Bp. West et al., EVIDENCE FOR VARIABLE UPPER-MANTLE TEMPERATURE AND CRUSTAL THICKNESS IN AND NEAR THE AUSTRALIAN ANTARCTIC DISCORDANCE, Earth and planetary science letters, 128(3-4), 1994, pp. 135-153
The Southeast Indian Ridge (SEIR) in and near the Australian-Antarctic
Discordance (AAD) exhibits, at a constant spreading rate, almost the
full range of the many geophysical and geochemical parameters characte
ristic of the 'slow' Mid-Atlantic Ridge and 'fast' East Pacific Rise.
We used satellite-derived gravity data, in combination with SeaMARC II
bathymetry in and near the AAD, to examine regional density variation
s in the upper mantle beneath the AAD. Through three-dimensional gravi
ty analysis, we found that at least two end-member models satisfy the
gravity observations: regional crustal thickness variations of at leas
t 3 km along the SEIR near the AAD or a temperature anomaly of the ord
er of 150 degrees C in the upper mantle beneath the SEIR. These new ob
servations, combined with other geophysical and geochemical characteri
stics of the Australian-Antarctic Discordance, provide further evidenc
e that the temperature structure of a mid-ocean ridge is a controlling
factor, in addition to spreading rate, in the crustal accretionary pr
ocess. Numerical models of mantle flow beneath mid-ocean ridges offer
one means of investigating the dynamic effect of a variable upper mant
le temperature on the accretionary process. Our results indicate that
temperature is important, especially at intermediate and slower spread
ing rates, where thermal effects can dominate mantle flow beneath a mi
d-ocean ridge and result in increasing crustal production with decreas
ing spreading rate. At the constant, intermediate spreading rate of 37
mm/yr, characteristic of the SEIR in and near the AAD, our numerical
models show that significant crustal thinning (2-4 km) can occur with
relatively small variations in upper mantle temperature, all else bein
g equal. Thus, combined with our end-member gravity models, these obse
rvations and results suggest that both anomalously cool upper mantle a
nd thin crust exist beneath the AAD.