Other
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993natur.364...25o&link_type=abstract
Nature (ISSN 0028-0836), vol. 364, no. 6432, p. 25-33.
Other
138
Carbon Stars, Graphite, Interstellar Matter, Meteoritic Composition, Nuclear Fusion, Silicon Carbides, Diamonds, Granular Materials, Solar Corona, Solar System, Meteorites, Grains, Composition, Silicon Carbide, Graphite, Oxides, Diamond, Isotopes, Nucleosynthesis, Condensation, Solar Nebula, Xenon, Rare Gases, Physical Properties, Anomalies, Abundance, Carriers, Neon, Solar System, Origin, Formation, Source, Interstellar Dust, S Process, Size, Distribution, Composition, Laboratory Studies, Carbon, Procedure
Scientific paper
Primitive meteorites contain grains of silicon carbide, graphite and diamond formed outside the Solar System and probably before its birth. The isotopic compositions of these grains provide a record of stellar nucleosynthesis and of condensation processes near carbon stars; the fact of their survival places constraints on conditions in the solar nebula and early Solar System. The search is now on for other surviving stellar condensates, such as nitrides and oxides.
No associations
LandOfFree
Interstellar grains in meteorites 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 Interstellar grains in meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar grains in meteorites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1073485