Pa. Bland et al., Climate and rock weathering: A study of terrestrial age dated ordinary chondritic meteorites from hot desert regions, GEOCH COS A, 62(18), 1998, pp. 3169-3184
Ordinary chondrites (OC) recovered from the desert areas of Roosevelt Count
y, New Mexico, the Nullarbor Region of Western Australia, and the Algerian
and Libyan Sahara, for which C-14 terrestrial ages have been determined, we
re examined by Fe-57 Mossbauer spectroscopy. OC were chosen as a standard s
ample to investigate weathering processes as their well constrained trace a
nd bulk element chemistry, normative mineralogy and isotopic composition de
fine a known, pre-weathering, starting composition. Given that terrestrial
ages are known, it is possible to compare (initially very similar) samples
that have been subsequently weathered in a range of climatic regimes from t
he present day to > 44 ka BP. In addition, recently fallen equilibrated OC
contain iron only as Fe-0 and Fe2+, thus the abundance of ferric iron is di
rectly related to the level of terrestrial weathering.
Mossbauer spectroscopy identifies two broad types of ferric alteration: par
amagnetic phases (akaganeite, lepidocrocite, and goethite), and magneticall
y ordered (principally magnetite and maghemite). OC finds show a range in t
he percentage of total Fe existing as Fe3+ from zero to over 80%. However,
oxidation is comparable between fragments of the same OC separated since th
eir time of fall (i.e., paired meteorites).
Our results indicate several features of meteorite weathering that may resu
lt from climatic or geomorphologic conditions at the accumulation site: (1)
Saharan samples rue, overall, less weathered than non-Saharan samples, whi
ch may be related to the relatively recent age (ca. 20 ka) of the Saharan a
ccumulation surface; (2) broad differences between sites in the rate of wea
thering, arising from regional differences in climate; (3) consistent diffe
rences in the weathering products between samples that fell during humid pe
riods and those that fell during more arid periods (those falling during hu
mid periods contain a higher proportion of magnetically ordered ferric oxid
es); (4) one region (the Nullarbor) that shows a variation in the total amo
unt of ferric species that closely matches the climatic record for this are
a of Australia for the last 30 ka. Points (3) and (4) may be related to the
identification of a rapid initial weathering phase: the majority of weathe
ring occurs in the first few hundred years after fall, followed by passivat
ion of weathering by porosity reduction. Porosity reduction, and the associ
ated restriction in the ability of water to penetrate the sample, appears t
o be the mechanism whereby a weathering assemblage formed during the brief
initial period of oxidation is preserved through subsequent climatic cycles
over the terrestrial lifetime of the sample. Copyright (C) 1998 Elsevier S
cience Ltd.