Results 211 to 220 of about 11,561 (252)
The initial solar system abundance of 60Fe and early core formation of the first asteroids. [PDF]
Sci AdvFang L +5 more
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Low-energy glycine formation and spectral masking in star-forming regions. [PDF]
Commun ChemMates-Torres E, Rimola A.
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Models and observational predictions of dust traps in protoplanetary discs. [PDF]
Astrophys Space SciPinilla P.
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Theoretical study on planetesimal formation through gravitational instability
, 2007 Shugo Michikoshi
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2017
Processes governing the evolution of planetesimals are critical to understanding how rocky planets are formed, how water is delivered to them, the origin of planetary atmospheres, how cores and magnetic dynamos develop, and ultimately, which planets have the potential to be habitable.
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Processes governing the evolution of planetesimals are critical to understanding how rocky planets are formed, how water is delivered to them, the origin of planetary atmospheres, how cores and magnetic dynamos develop, and ultimately, which planets have the potential to be habitable.
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Radial Migration of Planetesimals
Astrophysics and Space Science, 1994Planetesimals orbiting a protostar in a circumstellar disk are affected by gravitational interaction among themselves and by gas drag force due to disk gas. Within the Kyoto model of planetesimal accretion, the migration rate is interpreted as the inverse of the planetary formation time scale. Here, we study time scales of gravitational interaction and
Neuhäuser, R., Feitzinger, J.
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