PRELIMINARY INVESTIGATION OF THE OCCURRENCE OF MARBLE GRUS AND CORESTONES IN THE SAN BERNADINO MOUNTAINS, CALIFORNIA
Marble corestones are also common and range in diameter from 0.2 to 1 m as a function of joint spacing. Joint surfaces between corestones commonly exhibit rinds of reprecipitated calcite that, in some cases, clearly penetrates between grain boundaries. Root traces preserved along these rinds indicate that they formed prior to exhumation of the corestone. This secondary calcite surface acts as a local capstone that prevents granular disintegration of the underlying friable marble. In the absence of these rinds, however, marble outcrops erode rapidly by physical weathering, as evidenced by the lack of dissolution features. Such dissolution features are common on late Holocene-aged alluvial fan surfaces (Eppes, 2002). Preliminary soil pits show accumulation of decimeters to meters of unweathered, well-sorted grusy calcite crystals on hillslopes. Soil development is minimal with only incipient pedogenic carbonate precipitation on larger clasts and very weak structure development. Many explanations (e.g. alteration of plagioclase, biotite expansion) proposed to explain this style of physical weathering in granitic igneous rocks fail to explain similar weathering in carbonate. Further study of rock micromorphology, sediment production and marble grus soils of the region should provide insights into the characteristics and rates of processes acting on this landscape.