Rl. Hay et al., MAGNESIUM-RICH CLAYS OF THE MEERSCHAUM MINES IN THE AMBOSELI BASIN, TANZANIA AND KENYA, Clays and clay minerals, 43(4), 1995, pp. 455-466
The Sinya Beds of the Amboseli Basin in Tanzania and Kenya consist lar
gely of carbonate rocks and Mg-rich clays that are intensely deformed
where exposed in and near former meerschaum mines. The carbonate rocks
consist of limestone and dolomite in Tanzania, but only dolomite has
been identified in Kenya. Sepiolite and mixed-layered kerolite/stevens
ite (Ke/St) are subordinate constituents of the carbonate rocks. The c
arbonate rocks and overlying bedded sepiolite were deposited in a semi
arid lake basin at the foot of the large volcano Kilimanjaro. Calcite
and dolomite of the carbonate rocks have delta(18)O values 4-6 parts p
er thousand lower than calcite and dolomite of the late Pleistocene Am
boseli Clays, suggesting that the Sinya Beds were deposited in the mid
dle or early Pleistocene under a different climatic regime when meteor
ic water had lower delta(18)O values than at present. Mg-rich clay min
erals form veins and fill cavities in the Sinya Beds. The principal cl
ay minerals are sepiolite and Ke/St, some of which contains substantia
l Al and Fe (Al-Ke/St). NEWMOD(R) modeling and other X-ray diffraction
(XRD) data suggest that most of the Ke/St contains 25-50 percent kero
lite layers, but minor amounts of kerolite-rich Ke/St are present in s
ome samples. Illite with an inferred high content of Fe or Mg is a min
or constituent of the samples with Al-Ke/St. The cavity-filling clays
were chemically precipitated, as shown by field relationships and SEM
study. The early-deposited clays of veins and cavities are principally
Ke/St with minor sepiolite, and the latest clay is sepiolite (meersch
aum), generally with minor Ke/St. The delta(18)O values of cavity-fill
ing Ke/St range from 22.5-25.6 parts per thousand and correlate with m
ineral composition, with the highest values associated with the highes
t content of stevensite and the lowest values with the highest content
of kerolite. This relation suggests that high salinities favored stev
ensite and low salinities favored kerolite. delta(18)O values of sepio
lite (meerschaum) fall in the middle of the range for Ke/St, suggestin
g that salinity was not the main control on sepiolite precipitation. H
igh values of a(SiO2)/a(Mg2+) may have been a major factor in sepiolit
e precipitation. Different mixtures of dilute ground water and saline,
alkaline lake water in pore fluids may largely account for the differ
ences in clay mineralogy of cavity-filling clays. Sepiolite is the dom
inant clay mineral in lacustrine sediments of the Amboseli Basin, and
the cavity-filling sepiolite may reflect a high proportion of lake wat
er. The low-Al Ke/St may have formed from fluids with a higher proport
ion of ground water. Detrital clay was very likely a factor in forming
the Al-Ke/St, for which delta(18)O values suggest a saline environmen
t.