Numerical Simulation of I-type Spherule Formation

Details Numerical Simulation of I-type Spherule Formation Numerical Simulation of I-type Spherule Formation

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1463y&link_type=abstract

Lunar and Planetary Science, volume 27, page 1463

Physics

2

Atmospheric Entry, Numerical Simulation, Oxidation, Processes: Formation, Spherules: Cosmic

Scientific paper

Numerical simulations for atmospheric entry of spherules are performed to calculate the time dependence of velocity, altitude, spherules' radii and temperature. They indicate that the strong apparent gravitational acceleration due to atmospheric drag results in exposure of metallic cores to the air during melting and oxidation of spherules. Two major types of internal structures of Fe-Ni spherules are explained by this model.

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