HR: 0800h
AN: T41D-1336 [Abstracts]
TI: Igneous petrology of Hole U1309D, IODP Expeditions 304/305 at the Atlantis Massif, MAR
30°N
AU: * Johnson, K T
EM: kjohnso2@hawaii.edu
AF: University of Hawaii, 1680 East-West Rd., Honolulu, HI 96822
United States
AB:
IODP Expeditions 304 and 305 at the Atlantis Massif (western rift flank of the Mid-Atlantic Ridge, 30°N) intended to
investigate the processes that control formation of oceanic core complexes as well as the exposure of ultramafic rocks in
very young oceanic lithosphere. The domal, corrugated surface of the 0.5-2 Myr old massif is interpreted as a detachment
fault exposed at the seafloor. The domal core forms the footwall to the detachment fault system, and was the main focus of
drilling at Hole U1309D (bottom: 1416 mbsf, recovery: 75%). Over 96% of Hole U1309D is made up of gabbroic lithologies,
which comprise amongst the most primitive as well as freshest plutonic rocks known from the ocean floor. Impregnated mantle
peridotites, now heavily serpentinized, constitute only 0.3% of recovered sequence and are restricted to four thin lenses in
the uppermost 200 m. Subhorizontal diabase sheets of variable thickness (0.01 - 10 m) with chilled margins mainly occur in
the uppermost 130 m of the hole (2.9%), but isolated thin dikes are also found at greater depths. Medium-grained to
pegmatitic gabbros and gabbronorites form the most abundant rock types (56%). Both grain size and modal composition can vary
strongly on a dm-scale, and commonly include minor quantities of olivine (rarely exceeding 10%), Fe-Ti-oxides, and/or
orthopyroxene. Intercalated with these gabbros are medium-grained olivine gabbros (28%), which have an olivine mode that
nearly always exceeds 20%. Their modes are highly variable on a submeter scale as well and they frequently grade into
troctolitic gabbro and troctolite. Olivine-rich troctolite with more than 70% olivine is very rare at mid-ocean ridges, but
comprises 5.4% of the recovered section. In contrast to troctolite, it has a cumulate-like texture with subhedral to rounded
olivine and interstitial to poikilitic plagioclase and clinopyroxene in variable proportions. Another special but more
common lithology is oxide gabbro (7.7% of the rocks recovered), defined by the occurrence of more than 2% modal Fe-Ti-oxide
minerals. The oxide-bearing gabbros are most common within the gabbro sequence, and the Fe-Ti-oxides occur as
heterogeneously distributed patches or seams. The oxide gabbros can occur as discrete dikelets crosscutting other
lithologies, or display strong enrichment in ductile deformation zones. These lithologies appear to repeat in two separate
and distinct intrusive packages of several hundred meters thickness each, with similar lithologic sequences comprising each.
Where visible, the contact relationships suggest that gabbro is generally intrusive into olivine-rich lithologies (olivine
gabbros and troctolites) and is itself intruded by zircon- and apatite-bearing felsic (``leucocratic'') dikes and oxide
gabbros. We note also that the upper ~60 m of gabbros in Hole 1309B, located 20 m away from 1309D and cored to only
101.8 mbsf, do not correlate with this interval in Hole 1309D, although later stage diabase units do correlate between Holes.
DE: 3035 Midocean ridge processes
DE: 3036 Ocean drilling
DE: 3614 Mid-oceanic ridge processes (1032, 8416)
DE: 3642 Intrusive structures and rocks
SC: Tectonophysics [T]
MN: Fall Meeting 2005