Oxygen-isotopic composition and high-resolution secondary ion mass spectrometry imaging of Martian carbonate in Lafayette meteorite
Creators
Abstract
Carbonate from SNC meteorites gives insight into a variety of processes on and/or beneath the surface of Mars. In Lafayette, carbonate occurs in unusually intimate association with hydrous phases when compared with other carbonate-bearing SNCs [1]. We have measured the ^(18)O/^(16)O ratio of carbonate in the alteration veins of Lafayette using the magnetic sector ion microprobe. In addition, we obtained isotope images of major- and minor-element cations in veinlets with the focused ion beam (FIB) quadrupole SIMS. The spot size of the FIB probe used in this study (~0.03 µm) provides an opportunity for high spatial resolution chemical imaging, which is ideal for examining features in the fine-grained alteration assemblage.
Additional Information
© 1998 The Meteoritical Society. Article first published online: 4 Feb. 2010.Attached Files
Published - Eiler_1998pA159.pdf
Files
Eiler_1998pA159.pdf
Additional details
Identifiers
- Eprint ID
- 39265
- DOI
- 10.1111/j.1945-5100.1998.tb01327.x
- Resolver ID
- CaltechAUTHORS:20130709-095420187
Dates
- Created
-
2013-07-10Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)