Clinopyroxenes (cpx) separated from discrete spinel lherzolite xenoliths from Kilbourne Hole, New Mexico, are compositionally and isotopically heterogeneous. On a Nd-Sr isotope correlation diagram, the cpx plot largely within the mantle array, from near Bulk Earth to depleted MORB values. None of the bulk xenoliths are equivalent to primitive mantle; all have undergone one or more depletion events and some have been enriched in incompatible elements. The lherzolites as well as the cpx show significant variations in incompatible element ratios including Sm/ Nd and Sr/Nd; moreover, 147Sm 144Nd and 143Nd 144Nd ratios of the cpx are positively correlated and suggestive of an 0.4 Ga fractionation event. Cpx from spinel pyroxenite dikes and lherzolite wallrocks of composite xenoliths are relatively homogeneous (isotopically) and similar to OIB and some MORB. The wallrocks are isotopically equilibrated with the pyroxenites or nearly so, and have negative Nd model ages; we infer that the pyroxenite-forming event caused enrichment in incompatible elements in the contiguous wallrock. The pyroxenite parent magma was probably a primitive basanite characterized by low Hf/Sm and Ti/Sm ratios relative to primitive mantle as a consequence of residual garnet. Our data confirm the presence of a MORB-related component in the mantle beneath Kilbourne Hole. This component is fertile with respect to basaltic constituents, is relatively LREE-depleted, and is isotopically similar to MORB; it is probably derived from asthenosphere. The isotopic heterogeneity of the discrete lherzolites requires a second, enriched component characterized by relatively low 143Nd 144Nd and high 87Sr 86Sr ratios and unsupported 143Nd 144Nd ratios. Old but disparate Sr and Nd model ages require that MORB-related spinel lherzolites have had a complicated history and differentiated from primitive mantle more than 1 b.y. ago. Two plausible models, one involving more than one depletion event and the second involving mixing of mantle components depleted at distinct times, can explain the common observation that Sr model ages are older than Nd model ages.