INTRODUCTION Geologic Setting The Palos Verdes Peninsula (Figs. 1 and 2) is dominated by the Palos Verdes Hills, the topographic expression of a doubly plunging anticlinorium that is currently active (Ward and Valensise, 1994). Uplift and anticlinal growth of the peninsula have been linked in part with activity of the northwest-trending, southwest-dipping Palos Verdes fault (Fig. 1; Woodring et al., 1946; Yerkes et al., 1965; Ward and Valensise, 1994). However, a study by Clarke et al. (1998) in the inner Los Angeles Harbor suggests that only about 20%-30% of this uplift during late Pleistocene and Holocene time (Ponti and Lajoie, 1992) can be attributed directly to the vertical component of Palos Verdes fault displacement. This finding implies that another, as yet unlocated, fault (or faults) is a major contributor to the balance of late Quaternary uplift determined for the Palos Verdes Hills. The Palos Verdes fault is divisible into southern, central, and northern segments (Fig. 1; Ward and Valensise, 1994). The northern segment underlies Santa Monica Bay. The central segment, about 20 km long, is located onshore adjacent to the Palos Verdes Hills. The southern segment extends offshore beneath San Pedro Bay, and this segment may bifurcate below the shelf edge into two fault strands that trend southeastward to Lasuen