Morlock, A.; Sutton, Y. C.; Braithwaite, N. St.J. and Grady, M. M.
|Google Scholar:||Look up in Google Scholar|
The exact process of chondrule formation is still not known - common scenarios are formation in a protoplanetary nebular environment: e.g. X-wind model or nebular shock fronts, where precursor grains are heated by collisions with gas.
Most chondrules appear to have been heated to 1500–1600 ºC, followed by a rapid cooling of usually between 10 to 1000 ºC/h.
In this part of our study about the formation of chondrules by shock processes, we try to simulate the formation of chondrules by gas-grain collisions in a nebular environment.
|Item Type:||Conference Item|
|Copyright Holders:||2011 The Authors|
|Academic Unit/Department:||Science > Physical Sciences
Mathematics, Computing and Technology > Engineering & Innovation
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
|Depositing User:||Patricia Taylor|
|Date Deposited:||17 May 2012 14:37|
|Last Modified:||05 Mar 2014 10:44|
Actions (login may be required)
|Report issue / request change|