The sapphirine-like mineral surinamite, (Mg,Fe2+)3(Al,Fe3+)3O[AlBeSi3O15], occurs at South Harris as tiny grains enclosed in kyanite or as tabular grains up to 1 mm long mostly surrounded by Si-rich cordierite. A few surinamite grains enclose orthopyroxene, sillimanite, and Si-rich sapphirine. Ion microprobe analyses gave 3.52 to 3.81 wt% BeO (0.766 to 0.824 Be atoms per formula unit) and 2 to 13 ppm B in surinamite. Excess Si suggests the presence of significant BeO in cordierite and sapphirine. Given the anti-clockwise P-T-time path inferred for the South Harris rock, we suggest that surinamite formed at first by the continuous reaction BeSiAl−2 (in sapphirine) + sillimanite + orthopyroxene → surinamite + quartz and, subsequently, by the discontinuous reaction Be-depleted sapphirine + quartz → surinamite + orthopyroxene + kyanite with increase of P to >12 kbar at 850–900 °C. Surinamite reacted with orthopyroxene, kyanite, and quartz to form beryllian cordierite during subsequent decrease in P and T.

The high-silica content and peraluminous composition of the surinamite-bearing gneiss are consistent with a metasedimentary origin; this rock is markedly depleted in Th (0.13 ppm), U (0.11 ppm), Y (0.94 ppm), and rare-earth elements (e.g., Ce 7.7 ppm). Its bulk Be content (9 ppm) is not excessive. The appearance of a discrete Be phase in Be-poor rocks could be due to the absence of potential carriers of Be, namely muscovite and primary cordierite, at high T and low-water activity. Moreover, surinamite is indicative of a distinctive metamorphic history in which high-temperature rocks recrystallized at higher pressures or are isobarically cooled, and, consequently, scarcity of Be in metamorphic systems is not the only factor controlling surinamite formation.

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