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Turbulence, Chondrules, and PlanetesimalsIt has been shown both numerically and experimentally that 3-D turbulence concentrates aerodynamically size-selected particles by orders of magnitude. In a previous review chapter, in "Chondrules and the protoplanetary disk" we illustrated the initial predictions of Turbulent Concentration (TC) as applied to the solar nebula. We predicted the particle size which will be most effectively concentrated by turbulence; it is the particle which has a gas drag stopping time equal to the overturn time of the smallest (Kolmogorov scale) eddy. The primary uncertainty is the level of nebula turbulence, or Reynolds number Re, which can be expressed in terms of the standard nebula eddy viscosity parameter alpha = Re(nu)(sub m)/cH, where nu(sub m) is molecular viscosity, c is sound speed, and H is vertical scale height. Several studies, and observed lifetimes of circumstellar disks, have suggested that the level of nebula turbulence can be described by alpha = 10(exp -2) - 10(exp -4). There is some recent concern about how energy is provided to maintain this turbulence, but the issue remains open. We adopt a canonical minimum mass nebula with a range of alpha > 0. We originally showed that chondrule-sized particles are selected for concentration in the terrestrial planet region if alpha = 10(exp -3) - 10(exp -4). In addition, Paque and Cuzzi found that the size distribution of chondrules is an excellent match for theoretical predictions. One then asks by what concentration factor C these particles can be concentrated; our early numerical results indicated an increase of C with alpha, and were supported by simple scaling arguments, but the extrapolation range was quite large and the predictions (C ~ 10(exp 5) - 10(exp 6) not unlikely) uncertain. The work presented here, which makes use of our recent demonstration that the particle density field is a multifractal with flow-independent properties provides a far more secure ground for such predictions. We also indicate how fine-grained dust rims on chondrules might enter into constraining the situation.
Document ID
20070001976
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Cuzzi, Jeffrey
(NASA Ames Research Center Moffett Field, CA, United States)
Hogan, Robert C.
(NASA Ames Research Center Moffett Field, CA, United States)
Dobrovolskis, Anthony R.
(NASA Ames Research Center Moffett Field, CA, United States)
Paque, Julie M.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 1998
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Protostars and Planets IV Conference
Location: Santa Barbara, CA
Country: United States
Start Date: July 6, 1998
End Date: July 10, 1998
Funding Number(s)
PROJECT: RTOP 344-37-22-03
Distribution Limits
Public
Copyright
Other

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