Results 301 to 310 of about 171,913 (339)

A diamond-bearing core-mantle boundary on Mercury. [PDF]

open access: yesNat Commun
Xu Y   +5 more
europepmc   +1 more source

A hot-Jupiter progenitor on a super-eccentric retrograde orbit. [PDF]

open access: yesNature
Gupta AF   +59 more
europepmc   +1 more source

An Abrupt Change in the Disk Fraction of Free-Floating Planets at the Deuterium-Burning Ignition Limit

open access: yes
Rodrigues T   +11 more
europepmc   +1 more source

Planet Formation

2012
Astrobiology is an exciting interdisciplinary field that seeks to answer one of the most important and profound questions: are we alone? In this volume, leading international experts explore the frontiers of astrobiology, investigating the latest research questions that will fascinate a wide interdisciplinary audience at all levels.
Raymond, Sean N., Benz, W.
openaire   +4 more sources

The formation of the planets

Icarus, 1968
Abstract The possibility of formating a planetary system, starting from a diffuse rotating cloud of gas and dust, as a result of accretion by a proto-Sun is investigated. It is found that a ring of relatively high density is formed in the equatorial plane of the proto-Sun gas cloud system.
B. W. Pendred, Iwan P. Williams
openaire   +2 more sources

Formation and Evolution of Planets

Astrophysics and Space Science, 1994
The basic stages of the formation of the planets are considered. Decay of turbulence in the solar nebula allows the precipitation of dust particles to the solar nebula’s equatorial plane, their growth occurring by sticking at collisions and transformation into kilometer-sized bodies (planetesimals) partly by direct growth and partly via gravitational ...
V. S. Safronov, E. L. Ruskol
openaire   +2 more sources

Formation of the planets

Vistas in Astronomy, 1980
Abstract There are discussed briefly the following topics concerning the formation of the planets: 1.Formation of the protoplanetary nebula from a rotating interstellar magnetic cloud 2.The mass and temperature distribution in the protoplanetary nebula 3.The formation of planets by colliding planetesimals and by gas accretion 4.The distances, spin ...
openaire   +2 more sources

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