2012
DOI: 10.2204/iodp.sd.13.04.2011
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IODP Expedition 335: Deep Sampling in ODP Hole 1256D

Abstract: Observations of the gabbroic layers of untectonized ocean crust are essential to test theoretical models of the accretion of new crust at mid-ocean ridges. Integrated Ocean Drilling Program (IODP) Expedition 335 ("Superfast Spreading Rate Crust 4") returned to Ocean Drilling Program (ODP) Hole 1256D with the intention of deepening this reference penetration of intact ocean crust a significant distance (~350 m) into cumulate gabbros. Three earlier cruises to Hole 1256D (ODP 206, IODP 309/312) have drilled throu… Show more

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Cited by 11 publications
(13 citation statements)
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“…The depth interval for each section is cited from Teagle et al [, ]. As bulk rocks from different sections have similar density [ Teagle et al , ], the total mass of each section is proportional to its depth interval that was used to calculate the concentration‐weighted average δ 65 Cu and δ 66 Zn values of bulk oceanic crust at IODP Site 1256.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The depth interval for each section is cited from Teagle et al [, ]. As bulk rocks from different sections have similar density [ Teagle et al , ], the total mass of each section is proportional to its depth interval that was used to calculate the concentration‐weighted average δ 65 Cu and δ 66 Zn values of bulk oceanic crust at IODP Site 1256.…”
Section: Discussionmentioning
confidence: 99%
“…The oceanic crust at this site formed ~15 Ma ago during an episode of superfast ocean ridge spreading (~220 mm/yr) [ Wilson et al , ]. The 1271.6 m of drilled crustal rocks were recovered at Site 1256 after penetrating ~250 m of sediments [ Wilson et al , ; Teagle et al , , ] (Figure ). As revealed by preliminary downhole stratigraphy established from shipboard core observations and wire line log interpretations onboard [ Wilson et al , , ; Teagle et al , ], the drilled oceanic crust, from top to bottom, consists of (1) the volcanic section (~250–1004.2 m below seafloor, bsf); (2) the lava‐dyke transition zone (1004.2–1060.9 m bsf); (3) the sheeted dyke complex (1060.9–1406.6 m bsf); and (4) the plutonic complex (1406.6–1521.3 m bsf).…”
Section: Geological Background and Sample Descriptionsmentioning
confidence: 99%
“…Pilot Hole 1256C cored 250.7 m of sediments and 88.5 m into the basement, that is composed of a 32 m thick lava pond with thin sheet flows above and below (Figure 2) [ Wilson et al , 2003]. The main hole with the deepest penetration, Hole 1256D, lays ∼30 m south of 1256C, started coring at 276 m below seafloor (mbsf) within the uppermost basement and penetrated 1271 m into the oceanic basement completely through the volcanic and dike sections and into the uppermost plutonic rocks (Figure 2) [ Wilson et al , 2006; Teagle et al , 2006, 2012].…”
Section: Geological Setting and Methodsmentioning
confidence: 99%
“…A characteristic feature of the granoblastic hornfelses at IODP Site 1256 is that they contain intrusions of felsic, evolved plutonic rocks. These are small, irregular patches, veins (~1-2 mm wide), and dikelets (<1.5 cm wide) consisting of oxide gabbro, diorite, tonalite, and trondhjemite (Wilson et al 2006;Teagle et al 2012) with a fine-to medium-grained granular texture. Here, for the comparison to experimental anatectic melts, we focus only on those felsic veins and dikelets of the Hole 1256D drill core characterized as tonalites based on the mineral mode.…”
Section: Felsic Rocks From Iodp Site 1256mentioning
confidence: 99%