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Total alkali ? silica (TAS) diagram for Vesuvius starting materials, experimental glasses and eruption products. (a) Insert shows composition of starting materials. Rocks considered in this study are a trachybasalt (VS96-54A) and two tephrites, pp.97-718 ,
The composition of the phonotephrite V 1 of Dolfi & Trigila (1978) is indicated. The four phonolites studied by Scaillet et al. (2008) are also shown. (b) Comparison between experimental glasses (this study) and Vesuvius eruption products. The experimental data points are distinguished by starting material, 1993. ,
CaO vs MgO plot for (a) experimental glasses (Table 6) and (b) glass inclusions (recalculated compositions from Marianelli et al, 1995. ,
The glass inclusion data are distinguished by type of host crystal (either Ol or Cpx) Experimental symbols indicate a cotectic phase assemblage (Ol+Cpx) when filled and single phase assemblages (either Ol or Cpx, phase assemblage specified next to the appropriate data points) when open. Experiments from this study are distinguished by starting material (either VS96-54A or VES9) and addition of olivine. See Tables 3-4 for more information about experimental conditions. The 1150°C, 200 MPa olivine + clinopyroxene cotectic is defined by the three VS96-54A One point of the 50 MPa, 1100°C cotectic is defined by the VS96-54A charge #7-1. The three olivine-bearing, are labelled with temperature (either 1150 or 1200°C). They plot on olivine control lines that extend from the VS96-54A and VES9 starting glasses (Table 6) toward Fo-rich olivine, 1995. ,
the composition of experimental glasses from this study, of tephrite V36 (Trigila & De Benedetti, 1993) and of Vulsini leucite basanite B23 Table 7) are shown for comparison with the glass inclusions, 2009. ,
Redox state of primitive Vesuvius liquids as constrained from olivine-liquid equilibrium. Each curve gives the Fo content of olivine at equilibrium with a given trachybasaltic liquid for different ?NNO. Five trachybasaltic liquid compositions have been selected. They correspond to the most primitive glass inclusions from five different eruptions within the 1637-1944 period of activity of Vesuvius ,
The composition of their host olivine) is given by the five crosses. Chemical equilibrium is assumed between each trapped melt and its host olivine crystal, yielding a unique ?NNO equilibrium value. Note the narrow range of ?NNO (from +0.6 to +0.9) for the five glass inclusion-host olivine pairs selected, 1995. ,