1997
DOI: 10.1346/ccmn.1997.0450408
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An Fe-Berthierine From A Cretaceous Laterite: Part I. Characterization

Abstract: Abstract--An Fe-berthierine occurs in a buried laterite from the Late Cretaceous (Cenomanian) in southwestern Minnesota. It formed beneath a lignitic horizon in which reducing solutions percolated through a laterite comprising gibbsite, kaolinite and goethite. Morphologic differences suggest 2 separate conditions of Fe-berthierine formation. Early forms of Fe-berthierine include radial bladed or radial blocky crystallites coating pisoids, along with alteration of kaolinite at crystal boundaries. These morpholo… Show more

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Cited by 50 publications
(43 citation statements)
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“…Most prob a bly it forms very early in diagenesis (Hornibrook and Longstaffe, 1996), by re ac tion of kaolinite and Fe-ox ides (Shel don and Retallack, 2002), as part of a lateritic weath er ing pro file de vel oped on a broad, low-re lief pe ne plain par tic u larly in a swampy en vi ron ment (Toth and Fritz, 1997). Pri mary crys tal liza tion of berthierine de mands a sup ply rich in iron, readily sol uble vol ca nic rock ma te rial and a high or ganic mat ter con tent (Hornibrook and Longstaffe, 1996); how ever, low lev els of sulfide and bi car bon ate are also re quired (Toth and Fritz, 1997;Shel don and Retallack, 2002). Oth er wise, the for ma tion of pyrite and sid er ite is fa voured, re spec tively.…”
Section: General Palaeoenvironmental and Palaeoclimatic Remarksmentioning
confidence: 99%
“…Most prob a bly it forms very early in diagenesis (Hornibrook and Longstaffe, 1996), by re ac tion of kaolinite and Fe-ox ides (Shel don and Retallack, 2002), as part of a lateritic weath er ing pro file de vel oped on a broad, low-re lief pe ne plain par tic u larly in a swampy en vi ron ment (Toth and Fritz, 1997). Pri mary crys tal liza tion of berthierine de mands a sup ply rich in iron, readily sol uble vol ca nic rock ma te rial and a high or ganic mat ter con tent (Hornibrook and Longstaffe, 1996); how ever, low lev els of sulfide and bi car bon ate are also re quired (Toth and Fritz, 1997;Shel don and Retallack, 2002). Oth er wise, the for ma tion of pyrite and sid er ite is fa voured, re spec tively.…”
Section: General Palaeoenvironmental and Palaeoclimatic Remarksmentioning
confidence: 99%
“…Plotting onto the diagram in Figure 4d all chemical analyses known to the authors of berthierine published in the literature, except those concerning exotic varieties such as titanian berthierine (Arima et al, 1985) and zincian berthierine Slack et al, 1992), the microcrystalline variety from the Kremikovtsi SIF can be defined as rich in Mg or Mgberthierine (of Fe-berthierine reported by Toth and Fritz, 1997). The compositional field of all known berthierines is considerably larger than that given by Cur- A part of the so-called vug-filling chamosite that is not associated with the barite-sulfide assemblage resembles intergranular fillings characteristic of microcrystalline berthierine, implying that it was a transformation product after berthierine during progressive diagenesis.…”
Section: Berthierinementioning
confidence: 99%
“…Some are SEDEX in origin (Damyanov and Vassileva, 2001;Xu and Veblen, 1996;Kimberley, 1989;Curtis andSpears, 1968 Wiewiora et al, 1998), other sulfide massive volcanogenic (Slack et al, 1992), metamorphic origin (Wybrecht et al, 1985), and associated to bauxite and laterite (White et al, 1985;Toth and Fritz, 1997). These minerals also occur in Northampton ironstone (Hirt and Gehring, 1991), in paleosol near Waterval Onder, South Africa (Retallack, 1986), in the oolitic ironstone beds, Hazara, Lesser Himalayan Copyright c The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB.…”
Section: Introductionmentioning
confidence: 99%