rich exoplanets, potentially stored in the form…”
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    Coupling of thermal evolution and despinning of early Iapetus by Robuchon, G., Choblet, G., Tobie, G., Čadek, O., Sotin, C., Grasset, O.

    Published in Icarus (New York, N.Y. 1962) (01-06-2010)
    “…The Cassini mission revealed two spectacular characteristics of Iapetus: (1) a geologically old and high equatorial ridge, which is unique in the Solar System…”
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    The ammonia–water system at high pressures: Implications for the methane of Titan by Grasset, O., Pargamin, J.

    Published in Planetary and space science (01-04-2005)
    “…The Cassini/Huygens mission will provide an accurate description of Titan's surface features. One important outcome of these data is that it will help for…”
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  14. 14

    On the internal structure and dynamics of Titan by Grasset, O., Sotin, C., Deschamps, F.

    Published in Planetary and space science (01-06-2000)
    “…The purpose of this paper is to study the evolution of Titan from the primordial core overturn to the present, and to investigate the possible existence of…”
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  15. 15

    Calibration of the R ruby fluorescence lines in the pressure range [0-1 GPa] and the temperature range [250-300 K] by Grasset, O.

    Published in High pressure research (01-11-2001)
    “…The pressure range [&1 GPa] and the temperature range [250-300 K] are commonly used in many science fields like biology, agro-chemistry, pharmacology, or…”
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    Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry? by Selsis, F., Chazelas, B., Bordé, P., Ollivier, M., Brachet, F., Decaudin, M., Bouchy, F., Ehrenreich, D., Grießmeier, J.-M., Lammer, H., Sotin, C., Grasset, O., Moutou, C., Barge, P., Deleuil, M., Mawet, D., Despois, D., Kasting, J.F., Léger, A.

    Published in Icarus (New York, N.Y. 1962) (15-11-2007)
    “…Planets less massive than about 10 M Earth are expected to have no massive H–He atmosphere and a cometary composition (∼50% rocks, 50% water, by mass) provided…”
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  17. 17

    Thermal convection in a volumetrically heated, infinite Prandtl number fluid with strongly temperature-dependent viscosity: Implications for planetary thermal evolution by Grasset, O., Parmentier, E. M.

    Published in Journal of Geophysical Research (10-08-1998)
    “…Parameterized models of the thermal evolution of planets are usually based on the assumption that the lithosphere‐convecting mantle boundary can be defined by…”
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    Review of exchange processes on Ganymede in view of its planetary protection categorization by Grasset, O, Bunce, E J, Coustenis, A, Dougherty, M K, Erd, C, Hussmann, H, Jaumann, R, Prieto-Ballesteros, O

    Published in Astrobiology (01-10-2013)
    “…In this paper, we provide a detailed review of Ganymede's characteristics that are germane to any consideration of its planetary protection requirements…”
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    The Cooling Rate of a Liquid Shell in Titan's Interior by Grasset, O., Sotin, C.

    Published in Icarus (New York, N.Y. 1962) (01-09-1996)
    “…Models describing the evolution of the primordial liquid layer in Titan's interior are presented using parameterized models. These models incorporate recent…”
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