Jk. Tripathi et V. Rajamani, Geochemistry of the loessic sediments on Delhi ridge, eastern Thar desert,Rajasthan: implications for exogenic processes, CHEM GEOL, 155(3-4), 1999, pp. 265-278
Quartzite ridges in the Delhi region include in their local depressions thi
ck piles of unconsolidated, unstratified, yellowish brown, homogenous loamy
sediments. These Delhi ridge sediments (DRS) have textural, mineralogical
and geochemical characteristics similar to those of loess sediments. Geoche
mically, DRS, just as other loess sediments, are similar to average exposed
upper continental crust of Taylor and McLennan [Taylor, S.R., McLennan, S.
M., 1985. The Continental Crust: Its Composition and Evolution. Blackwell,
London, 311 pp.]. The calculated chemical index of alteration [Nesbitt, H.W
., Young, G.M., 1984. Prediction of some weathering trends of plutonic and
volcanic rocks based on thermodynamic and kinetic considerations. Geochim.
Cosmochim. Acta 54, 1523-1534; Nesbitt, H.W., Young, G. M., 1989. Formation
and diagenesis of weathering profiles. J. Geol. 97, 129-147.] and other ch
emical parameters suggest a provenance of chemically less weathered rocks.
During the process of wind transport and deposition, not only the dilution
effect of silica on the REE abundance was counterbalanced but also the REE
pattern was kept similar to the UCC and PAAS by the appropriate concentrati
on and mixing of the REE bearing phases. The immediate source to these sedi
ments is likely to be mechanically ground sediments of glacial origin. The
last phase of the upliftment of the Himalayas, accompanied by Pleistocene g
laciation could have provided a vast glacio-fluvial outwash plain. The aeol
ian processes associated with prevailing W to SW winds in the hot arid cond
ition seem to have been selectively transporting fertile silt materials lea
ving behind infertile desert sands. (C) 1999 Elsevier Science B.V. All righ
ts reserved.