Other
Scientific paper
Jul 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999m%26ps...34..541w&link_type=abstract
Meteoritics & Planetary Science, vol. 34, no. 4, pp. 541-557 (1999).
Other
38
Scientific paper
Several classes of chondritic meteorites experienced heterogeneous aqueous alteration and subsequent brecciation before agglomeration into the final parent bodies. These processes resulted in intimate mixing of materials altered to various degrees. In the past, this mixing has been attributed solely to impact processes. However, our investigation of the physical consequences of aqueous alteration processes in bodies accreting from a mixture of silicate and ice grains shows that aqueous alteration was commonly accompanied by substantial gas production. The asteroids may have become so internally pressurized by these gases that the sudden onset of gas release led to partial or complete disaggregation of the body. In some cases, fragments may have escaped completely from the parent asteroid and could potentially have been incorporated into other accreting asteroids. In other cases, fragments originating from different parts of the initial body, having various sizes and temperatures and exhibiting varying degrees of alteration, may have re-accreted into a second generation object and undergone further stages of alteration. Such events could have been repeated two or three times during the lifetime of 26Al, the likely heat source for these processes.
Bourcier William
Browning Lauren B.
Keil Klaus
Krot Alexander N.
Wilson Leslie
No associations
LandOfFree
Early aqueous alteration, explosive disruption, and re-processing of asteroids does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Early aqueous alteration, explosive disruption, and re-processing of asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Early aqueous alteration, explosive disruption, and re-processing of asteroids will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-996113