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Source of the Quaternary alkalic basalts, picrites and basanites of the Potrillo volcanic field, New Mexico, USA; lithosphere or convecting mantle?

Thompson, R N; Ottley, C J; Smith, P M; Pearson, D G; Dickin, A P (2005) Source of the Quaternary alkalic basalts, picrites and basanites of the Potrillo volcanic field, New Mexico, USA; lithosphere or convecting mantle?. Journal of Petrology, vol.46, no.8, pp.1603-1643, Aug 2005

AuthorsThompson, R N; Ottley, C J; Smith, P M; Pearson, D G; Dickin, A P
Year2005
TitleSource of the Quaternary alkalic basalts, picrites and basanites of the Potrillo volcanic field, New Mexico, USA; lithosphere or convecting mantle?
SourceJournal of Petrology, vol.46, no.8, pp.1603-1643, Aug 2005
ISSN0022-3530
GeoRef2006-083239
Keywordsalkali basalts; basalts; basanite; Cenozoic; chemical properties; chemical ratios; convection; Dona Ana County New Mexico; geochemistry; igneous rocks; Las Cruces New Mexico; lithogeochemistry; lithosphere; mantle; New Mexico; picrite; Potrillo volcanic field; Quaternary; United States; volcanic fields; volcanic rocks
DOI10.1093/petrology/egi028

Abstract

The <80 ka basalts-basanites of the Potrillo Volcanic Field (PVF) form scattered scoria cones, lava flows and maars adjacent to the New Mexico-Mexico border. MgO ranges up to 12.5%; lavas with MgO<10.7% have fractionated both olivine and clinopyroxene. Cumulate fragments are common in the lavas, as are subhedral megacrysts of aluminous clinopyroxene (with pleonaste inclusions) and kaersutitic amphibole. REE modelling indicates that these megacrysts could be in equilibrium with the PVF melts at approximately 1.6-1.7 GPa pressure. The lavas fall into two geochemical groups: the Main Series (85% of lavas) have major- and trace-element abundances and ratios closely resembling those of worldwide ocean-island alkali basalts and basanites (OIB); the Low-K Series (15%) differ principally by having relatively low K (sub 2) O and Rb contents. Otherwise, they are chemically indistinguishable from the Main Series lavas. Sr- and Nd-isotopic ratios in the two series are identical and vary by scarcely more than analytical error, averaging (super 87) Sr/ (super 86) Sr = 0.70308 (SD = 0.00004) and (super 143) Nd/ (super 144) Nd = 0.512952 (SD = 0.000025). Such compositions would be expected if both series originated from the same mantle source, with Low-K melts generated when amphibole remained in the residuum. Three PVF lavas have very low Os contents (<14 ppt) and appear to have become contaminated by crustal Os. One Main Series picrite has 209 ppt Os and has a gamma (sub Os) value of +13.6, typical for OIB. This contrasts with published (super 187) Os/ (super 188) Os ratios for Kilbourne Hole peridotite mantle xenoliths, which give mostly negative gamma (sub Os) values and show that Proterozoic lithospheric mantle forms a thick Mechanical Boundary Layer (MBL) that extends to approximately 70 km depth beneath the PVF area. The calculated mean primary magma, in equilibrium with Fo (sub 89) , has Na (sub 2) O and FeO contents that give a lherzolite decompression melting trajectory from 2.8 GPa (95 km depth) to 2.2 GPa (70 km depth). Inverse modelling of REE abundances in Main Series Mg-rich lavas is successful for a model invoking decompression melting of convecting sub-lithospheric lherzolite mantle (epsilon Nd = 6.4; T (sub p) approximately 1400 degrees C) between 90 and 70 km. Nevertheless, such a one-stage model cannot account for the genesis of the Low-K Series because amphibole would not be stable within convecting mantle at T (sub f) approximately 1400 degrees C. These magmas can only be accommodated by a three-stage model that envisages a Thermal Boundary Layer (TBL) freezing conductively onto the approximately 70 km base of the Proterozoic MBL during the approximately 20 Myr tectonomagmatic quiescence before PVF eruptions. As it grew, this was veined by hydrous small-fraction melts from below.

59 samples from this reference

SampleRock nameMajorTraceIsotope
671Basalt yesyes
672Basalt yesyes
674Basalt yesyes
675Basalt yesyes
676Basalt yesyes
678Basalt yesyes
695Basalt yesyes
699Basalt yesyes
860Basalt yesyes
864Basalt yesyes
865Basalt yesyes
866Basalt yesyes
869Basalt yesyesyes
870Basalt yesyesyes
875Basalt yesyes
879Basalt yesyes
882Basalt yesyes
883Basalt yesyes
888Basalt yesyes
894Basalt yesyes
895Basalt yesyes
898Basalt yesyes
6100Basalt yesyes
6102Basalt yesyes
6103Basalt yesyes
6104Basalt yesyes
6108Basalt yesyes
6110Basalt yesyesyes
6127Basalt yesyes
6130Basalt yesyes
6140Basalt yesyes
6143Basalt yesyes
6151Basalt yesyes
6152Basalt yesyes
6155Basalt yesyes
6157Basalt yesyes
6158Basalt yesyes
6185Basalt yesyes
6187Basalt yesyes
8101Basalt yesyes
8103Basalt yesyes
8107Basalt yesyes
8109Basalt yesyes
8110Basalt yesyes
8111Basalt yesyesyes
8112Basalt yesyesyes
8128Basalt yesyes
8129Basalt yesyesyes
8134Basalt yesyes
8136Basalt yesyes
8138Basalt yesyes
8139Basalt yesyes
8140Basalt yesyes
8144Basalt yesyesyes
8157Basalt yesyes
8159Basalt yesyesyes
8160Basalt yesyes
8161Basalt yesyes
8164Basalt yesyesyes