Results 111 to 120 of about 1,415 (183)
The hidden mysteries of our ice giant planets. [PDF]
de Villa K, Ge H.
europepmc +1 more source
Origin and Evolution of the Galilean Satellites Within the Jovian System. [PDF]
Nimmo F +10 more
europepmc +1 more source
It has been proposed recently that the first step in the formation of both rocky and gas giant planets is dust sedimentation into a solid core inside a gas clump (giant planet embryo). The clumps are then assumed to migrate closer to the star where their
figshare admin leicester (5539453)
core
Dawn-dusk Asymmetrical Distribution of Saturn's Cusp. [PDF]
Xu Y +12 more
europepmc +1 more source
Asteroid sample return missions are critical for understanding our Solar System. [PDF]
Bates H.
europepmc +1 more source
Extrasolar planets: Water on distant worlds
Is the presence of water a feature common to all gas-giant planets? The first convincing detection of water vapour in the atmosphere of such a planet from outside our Solar System indicates that the answer is ...
Knutson, Heather A.
core
Context. The birth of giant planets in protoplanetary discs is known to alter the structure and evolution of the disc environment, however most of our knowledge is focussed on its effects on the observable gas and dust. The impact on the evolution of the
J. M. Trigo-Rodriguez +46 more
core +1 more source
Characterization of exoplanets in the James Webb Space Telescope era. [PDF]
Lunine JI, Bahcall N.
europepmc +1 more source
Phosphorus-nitrogen systematics of first-generation planetesimals constrain life-essential element delivery to Earth. [PDF]
Pathak D, Dasgupta R, Iyer N.
europepmc +1 more source

