Primitive material surviving in chondrites - matrix
Description
A logical place to search for surviving pristine nebular material is in the fine-grained matrices of ordinary and carbonaceous chondrites of petrographic type 3. Unfortunately, many of these chondrites have experienced brecciation, thermal metamorphism, and aqueous alteration, so that interpreting individual features in terms of specific nebular conditions and/or processes is difficult. It follows that the origin and evolutionary history of such matrix phases are controversial, and a consensus is difficult to define. In this chapter, therefore, after summarizing the salient mineralogical, petrographic, chemical, and isotopic features of matrix in apparently primitive chondrites, an attempt is made to provide an overview both of areas of agreement and of topics that are currently in dispute. 82 references
Additional details
Publishing Information
- Publisher
- University of Arizona Press.
- Imprint Place
- Tucson, AZ (USA)
- Imprint Title
- Meteorites and the early solar system
- Journal Page Range
- p. 718-745.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20054375
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; CHONDRITES; METAMORPHISM; MINERALOGY; MINERALS; OLIVINE; ORIGIN; OXYGEN ISOTOPES; PETROLOGY; SILICATES; SOLAR NEBULA; SOLAR SYSTEM; SOLAR SYSTEM EVOLUTION
- Descriptors DEC
- METEORITES; NEBULAE; OXYGEN COMPOUNDS; SILICATE MINERALS; SILICON COMPOUNDS; STONE METEORITES