Meteoritic diagenesis is a transformation that occurs at or near the Earth’s surface in strata influenced or penetrated by water of recent atmospheric origin. The meteoritic environment is generally divided into unsaturated (vadose) and saturated (phreatic) zones separated by a water table (see top diagram, opposite page). The interfaces between surficial meteoritic fluids and layers filled with other pore fluids (seawater or groundwater) are “mixing zones” that may have special diagenetic properties. Many, perhaps most, near-surface marine carbonate deposits undergo meteoritic diagenesis, either as a result of the buildup of sediments above sea level or as a result of a drop in sea level that exposes platform carbonates. In addition, meteoric water can circulate far below the land surface and alter carbonate deposits that are far older than the exposure interval. Meteoric processes typically occur over periods of hundreds to millions of years.