Littérature scientifique sur le sujet « Giant gaseous planets »
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Articles de revues sur le sujet "Giant gaseous planets"
Veras, Dimitri, et Jim Fuller. « Tidal circularization of gaseous planets orbiting white dwarfs ». Monthly Notices of the Royal Astronomical Society 489, no 2 (26 août 2019) : 2941–53. http://dx.doi.org/10.1093/mnras/stz2339.
Texte intégralBoss, Alan P. « Metallicity and Planet Formation : Models ». Proceedings of the International Astronomical Union 5, S265 (août 2009) : 391–98. http://dx.doi.org/10.1017/s1743921310001067.
Texte intégralGuenel, M., S. Mathis et F. Remus. « Unravelling tidal dissipation in gaseous giant planets ». Astronomy & ; Astrophysics 566 (juin 2014) : L9. http://dx.doi.org/10.1051/0004-6361/201424010.
Texte intégralCarleo, Ilaria, Paolo Giacobbe, Gloria Guilluy, Patricio E. Cubillos, Aldo S. Bonomo, Alessandro Sozzetti, Matteo Brogi et al. « The GAPS Programme at TNG XXXIX. Multiple Molecular Species in the Atmosphere of the Warm Giant Planet WASP-80 b Unveiled at High Resolution with GIANO-B ∗ ». Astronomical Journal 164, no 3 (18 août 2022) : 101. http://dx.doi.org/10.3847/1538-3881/ac80bf.
Texte intégralRaymond, Sean N. « Terrestrial planet formation in extra-solar planetary systems ». Proceedings of the International Astronomical Union 3, S249 (octobre 2007) : 233–50. http://dx.doi.org/10.1017/s1743921308016645.
Texte intégralBoss, Alan P. « Modes of Gaseous Planet Formation ». Symposium - International Astronomical Union 202 (2004) : 141–48. http://dx.doi.org/10.1017/s0074180900217725.
Texte intégralMayor, M., D. Naef, F. Pepe, D. Queloz, N. C. Santos, S. Udry et M. Burnet. « HD 83443 : a system with two Saturns ». Symposium - International Astronomical Union 202 (2004) : 84–86. http://dx.doi.org/10.1017/s0074180900217543.
Texte intégralMasset, Frédéric S. « Planetary migration in gaseous protoplanetary disks ». Proceedings of the International Astronomical Union 3, S249 (octobre 2007) : 331–46. http://dx.doi.org/10.1017/s1743921308016797.
Texte intégralBitsch, Bertram, Andre Izidoro, Anders Johansen, Sean N. Raymond, Alessandro Morbidelli, Michiel Lambrechts et Seth A. Jacobson. « Formation of planetary systems by pebble accretion and migration : growth of gas giants ». Astronomy & ; Astrophysics 623 (mars 2019) : A88. http://dx.doi.org/10.1051/0004-6361/201834489.
Texte intégralHansen, Bradley M. S. « Formation of exoplanetary satellites by pull-down capture ». Science Advances 5, no 10 (octobre 2019) : eaaw8665. http://dx.doi.org/10.1126/sciadv.aaw8665.
Texte intégralThèses sur le sujet "Giant gaseous planets"
Debras, Florian. « Inner structure and atmospheric dynamics of gaseous giant planets ». Thesis, Lyon, 2018. http://www.theses.fr/2018LYSEN085/document.
Texte intégralThrough this thesis, I have been motivated by the will to improve our knowledge of giant planets, from our neigh- bouring Jupiter to the far away worlds across the galaxy: hot Jupiters.With the latest, extremely precise observations of the satellite Juno, new models of the interior of Jupiter can be derived. A precise enough method is required to take full advantage of these outstanding data, and I therefore studied the concentric Maclaurin spheroid method and its limitations.With contemporary understanding on the equations of state, diffusive properties and phase transition/separation of hydrogen and helium, I could then focus on producing new interior models of Jupiter. Combining the gravitational observations of Juno with the elemental observations of Galileo has proven to be a complicated task, which required to decompose the planet into at least four regions from the outer envelope to the inner, compact core. I have shown that the size of the compact core is degenerated with the entropy variation within the planet.Concerning hot Jupiters, I have reminded of the need to understand their atmospheric dynamics to constrain their interior structure, as the wind circulation can lead to an inflation of their radius. Studying numerically their at- mospheric dynamics was performed with the University of Exeter’s global circulation model as well as with the development of a linear solver that I called ECLIPS3D. An important, robust feature is the presence of a broad equatorial superrotation in the atmosphere of these planets.Finally, I have explored the spin up of this superrotation on theoretical grounds, to assess its physical relevance. I have calculated the linear time dependent solution to show the importance of differential drag and radiative damp- ing, and have used numerical simulations to highlight the importance of vertical momentum acceleration. Globally, a coherent picture of the initial spin up of superrotation was obtained.Through this work, I have improved my theoretical understanding of giant planets and developed various codes that can be used to study and improve our knowledge of the interior structure and atmospheric dynamics of giant planets, from Jupiter and Saturn to hot Jupiters
Lufkin, Graeme. « Simulations of giant planet migration in gaseous circumstellar disks / ». Thesis, Connect to this title online ; UW restricted, 2004. http://hdl.handle.net/1773/9698.
Texte intégralOrtiz, Mauricio, Sabine Reffert, Trifon Trifonov, Andreas Quirrenbach, David S. Mitchell, Grzegorz Nowak, Esther Buenzli et al. « Precise radial velocities of giant stars ». EDP SCIENCES S A, 2016. http://hdl.handle.net/10150/622444.
Texte intégralMoses, J. I., M. S. Marley, K. Zahnle, M. R. Line, J. J. Fortney, T. S. Barman, C. Visscher, N. K. Lewis et M. J. Wolff. « ON THE COMPOSITION OF YOUNG, DIRECTLY IMAGED GIANT PLANETS ». IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621961.
Texte intégralLavvas, P., et T. Koskinen. « Aerosol Properties of the Atmospheres of Extrasolar Giant Planets ». IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/626046.
Texte intégralDyrek, Achrène. « L'atmosphère des exoplanètes avec le James Webb Space Telescope ». Electronic Thesis or Diss., Université Paris Cité, 2023. http://www.theses.fr/2023UNIP7096.
Texte intégralMy thesis is devoted to the characterisation of exoplanet atmospheres with the newly-operating James Webb Space Telescope (JWST). Our understanding of exoplanet atmospheres is being revolutionised by the observational capabilities of such an observatory. The scientific outcomes will reach our scientific community and the general public, putting into perspective our knowledge of our own Solar System, the only system that is known to host life. The first part of this manuscript is devoted to an introduction that includes a state-of-the-art review of exoplanet atmospheres characterisation in terms of atomic and molecular composition, structure and dynamics. In this introduction, we focus on transiting exoplanets (when the planet passes in front of or behind its host star in the telescope's line of sight). We provide a description of this observational method and key results that have been obtained over the past two decades. The second part of this manuscript focuses on the molecular composition predictions with the JWST Mid-InfraRed Instrument (MIRI) and its Low-Resolution Spectrometer (LRS) that is meant to carry out atmospheric spectroscopy in an uncharted wavelength range. Here, we present realistic simulations of transiting exoplanets I developed during my thesis, with the MIRI LRS instrument that include various instrumental systematics likely to alter the atmospheric features we are meant to detect in our data [Dyrek+, sub., 2023, Morello, Dyrek+, 2022]. Our main objective is to design a comprehensive simulation tool that enables the community to build robust data reduction methods and to predict molecular detections. The third part of this manuscript is dedicated to the characterisation of the in-flight post-commissioning performances of the MIRI LRS. This work is based on the first exoplanetary transit observed with MIRI of the Super-Earth L168-9b, chosen to be a calibration target. My work focuses on identifying in-flight instrumental systematics that undermine observations' stability and more generally, the study of transiting exoplanets [Dyrek+, sub., 2023]. The final part of this manuscript is devoted to the scientific analysis of photometric and spectroscopic observations of both gas giants and temperate rocky exoplanet atmospheres. Here, I present my contribution on data reduction and analysis to the collaborative work we conducted as part of the Guaranteed Time Observation (GTO) and the Early Release Science (ERS) consortia. In particular, our work on the super-Neptune WASP-107b led to the first mid-infrared detection of sulphur dioxide (SO2) and silicate clouds [Dyrek+, sub., 2023b]. In addition, we conducted the first detection of the thermal emission of the rocky temperate exoplanet TRAPPIST-1b. In this work, we have constrained its brightness temperature, revealing key insights in the presence or not of an atmosphere [Greene+, 2023]. The final chapter of my thesis is dedicated to the prospects offered by JWST and the future Ariel mission, as these two telescopes will provide game-changing observations over the next decades
Livres sur le sujet "Giant gaseous planets"
Trieloff, Mario. Noble Gases. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.30.
Texte intégralBerner, Robert A. The Phanerozoic Carbon Cycle. Oxford University Press, 2004. http://dx.doi.org/10.1093/oso/9780195173338.001.0001.
Texte intégralChapitres de livres sur le sujet "Giant gaseous planets"
Chambers, John, et Jacqueline Mitton. « Worlds of Gas and Ice ». Dans From Dust to Life. Princeton University Press, 2017. http://dx.doi.org/10.23943/princeton/9780691175706.003.0012.
Texte intégralBeerling, David. « Oxygen and the lost world of giants ». Dans The Emerald Planet. Oxford University Press, 2007. http://dx.doi.org/10.1093/oso/9780192806024.003.0010.
Texte intégralBeerling, David. « Leaves, genes, and greenhouse gases ». Dans The Emerald Planet. Oxford University Press, 2007. http://dx.doi.org/10.1093/oso/9780192806024.003.0009.
Texte intégralYung, Yuk L., et William B. DeMore. « Chemical Kinetics ». Dans Photochemistry of Planetary Atmospheres. Oxford University Press, 1999. http://dx.doi.org/10.1093/oso/9780195105018.003.0006.
Texte intégralBoss, A. P. « 3D Solar Nebula Models : Implications For Earth Origin ». Dans Origin of the Earth, 3–15. Oxford University PressNew York, NY, 1990. http://dx.doi.org/10.1093/oso/9780195066197.003.0001.
Texte intégralSilva, Flávio C., Márcia Santos, Jéssica Moura, Ana C. Vilas Boas, Manuel A. Matos et Luís A. C. Tarelho. « Preventing wildfires through smart management and valorisation of residual forest biomass into biochar : experiences from the BioValChar project ». Dans Advances in Forest Fire Research 2022, 1507–12. Imprensa da Universidade de Coimbra, 2022. http://dx.doi.org/10.14195/978-989-26-2298-9_230.
Texte intégralActes de conférences sur le sujet "Giant gaseous planets"
Patel, C. K. N. « Spectroscopy of solid hydrogen using optoacoustic techniques ». Dans International Laser Science Conference. Washington, D.C. : Optica Publishing Group, 1986. http://dx.doi.org/10.1364/ils.1986.wh1.
Texte intégralRegnier, Pascal, Jeremy Llamas et Jonathan Grzymisch. « JUICE Attitude and Orbit Control System : major HW & ; SW challenges from design to development & ; validation ». Dans ESA 12th International Conference on Guidance Navigation and Control and 9th International Conference on Astrodynamics Tools and Techniques. ESA, 2023. http://dx.doi.org/10.5270/esa-gnc-icatt-2023-150.
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