Published 1988
| Version v1
Report
Noble gases, C,N, and Si isotopes in interstellar SiC form the Murchison carbonaceous chondrite
Description
Isotopic measurements of presolar interstellar silicon carbide are presented. Silicon carbide was recently identified in a primitive meteorite Murray. There exists strong evidence that the silicon carbide predates the formation of the solar system and originated in the atmospheres of certain stars. Thus, this material provides a link with its stellar sources and gives the opportunity to study processes taking place in distant stars
Additional details
Publishing Information
- Imprint Title
- Nineteenth lunar and planetary science conference. Press abstracts
- Journal Page Range
- p. 25-27.
- Report number
- N--88-30473
Conference
- Title
- 19. lunar and planetary science conference.
- Dates
- 14-18 Mar 1988.
- Place
- Houston, TX (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20043342
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- CARBON ISOTOPES; CHEMICAL COMPOSITION; CHONDRITES; EXPERIMENTAL DATA; GEOLOGIC HISTORY; INTERSTELLAR GRAINS; ISOTOPE RATIO; NITROGEN ISOTOPES; ORIGIN; RARE GASES; SILICON CARBIDES; SILICON ISOTOPES; SOLAR SYSTEM
- Descriptors DEC
- CARBIDES; CARBON COMPOUNDS; DATA; ELEMENTS; INFORMATION; METEORITES; NONMETALS; NUMERICAL DATA; PARTICLES; SILICON COMPOUNDS; STONE METEORITES