TEMPORAL AND SPATIAL VARIATIONS IN CRUSTAL ACCRETION ALONG THE MID-ATLANTIC RIDGE (29-DEGREES-31-DEGREES-30'-N) OVER THE LAST 10 MY - IMPLICATIONS FROM A 3-DIMENSIONAL GRAVITY STUDY
Je. Pariso et al., TEMPORAL AND SPATIAL VARIATIONS IN CRUSTAL ACCRETION ALONG THE MID-ATLANTIC RIDGE (29-DEGREES-31-DEGREES-30'-N) OVER THE LAST 10 MY - IMPLICATIONS FROM A 3-DIMENSIONAL GRAVITY STUDY, J GEO R-SOL, 100(B9), 1995, pp. 17781-17794
We have conducted a three-dimensional gravity study of the Mid-Atlanti
c Ridge near the Atlantis Transform to study the evolution of accretio
nary processes at this slow-spreading center over the last 10 m.y. We
have removed from the free-air gravity anomaly the gravity contributio
n of the density contrast at the seafloor and the gravity contribution
of the lateral density variations associated with the cooling of the
lithosphere. The resulting residual gravity anomaly exhibits substanti
al variation along and across the ridge axis. The residual gravity ano
maly can be accounted for by variations in crustal thickness of up to
3 km. For the first two segments south of the Atlantis Transform, the
midportions of the segments have been associated with thick crust and
the segment discontinuities have been associated with thin crust for t
he last 10 m.y., suggesting the segment discontinuities act as long-te
rm boundaries in the delivery of melt to the individual segments. In c
ontrast, our calculations indicate that for the segments north of the
fracture zone, thick crust is associated with the midportions of segme
nts and thin crust is associated with segment discontinuities only in
crust less than similar to 3 m.y. This result suggests that focused ma
ntle upwelling has only recently developed north of the fracture zone.
The onset of focused mantle upwelling at approximately 2-3 m.y. may b
e related to a change in the spreading direction which occurred betwee
n magnetic anomalies 5 and 3 (Figure 1) and resulted in changes in the
geometry of the plate boundary north of the fracture zone. Cross sect
ions of crustal thickness extracted along the midpoint traces of paleo
segments show that, for a few segments, up to 2 km of gradual crustal
thinning is observed. We suggest that the ''apparent'' crustal thinnin
g is a result of lateral changes in mantle density associated with buo
yant upwelling not predicted by the passive flow model used in our stu
dy. Variations in computed crustal thickness are observed across axis
in all of the paleosegments in our study area, but are not correlated
between individual segments. If these computed crustal thickness varia
tions are due to temporal variations in melt production, this implies
that there is little interdependence in the amount of melt supplied to
adjacent segments.