Computer Science
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.249..153k&link_type=abstract
In ESA Proceedings of an ESA Workshop on the Comet Nucleus Sample Return Mission p 153-159 (SEE N87-25109 18-90)
Computer Science
1
Comet Nuclei, Cosmochemistry, Meteorites, Samples, Solar System, Volatility, Abundance, Chemical Composition, Solar Corona
Scientific paper
The study of volatile trace element concentrations in the solid parts of comet nuclei samples is discussed. Volatile elements are depleted even in primitive meteorites when compared to solar abundances. Since solar abundances are not too well known, cosmic abundances are usually derived from meteorites. In spite of the volatility of elements it seems more reliable to take these abundances from unprocessed cometary material. The behavior of volatile elements and their compounds is different in the outer part of the solar nebula. Homogeneous and heterogeneous accretion models predict different volatile elements compounds. In meteorites only products from homogeneous accretion are detected, but in the low temperature parts of the nebula the condensation behavior may have been different.
No associations
LandOfFree
Volatile elements in the early solar system and comet nucleus samples 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 Volatile elements in the early solar system and comet nucleus samples, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Volatile elements in the early solar system and comet nucleus samples will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1122086