Zobrazeno 1 - 10
of 273
pro vyhledávání: '"Grasset O"'
Autor:
Doran, P.T., Hayes, A., Grasset, O., Coustenis, A., Prieto-Ballesteros, O., Hedman, N., Al Shehhi, O., Ammannito, E., Fujimoto, M., Groen, F., Moores, J.E., Mustin, C., Olsson-Francis, K., Peng, J., Praveenkumar, K., Rettberg, P., Sinibaldi, S., Ilyin, V., Raulin, F., Suzuki, Y., Xu, K., Whyte, L.G., Zaitsev, M., Buffo, J., Kminek, G., Schmidt, B.
Publikováno v:
In Life Sciences in Space Research May 2024 41:86-99
Autor:
GRASSET O.
Publikováno v:
Knowledge and Management of Aquatic Ecosystems, Vol 0, Iss 186, Pp 22-25 (1957)
Externí odkaz:
https://doaj.org/article/fa3a0d2e87704f2a8a865a45adb7a83d
Autor:
Stephan, K., Roatsch, T., Tosi, F., Matz, K.-D., Kersten, E., Wagner, R., Molyneux, P., Palumbo, P., Poulet, F., Hussmann, H., Barabash, S., Bruzzone, L., Dougherty, M., Gladstone, R., Gurvits, L.I., Hartogh, P., Iess, L., Wahlund, J.-E., Wurz, P., Witasse, O., Grasset, O., Altobelli, N., Carter, J., Cavalié, T., d'Aversa, E., Della Corte, V., Filacchione, G., Galli, A., Galluzzi, V., Gwinner, K., Hauber, E., Jaumann, R., Krohn, K., Langevin, Y., Lucchetti, A., Migliorini, A., Piccioni, G., Solomonidou, A., Stark, A., Tobie, G., Tubiana, C., Vallat, C., Van Hoolst, T.
Publikováno v:
In Planetary and Space Science 15 November 2021 208
Autor:
Tinetti, G., Beaulieu, J. P., Henning, T., Meyer, M., Micela, G., Ribas, I., Stam, D., Swain, M., Krause, O., Ollivier, M., Pace, E., Swinyard, B., Aylward, A., van Boekel, R., Coradini, A., Encrenaz, T., Snellen, I., Zapatero-Osorio, M. R., Bouwman, J., Cho, J. Y-K., Foresto, V. Coudé du, Guillot, T., Lopez-Morales, M., Mueller-Wodarg, I., Palle, E., Selsis, F., Sozzetti, A., Ade, P. A. R., Achilleos, N., Adriani, A., Agnor, C. B., Afonso, C., Prieto, C. Allende, Bakos, G., Barber, R. J., Barlow, M., Bernath, P., Bezard, B., Bordé, P., Brown, L. R., Cassan, A., Cavarroc, C., Ciaravella, A., Cockell, C. O. U., Coustenis, A., Danielski, C., Decin, L., De Kok, R., Demangeon, O., Deroo, P., Doel, P., Drossart, P., Fletcher, L. N., Focardi, M., Forget, F., Fossey, S., Fouqué, P., Frith, J., Galand, M., Gaulme, P., Hernández, J. I. González, Grasset, O., Grassi, D., Grenfell, J. L., Griffin, M. J., Griffith, C. A., Grözinger, U., Guedel, M., Guio, P., Hainaut, O., Hargreaves, R., Hauschildt, P. H., Heng, K., Heyrovsky, D., Hueso, R., Irwin, P., Kaltenegger, L., Kervella, P., Kipping, D., Koskinen, T. T., Kovács, G., La Barbera, A., Lammer, H., Lellouch, E., Leto, G., Morales, M. Lopez, Valverde, M. A. Lopez, Lopez-Puertas, M., Lovis, C., Maggio, A., Maillard, J. P., Prado, J. Maldonado, Marquette, J. B., Martin-Torres, F. J., Maxted, P., Miller, S., Molinari, S., Montes, D., Moro-Martin, A., Moses, J. I., Mousis, O., Tuong, N. Nguyen, Nelson, R., Orton, G. S., Pantin, E., Pascale, E., Pezzuto, S., Pinfield, D., Poretti, E., Prinja, R., Prisinzano, L., Rees, J. M., Reiners, A., Samuel, B., Sanchez-Lavega, A., Forcada, J. Sanz, Sasselov, D., Savini, G., Sicardy, B., Smith, A., Stixrude, L., Strazzulla, G., Tennyson, J., Tessenyi, M., Vasisht, G., Vinatier, S., Viti, S., Waldmann, I., White, G. J., Widemann, T., Wordsworth, R., Yelle, R., Yung, Y., Yurchenko, S. N.
A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the presence of life
Externí odkaz:
http://arxiv.org/abs/1112.2728
Autor:
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.
The search for rocky exoplanets plays an important role in our quest for extra-terrestrial life. Here, we discuss the extreme physical properties possible for the first characterized rocky super-Earth, CoRoT-7b (R_pl = 1.58 \pm 0.10 R_Earth, Mpl = 6.
Externí odkaz:
http://arxiv.org/abs/1102.1629
Autor:
Leger, A., Rouan, D., Schneider, J., Barge, P., Fridlund, M., Samuel, B., Ollivier, M., Guenther, E., Deleuil, M., Deeg, H. J., Auvergne, M., Alonso, R., Aigrain, S., Alapini, A., Almenara, J. M., Baglin, A., Barbieri, M., Bruntt, H., Borde, P., Bouchy, F., Cabrera, J., Catala, C., Carone, L., Carpano, S., Csizmadia, Sz., Dvorak, R., Erikson, A., Ferraz-Mello, S., Foing, B., Fressin, F., Gandolfi, D., Gillon, M., Gondoin, Ph., Grasset, O., Guillot, T., Hatzes, A., Hebrard, G., Jorda, L., Lammer, H., Llebaria, A., Loeillet, B., Mayor, M., Mazeh, T., Moutou, C., Paetzold, M., Pont, F., Queloz, D., Rauer, H, Renner, S., Samadi, R., Shporer, A., Sotin, Ch., Tingley, B., Wuchterl, G.
We report the discovery of very shallow (DF/F = 3.4 10-4), periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which we interpret as due to the presence of a transiting companion. We describe the 3-colour
Externí odkaz:
http://arxiv.org/abs/0908.0241
Publikováno v:
Astrophys.J.693:722-733,2009
A mass-radius relationship is proposed for solid planets and solid cores ranging from 1 to 100 Earth-mass planets. It relies on the assumption that solid spheres are composed of iron and silicates, around which a variable amount of water is added. Th
Externí odkaz:
http://arxiv.org/abs/0902.1640
Autor:
Schneider, J., Boccaletti, A., Aylward, A., Baudoz, P., Beuzit, J. -L., Brown, R., Cho, J., Dohlen, K., Ferrari, M., Galicher, R., Grasset, O., Grenfell, L., Griessmeier, J. -M., Guyon, O., Hough, J., Kasper, M., Keller, Ch., Longmore, A., Lopez, B., Martin, E., Mawet, D., Menard, F., Merin, B., Palle, E., Perrin, G., Pinfield, D., Sein, E., Shore, P., Sotin, Ch., Sozzetti, A., Stam, D., Surdej, J., Tamburini, F., Tinetti, G., Udry, S., Verinaud, C., Walker, D.
The physical characterization of exoplanets will require to take spectra at several orbital positions. For that purpose, a direct imaging capability is necessary. Direct imaging requires an efficient stellar suppression mechanism, associated with an
Externí odkaz:
http://arxiv.org/abs/0811.2496
Autor:
Selsis, F., Chazelas, B., Borde, 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., Leger, A.
Planets less massive than about 10 MEarth are expected to have no massive H-He atmosphere and a cometary composition (50% rocks, 50% water, by mass) provided they formed beyond the snowline of protoplanetary disks. Due to inward migration, such plane
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701608
Publikováno v:
In Icarus 15 March 2017 285:252-262