Results 151 to 160 of about 259 (170)
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Formation of the regular satellites of giant planets in an extended gaseous nebula II: satellite migration and survival

Icarus, 2003
For a satellite to survive in the disk the time scale of satellite migration must be longer than the time scale for gas dissipation. For large satellites (∼1000 km) migration is dominated by the gas tidal torque. We consider the possibility that the redistribution of gas in the disk due to the tidal torque of a satellite with mass larger than the ...
Ignacio Mosqueira, Paul R. Estrada
openaire   +1 more source

Discussion of Some Real and/or Theoretical Effects of Captured Satellites on Both Terrestrial Planets and Gaseous Planets

2020
The purpose of this chapter is to demonstrate pathways to make Mars more habitable. Mars as it exists today is not habitable but it probably had habitable conditions for a brief era in the history of the planet. Prograde gravitational capture of a 0.1 moon-mass (~0.01 mars-mass) planetoid would cause high tidal amplitudes and ranges in both the ocean ...
openaire   +1 more source

Forming Planets via Pebble Accretion

Annual Review of Earth and Planetary Sciences, 2017
Anders Johansen, Michiel Lambrechts
exaly  

Eccentricity Evolution for Planets in Gaseous Disks

Astrophysical Journal, 2003
Re'em Sari, Peter Goldreich
exaly  

Evolutionary Analysis of Gaseous Sub-Neptune-Mass Planets With MESA

Astrophysical Journal, 2016
Leslie Rogers, Howard Chen
exaly  

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