The Cr# (100Cr/(Cr + Al)) and Fe2# (100Fe(2+)/(Mg + Fe2+)) of Cr-spine
ls affected by low-temperature reequilibration with olivine are contro
lled by isotherms with shallow slopes on the Cr# vs. Fe2# diagram. Con
sequently, in slowly cooled olivine-rich plutonic rocks, the Fe2# of C
r-spinel is an unreliable measure of the degree of evolution of the ma
gma from which it crystallized. For example, high-Cr# spinels in a ree
quilibrated dunite could have a higher Fe2# than low-Cr# spinels in a
reequilibrated gabbro, despite the fact that the spinel in the gabbro
originally crystallized at a lower temperature from a more evolved liq
uid than did the spinel in the dunite. As a result, the distribution o
f data points is difficult to interpret when minor elements in Cr-spin
el (Ti, V, Fe3+, Mn) are plotted against Cr-spinel Fe2#. A solution to
this problem is to project spinel compositional data onto an axis per
pendicular to isotherms in Cr# versus Fe2# space. This allows better d
iscrimination of spinel compositional associations and trends. The com
positional changes attendant upon down-temperature reequilibration of
Cr-spinels also causes problems when comparing Cr-spinels from plutoni
c rocks with those from volcanic rocks or liquidus-temperature numeric
al models. A solution to this problem is to recalculate high-temperatu
re spinels to their low-temperature equilibrium compositions before ma
king the comparison. A procedure is outlined allowing higher-temperatu
re spinels to be adjusted down to the 700 degrees C isotherm. (C) 1997
Elsevier Science B.V.