This paper has briefly reviewed the results of Leg 173 with allusions to results of Leg 149, where appropriate and for completeness, that also relate to the development of the west Iberia continental margin before the onset of seafloor spreading. Further details can be found in the references that accompany the text. Other references refer to geophysical observations off west Iberia and to comparable work done in the rifted margin and transition zone fragments now exposed in the Alps. In spite of the importance of considering both members of a conjugate pair of margins when discussing their development, this has not been done here because of the lack of comparable ODP or other borehole data from beyond the shelf edge off the Newfoundland margin. Aspects of the postrift history, which was not a specific objective of Leg 173 drilling, are also omitted and are discussed elsewhere (Kuhnt and Urquhart, in press; Whitmarsh, Sawyer, Klaus, and Masson, 1996) and in this volume (Roessig and Wise, Chap. 4; Urquhart, Chap. 9; Wallrabe-Adams, Chap. 6; Zhao et al., Chap. 8).
One as-yet unresolved
problem on the west Iberia margin is the apparently almost complete lack of
synrift melt products in the ODP cores, although a synrift (122.1 ± 0.3 Ma)
chlorite schist derived from a Fe-Ti-rich gabbro protolith has been sampled
northwest of Galicia Bank (Schärer et al., 1995). It has also been suggested,
from analysis of mostly deep-towed magnetometer profiles, that scattered
gabbroic bodies may exist within the serpentinized peridotite basement of the
OCT (Russell, 1999; Whitmarsh et al., in press). The lack of melt is a problem
for melting models (Bown and White, 1995), given the relatively short minimum
periods of continental lithosphere extension suggested by Wilson et al. (in
press a) (5 m.y.) and Dean et al. (2000) (7 m.y.); for
= 10 stretching of a 125-km lithosphere overlying a 1300°-1350°C
potential temperature asthenosphere, Bown and White's model predicts 3-6 km of
melt. Harry and Bowling (1999) and Bowling and Harry (in press) presented a
finite element model of nonvolcanic rifted margins that predicts that melting
begins only after lithospheric necking has become focused and results in a short
period of magmatism confined to the end of the rift episode just before
continental breakup. Unfortunately, the problem off west Iberia is a lack of
evidence for significant melt, not only in the thinned continental crust prior
to breakup but also in the broad OCT, for some time immediately after breakup.
Minshull et al. (in press) considered and rejected the effects of lateral heat
conduction, anomalously low mantle potential temperature, and depth-dependent
stretching to explain totally the lack of melt products at the time of
continental breakup and subsequently in the OCT. Instead, they proposed
qualitative arguments that, even for OCT extension lasting only 10 m.y., melting
was inhibited while asthenospheric upwelling remained relatively unfocused as
the thermal structure of the lithosphere evolved from that of a rifting margin
to that of a steady-state spreading ridge. In this context, it is salutary to
recognize that radiometric dates from Site 1067 suggest that exhumation, and
therefore extension, at the seaward edge of thinned continental crust lasted at
least 24 m.y. (Table T2),
far longer than suggested by Wilson et al. (in press a).
It is clear that the
combined efforts of scientific drilling and geophysical observations off west
Iberia, and particularly in the southern Iberia Abyssal Plain, have provided a
valuable set of data with which to investigate the development of this
nonvolcanic rifted margin. Even so, several problems remain. The significance
and continental or oceanic origin of the peridotite ridge remains obscure. The
OCT is 15
km wide off Galicia Bank and is up to 170 km wide in the southern Iberia Abyssal
Plain, but there is insufficient evidence at present to estimate its width in
the Tagus Abyssal Plain with confidence. How and why does the width of the OCT
vary along the margin? Does the so-far unsampled deep OCT (Region C in Fig. F3)
really consist of serpentinized peridotite, as inferred from indirect evidence?
A deep drill hole in this region would test this inference and also provide a
very valuable and potentially complete postrift sedimentary record (and
subsidence history), which is currently lacking. Lastly, scientific drilling on
the deep conjugate Newfoundland margin has the potential to make a very
significant contribution to our understanding of the development and eventual
lithospheric reconstruction of the west Iberia-Newfoundland conjugate pair of
margins.