Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body

Details Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2317t&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

We applied the Hf-W chronometer to three acapulcoites. Our new data
suggest that acapulcoites derive from a planetary body that accreted in
a narrow time interval between the accretion of the parent bodies of
differentiated asteroids and chondrites.

Affiliated with

Also associated with

No associations

Rating

Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body 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 Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hf-W Evidence for Rapid Accretion and Fast Cooling of the Acapulcoite Parent Body will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1823639