I. Valeton et al., SUPERGENE ALTERATION SINCE THE UPPER CRETACEOUS ON ALKALINE IGNEOUS AND METASOMATIC ROCKS OF THE POCOS DE CALDAS RING COMPLEX, MINAS-GERAIS, BRAZIL, Applied geochemistry, 12(2), 1997, pp. 133-154
This contribution presents field evidence, mineralogical observations
and geochemical data of different modes of lateritic weathering which
affected the alkaline magmatic rocks and their metasomatic alteration
products since the Upper Cretaceous. Field relations demonstrate that
ferralitic (bauxitic) weathering is confined to well-drained hill cres
t and upper slope settings. In the Popes de Caldas area bauxite normal
ly rests directly on parent rock. Stagnant drainage and reducing condi
tions beneath tropical peat deposits, along valley floors and in lower
slope situations favour sialitic (saprolitic) weathering. The additio
nal importance of high porosity and permeability is demonstrated by co
-occurring parent rocks with strongly contrasting response on weatheri
ng attack. In normal nepheline syenites and phonolites nepheline break
s down first and nearly instantly upon weathering. This results in hig
h porosity, giving water and atmospheric gases easy access to the more
resistant minerals. Thus in well-drained morphological positions baux
ite is generated. if the same original magmatic parent rocks are ''shi
elded'' against pervasive weathering attack by pre-lateritic metasomat
ic alteration, no comparable early permeability arises. A fine-grained
and dense metasomatic assemblage of kaolinite, illite, microcline and
smectite, combined with the annealing of fractures and joints, is abl
e to prevent bauxite generation, and saprolite is formed instead. This
metasomatically induced saprolite is significantly richer in illite t
han ''normal'' saprolite. Bauxite formation results in a strong deplet
ion of Mg, Ca, Na, K, Si, Ni, Co, Cu, Zn, Rb, Ba, Sr, Y and REE. Siali
tic (saprolitic) weathering leads to a generally less pronounced deple
tion of essentially the same elements. Silicon and Ni are more efficie
ntly retained than in bauxite. Mobile elements are Mn, Ca, Na, K, Mg,
Co, Zn, Rb, Ba, Sr and REE. Cerium can be re-precipitated under oxidiz
ing local conditions. Closely associated positive and negative Ce-anom
alies are due to inhomogenously concentrated precipitates in small-sca
le spatial alternation with zones of nearly total depletion. A general
correlation between the type of laterite (saprolite or bauxite) and C
e-retainment or depletion does not exist. Host phases for most of the
immobile trace elements are goethite and related plasmas in bauxites a
nd saprolites. Immobility is exhibited by V, Pb, Ga, Nb, Zr, Th and U.
Relict zircon is too rare to explain a seemingly retarded HREE-loss i
n saprolites. (C) 1997 Elsevier Science Ltd.