Published 1988 | Version v1
Book

Highly labile elements

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.