Precondensed matter - Key to the early solar system

Physics – Condensed Matter

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

55

Chemical Fractionation, Condensation, Meteoritic Composition, Protostars, Solar System, Stellar Evolution, Abundance, Interstellar Matter, Nebulae, Radioactive Isotopes, Stellar Mass Ejection, Supernovae

Scientific paper

Explicit astrophysical details are developed for the hypothesis that chemical and isotopic anomalies in primitive solar-system samples reflect routine initial chemical conditions within precondensed matter. The central feature of this theory concerns the chemical state of presolar dust, which is regarded as never having been vaporized in the region where the most chemically primitive samples (carbonaceous meteorites) accumulated. It is suggested that the initial chemical state of heavy atoms during meteorite and planetary accumulation was distributed between a refractory-mineral component from high-temperature condensation and a volatile component resulting from cold matter adhering to preexisting grains. Thermal conditions in the solar nebula are considered along with the existence of supernova condensates and other thermal condensates in the interstellar dust. Fractionation into volatile and refractory elements is idealized in terms of four distinct interstellar components, and the fractionated precondensed matter is described.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Precondensed matter - Key to the early solar system 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 Precondensed matter - Key to the early solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precondensed matter - Key to the early solar system will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1692081

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.