I offer some comments which might complement the valuable recent paper by De Angelis et al (1987), on the newly discovered nickel-copper deposit at Radio Hill.The authors have accepted subdivisions and correlations by Hickman (1977, 1983) although they are disputed (Fitton, Horwitz and Sylvester, 1975; Horwitz, 1979; Horwitz and Guj, 1986).Also, in my opinion, more plausible correlations of the Sholl Belt with Whim Creek Belt have been shown, but not discussed, in Hudson and Horwitz (1986, Figure 1). Our suggested correlations and subdivisions have appeared in publications and reports which are not readily available, but it is gratifying to note that many of the observations and conclusions of De Angelis et al are consistent with our conclusions of the Whim Creek Belt.The units of the Sholl Belt (of Hickman, 1983), between the Sholl Fault (Shear Zone) and the overlying Mt Bruce Supergroup to the south, equate well with units of the Whim Creek Belt. A basalt, characterised by an abundance of vesicles and similar in many ways to the Wararnbi Basalt of Fitton, Horwitz and Sylvester (I975), is well developed at the base of the succession, particularly in the southern part of the area (Figure 1). It is overlain by acid tuffs (locally metamorphosed, such as at Whundoo Mine) and associated acid and mafic lavas, similar to those of the Mons Cupri area. The mafics in the succession are marked by the absence of the numerous cherty sedimentary intercalations, such as the Marble Bar Chert, which occur in the Warrawoona Group; and they also lack the intense chertification that is prevalent in all parts of the proven areas of Warrawoona Group rocks.The Whim Creek Group is overlain, locally unconformably (two to three km east of Mount Negri), by the Negri Volcanics which include here the Louden Volcanics (unit Abu of Hickman, 1977), (Horwitz, 1979). The negri volcanics are an alternating sequence of variolitic and quench textured lavas not dissimilar to the highest units of the Sholl Belt (Figure 1). They range from high-Mg basalt to tholeitic andesites (Glikson et al, 1986, pp 79 and 84). The whole succession of the Sholl Belt is estimated to be of the order of four km in thickness, more consistent with the two km thick (Horwitz, 1979, Figure 1) Whim Creek area sequence than with the much thicker Warrawoona Group sequences. The Whim Creek Group (including the Negri Volcanics) is considered to be a widespread grouping (Fitton, Horwitz and Sylvester, 1976; Horwitz, 1979; Horwitz and Guj, 1986) which is prevalent in the northern part of the Pilbara Craton. It is considered by these authors to include the Mallina Formation turbidites of the trough area of Ryan (1965). One component, the Mons Cupri Volcanic, is about 2.95 Ga (Richards and Blockley, 1984). Between the Sholl Fault and Egina, the Whim Creek Group is intruded by large ultrarnafic to granophyric ills of the Millindinna Complex (Fitton, Horwitz and Sylvester, 1975), dated at 2.860_x000D_
002 Ga by Gulson and Korsh (1983) near the Sherlock River (south side of Caines Well Granite area). The Millindinna Complex has been equated to the same magmatic episode as the layered complexes of the Sholl Belt by Fitton, Horwitz and Sylvester (1975, p 20).