Published 1988
| Version v1
Book
Highly labile elements
Creators
Description
Certain elements of high lability are very responsive to thermal processes, being either highly volatile during primary nebular condensation or highly mobile by postaccretionary metamorphic or shock heating. Data for highly labile elements indicate that different thermal processes were important in the genesis of each of the chondritic groups and a discussion of each is given. Contents of highly labile elements in a given group of contemporary falls differ from those of the same group that fell in Antarctica more than 0.1 Myr ago. This difference is due either to a time-dependent change in meteorite sources or, less likely, orbital variation of the meteorite flux to Earth. 46 references
Additional details
Additional titles
- Augmented title (English)
- In meteorites
Publishing Information
- Publisher
- University of Arizona Press.
- Imprint Place
- Tucson, AZ (USA)
- Imprint Title
- Meteorites and the early solar system
- Journal Page Range
- p. 462-487.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20054370
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACTIVATION ENERGY; CHEMICAL COMPOSITION; CHONDRITES; ELEMENTS; HEATING; MAGNESIUM SILICATES; NEBULAE; RARE GASES; SOLAR SYSTEM; STABILITY; TRACE AMOUNTS
- Descriptors DEC
- ALKALINE EARTH METAL COMPOUNDS; ENERGY; MAGNESIUM COMPOUNDS; METEORITES; NONMETALS; OXYGEN COMPOUNDS; SILICATES; SILICON COMPOUNDS; STONE METEORITES