PRECARIOUS ROCKS AND SEISMIC RISK IN THE LAS VEGAS REGION James N. Brune and John G. Anderson Seismological Laboratory University of Nevada, Reno ABSTRACT In some types of terrain, groups of precariously balanced rocks evolve naturally unless shaken down by earthquakes. The time scale for the evolution and stability of these rocks is on the order of thousands of years. Therefore groups of precariously balanced rocks are effectively earthquake strong ground motion seismoscopes. Zones of precarious rocks are direct evidence that no strong ground accelerations have occurred in the zone for thousands of years. They thus have the potential to provide important information about seismic risk. Precarious rocks have been found at more than a dozen sites in Nevada. Although we have not been able to do any accurate age dating on these rocks, we can make rough estimates of their age based on geomorphic conditions. Most of the spectacular precarious rocks near Las Vegas are of the hoodoo type, i.e., a hard protective boulder on top of a less weather-resistant pillar. Because the pillars may erode relatively rapidly we cannot establish as long existence times as we can for more resistant rocks. A rough estimate is that these hoodoos have been in existence for at least a thousand years. They have been documented at Nelson Landing and in Kyle Canyon. Precarious rocks in more resistant formations near Beatty and Yucca mountain have probably been in existence for more than ten thousand years. Indirect positive evidence of strong ground shaking may be provided by the lack of precarious rocks in the Red Rock area. The formations there appear to be of the type that should create numerous precarious rocks, yet none have been found. This suggests that there has been relatively strong ground motion in the Red Rock area in the last ten thousand years. We plan to present updated evidence from precarious rocks in the Las Vegas area. We will use the evidence to provide constraints on the probability of strong ground motion for the area.