Download PDF by Luyten W.J.: Notes on Stellar Statistics III. On the Calculation of a

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Additional info for Notes on Stellar Statistics III. On the Calculation of a Mean Absolute Magnitude from Apparent Magnitudes, Angular Proper Motions and Linear Radial Velocities

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T. Arndt Archaean komatiite sequence, Barberton Mountain Land, South Africa. , 37: 125-1 46. , 1980. Tertiary or Mesozoic komatiites from Gorgona Island, Colombia; field relations and geochemistry. Contrib. Mineral. , 73: 253-266. , 1982. Komatiites from Gorgona Island, Colombia. T. G. ), Komatiites. George Allen and Unwin, London, pp. 199-210. , 1975. Genesis of Archaean peridotitic magmas and constraints on Archaean geothermal gradients and tectonics. Geology, 3: 15-18. , 1981. Petrogenesis of Archean ultramafic magmas and implications for Archaean tectonics.

Whereas this element appears to have been relatively immobile in the Zvishavane flows, data from most other komatiites scatter widely in variation diagrams and show no relationship to olivine control lines (Fig. 8). Many komatiites appear to have lost a large proportion (5040%)of their original Na. Mobility of Mg In general MgO seems to have been relatively immobile in Archean komatiites. This is shown by the tight trends in diagrams of MgO vs various immobile elements, and by the appropriate intercepts with MgO axes in variation diagrams.

This temperature is about 250°C above the liquidus temperature of the magma, which can be estimated from the 20% melting contour in Fig. 14: -1300°C at 0 GPa. This magma is a superheated picrite, not a komatiite. True komatiites form at higher degrees of melting or at greater depths. Path B-BI is that of a magma that forms by about 60% partial melting but interacts with wall rocks or with shallower-level melts as it ascends from the site of initial magma segregation to the surface. This magma also reaches the surface with a temperature of 1600°C.

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