Results 111 to 120 of about 1,415 (183)

Origin and Evolution of the Galilean Satellites Within the Jovian System. [PDF]

open access: yesSpace Sci Rev
Nimmo F   +10 more
europepmc   +1 more source

Rotation of the Solar system planets and the origin of the Moon in the context of the tidal downsizing hypothesis

open access: yes, 2011
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  

Nereid as a regular satellite of Neptune. [PDF]

open access: yesSci Adv
Belyakov M   +4 more
europepmc   +1 more source

Dawn-dusk Asymmetrical Distribution of Saturn's Cusp. [PDF]

open access: yesNat Commun
Xu Y   +12 more
europepmc   +1 more source

Extrasolar planets: Water on distant worlds

open access: yes, 2007
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  

HD 163296 and its giant planets: Creation of exo-comets, interstellar objects and transport of volatile material

open access: yes
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

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