Место издания:Kharkiv National University Kharkiv, Ukraine
Аннотация:Condensation of refractory elements in protosolar nebula was studied with usage of several thermochemical programs. Planned including of minerals into the list of studied species by
EQL program will help us to achieve better agreement with previous theoretical results and experimental
data and to understand deeper the role of impacts as a source of atoms in the exospheres of the
Moon and Mercury.