Primary Accretion by Turbulent Concentration: The Rate of Planetesimal Formation and the Role of Vortex Tubes

Details Primary Accretion by Turbulent Concentration: The Rate of Planetesimal Formation and the Role of Vortex Tubes Primary Accretion by Turbulent Concentration: The Rate of Planetesimal Formation and the Role of Vortex Tubes

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2536c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2536

Physics

Scientific paper

We present a new fundamental timescale for direct formation of
10-100-km-diameter asteroids and TNOs by concentration of small
particles in turbulence, and show how vortex tubes acting on large
scales may explain the properties of numerical simulations.

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