Planets and satellites
Theoretical and experimental studies of electromagnetic resonances in the ionospheric cavities of planets and satellites; instrument and mission perspectives
... circuit and associated energy sources, and to the identification of the inner and outer cavity ...developed and applied to all planets and satellites surrounded by an ...
301
Science goals for future exploration of the habitability of the gaseous giant planets' satellites
... giant planets, space missions, JUICE) 1. Introduction The satellites of Jupiter and Saturn have been revealed as extremely astrobiologically interesting bodies presenting promising conditions for ...
4
Giant Planets
... few satellites stand out by having relatively large masses: it is the case of Jupiter’s Io, Europa, Ganymede and Callisto, of Saturn’s Titan, and of Neptune’s ...moons and satellites ...
47
Water and the Interior Structure of Terrestrial Planets and Icy Bodies
... 0.335 and 0.342. For Ganymede and Callisto, the two coefficients have not been determined independently, and the -10/3 relationship has been prescribed when inverting the degree-two gravity ...
46
An educated search for transiting habitable planets: (Research Note) Targetting M dwarfs with known transiting planets
... habitable planets transiting nearby M dwarfs. Its main principle is simple: planets form within disks, therefore a planet orbiting in the HZ of a given star should have a higher a priori tran- sit ...
5
197 Candidates and 104 Validated Planets in K2' First Five Fields
... inter- and intra-pixel sensitivity variations and aperture losses, results in significant changes in our aperture ...frame and an arbitrary reference frame using roughly 100 stars of Kp∼12 mag on an ...
66
Planets and Stellar Activity: Hide and Seek in the CoRoT-7 system
... 2 and in- jected a synthetic sinusoid with the orbital parameters of planet d reported by Tuomi et ...plerian and a constant ...ibility, and allow other parts of the model to fit the data if they are ...
17
The HARPS search for southern extra-solar planets. III. Three Saturn-mass planets around HD 93083, HD 101930 and HD 102117
... Observations and measurement precision HD 93083, HD 101930 and HD 102117 are all members of the HARPS high-precision RV ...) and exhibiting low ac- tivity levels (log R HK < ...variations ...
7
The rotation of extra-solar planets
... point, and a tidal bulge will result, with an important quadrupolar component, perpendicular to the direction of the Sun ...δ, and an accelerating torque will appear ...
11
Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1
... loss and the time the planet spends in the HZ: planets around low mass BDs lose little hydrogen but they stay a short time in the HZ, planets around the higher mass UCDs considered here spend a ...
14
WASP-86b and WASP-102b: super-dense versus bloated planets
... Palma and In- stituto de Astrofísica de ...Palma and WASPSouth is hosted by ...support and assistance. Funding for WASP comes from consortium universities and from the UK’s Science and ...
15
Store and Forward routing in satellite constellationslations de satellites
... Tous ces services peuvent ˆetre combin´es pour en composer d’autres plus performants. On peut prendre l’exemple d’un service de t´el´e-surveillance d’une flotte de v´ehicules de transport qui transmet l’´etat de ...
155
12-Mouvements des planètes et des satellites
... 2) Les satellites géostationnaires (9) : Comme leur nom l’indique, ces satellites sont fixes (stationnaire) par rapport à la terre (géo). Pour que ce soit le cas, il faut que Ils décrivent un mouvement ...
6
Théorie dynamique des satellites galiléens
... 1.3 E quations du probleme des N -corps non ponctuels dans un repere planetocentrique d'axes xes A travers cette section, nous allons commencer par presenter les termes a introduire pour[r] ...
185
Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets
... and chemistry of the weather layer, both in terms of small-scale convective events (storms, plumes and vortices, like the discrete activity in ...3 and planetary-scale ...equator and ...
39
La radiodiffusion directe par satellites et le cas du Québec
... Cette etude cherche a situer le phenomene de la radiodiffusion directe par satellites dans son conte;x;te per- tinent en ce qui concerne le Quebec. A partir de l[r] ...
309
Populations of Extrasolar Giant Planets from Transit and Radial Velocity Surveys
... Multiplicity of EGP Spectroscopic surveys of hot Jupiters revealed that about half of them have long- period (at several AU) massive companions, within the planetary or stellar regime (e.g. Knutson et al. 2014; ...
23
Magnetic coupling of planets and small bodies with a pulsar wind"
... the planets are pro- tected from a direct contact with the wind by a bow ...quency and large amplitude electromagnetic wave to be emit- ted, the wave character of which reveals itself in the wave zone, ...
11
The Spitzer search for the transits of HARPS low-mass planets. II. Null results for 19 planets
... detect, and its amplitude is much larger than the one of the searched ...nature and we could not find any analytical function of external parameters (PSF peak value, center position and width, ...
23
en fr Study of the organisation and the transcriptional activity of mouse major satellites L’étude de l’organisation et l’activité transcriptionnelle des satellites majeurs de la souris
... nt) and B2 RNA (178 nt), that was found to be involved in the regulation of the RNA pol II transcription during stress (Allen et ...transcription and together with the heat shock protein 1 form nuclear ...
192