Basaltic lavas were erupted from a 40-km-long lineament near the Hobbs
Coast of Marie Byrd Land, Antarctica, over the period from 11.7 m.y.
to 2.3 m.y. ago. The lavas from the southernmost locality, Coleman Nun
atak, are virtually constant in major, trace element and isotopic comp
osition over this entire age span. Their high FeO-low Al2O3 character
indicates melting of garnet peridotite at about 140 km depth. There is
no evidence for the involvement of ancient continental Lithosphere or
MORE asthenosphere in the magmatism. Isotopically, the lavas show the
highest Pb-206/Pb-204 ratios (up to 20.7) of any of the Cenozoic volc
anism associated with the West Antarctic rift system (WARS). This HIMU
isotopic signature is also clear in the trace element patterns, which
closely mimic end-member HIMU basalts from the oceanic islands of Tub
uai and Mangaia. From the other localities along the Hobbs Lineament,
the earliest volcanism, which is coeval with that at Coleman Nunatak,
is of shallower derivation (similar to 110 km), and isotopically like
the oceanic FOZO end-member (Pb-206/Pb-204 similar to 19.5). The trace
-element patterns are similar to those at Coleman, but less enriched i
n the most incompatible elements by a factor of two. Modeling of the t
race element data is consistent with a uniform mantle source compositi
on, depleted in major elements, but hydrous and mildly enriched in the
incompatible and LREE. Inversion for the bulk distribution coefficien
ts of the source mantle reveals a spidergram with a marked negative Ti
anomaly and marked positive anomalies for K, Sr, Zr and Hf. From this
modeling, the extent of melting at Coleman is inferred to be similar
to 1.6%, as compared to similar to 3.2% during the earliest volcanism
elsewhere on the lineament. With time, the volcanism from these other
localities progresses to greater depth, becomes more HIMU in character
, and lower in extent of melting (i.e., approaches the character of ba
salts from the Coleman locality). The FOZO component is prevalent as a
mixing end-member in WARS volcanism from numerous other Marie Byrd La
nd (MEL) and Northern Victoria Land (NVL) localities. It is also the m
ain constituent of the three nearby oceanic plumes (Balleny, Scott, Pe
ter I islands). The HIMU component is at best a minor constituent of t
hese oceanic plumes, but is present at several other MBL and NVL local
ities, as well as in pieces of Zealandia which were adjacent to this c
oast of Antarctica prior to fragmentation of Gondwana. We propose that
this HIMU mantle source was emplaced under Gondwana lithosphere prior
to breakup, as a large weak plume head, with Little or no accompanyin
g volcanism. This 'fossil-plume' proto-lithosphere is now being sample
d during WARS extension. Likely mechanisms for the volcanism relate ei
ther to small-scale convection associated with strong basal topography
of the lithosphere (such as that recorded by the Hobbs Lineament volc
anism), or to emplacement of a new plume, which may in part be driving
the extension. (C) 1997 Elsevier Science B.V.