An experimental study on kinetically-driven precipitation of calcium-magnesium-iron carbonates from solution: Implications for the low-temperature formation of carbonates in martian meteorite Allan Hills 84001

Citation
Dc. Golden et al., An experimental study on kinetically-driven precipitation of calcium-magnesium-iron carbonates from solution: Implications for the low-temperature formation of carbonates in martian meteorite Allan Hills 84001, METEORIT PL, 35(3), 2000, pp. 457-465
Citations number
34
Categorie Soggetti
Earth Sciences
Journal title
METEORITICS & PLANETARY SCIENCE
ISSN journal
10869379 → ACNP
Volume
35
Issue
3
Year of publication
2000
Pages
457 - 465
Database
ISI
SICI code
1086-9379(200005)35:3<457:AESOKP>2.0.ZU;2-N
Abstract
Spherical carbonate globules of similar composition, size, and radial Ca-, Mg-, and Fe-zonation to those in martian meteorite Allan Hills (ALH) 84001 were precipitated from Mg-rich, supersaturated solutions of Ca-Mg-Fe-CO2-H2 O at 150 OC. The supersaturated solutions (pH congruent to 6-7) were prepar ed at room temperature and contained in Teflon(TM)-lined stainless steel ve ssels, which were sealed and heated to 150 degrees C for 24 h. Experiments were also conducted at 25 degrees C and no globules comparable to those of ALH 84001 were precipitated. Instead, amorphous Fe-rich carbonates were for med after 24 h and Mg-Fe calcites formed after 96 h. These experiments sugg est a possible low-temperature inorganic origin for the carbonates in marti an meteorite ALH 84001.