that the pressure is below 45 GPa for its formation, and that it forms from rapid disordering of plagioclase feldspar by impact (P ~35 GPa, T ~200-600 C, t ~ 1-2 seconds). Others seem to state that this is a quenched melt from shock (e.g., Chen and El Goresy):
It looks like there was quite a debate a on this material a bit more than a decade ago (diaplectic glass vs. remnants of a shock melt). There's some hint of resolution in:
Sharp, T. G., & DeCarli, P. S. (2006). Shock effects in meteorites. Meteorites and the early solar system II, 653-677.
I am afraid you have to look at the shock literature for silicates and the equations of states of high-pressure silicate glass and then try to infer formation conditions.
Thanks for your answers. Actually, i`m familiar with the shock literature. Sharp and DeCarli, believe that maskelynite pressure stability has been overestimated ~2 orders of magnitude. But it is a really common mineral in meteorites and several papers have based their shock results on the presence of maskelynite; which is not correct. But, my question is, what is the abdolute true? What are the exact (?) P-T boundaries for this mineral?
I think we did see a glass of potassium feldspar-like composition in some fulgurites we analyzed. This material was isotropic with a feldspar composition, yet only required rapid heating, and not necessarily the corresponding increase in pressure. I'm not sure that would qualify as a maskelynite.
I think the SiO2 P-T-t diagram is better known than maskelynite?