A critical analysis of shock models for chondrule formation
β Scribed by Stammler, Sebastian M.; Dullemond, Cornelis P.
- Book ID
- 125861208
- Publisher
- Elsevier Science
- Year
- 2014
- Tongue
- English
- Weight
- 938 KB
- Volume
- 242
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Chondrule formation due to the shock heating of dust particles with a wide variety of shock properties are examined. We numerically simulate the steady postshock region in a framework of one-dimensional hydrodynamics, taking into account many of the physical and chemical processes that determine the
We present numerical simulations of the thermal and dynamical histories of solid particles (chondrules and their precursorstreated as 1-mm silicate spheres) during passage of an adiabatic shock wave through a particle-gas suspension in a minimum-mass solar nebula. The steady-state equations of energ
We present numerical simulations of the interaction of a onedimensional radiative gas dynamic shock wave with a dust cloud in the solar nebula that is finite in dimension parallel to the direction of shock propagation. Energy and momentum transfer to the shock-heated gas as the gas penetrates the du
A shock-wave heating model is one of the possible models for chondrule formation. We examine, within the framework of a shock-wave heating model, the effects of evaporation on the heating of chondrule precursor particles and the stability of their molten state in the postshock flow. We numerically s