Brother Guy Consolmagno SJ is Director of the the Vatican Observatory and President of the Vatican Observatory Foundation. A native of Detroit, Michigan. Brother Guy Consolmagno, head of the Vatican Observatory, explains how he combines a love for science with his love for God. Brother Guy Consolmagno, SJ, is the Director of the Vatican Observatory and President of the Vatican Observatory Foundation. A native of.

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From he was a postdoctoral fellow and lecturer at the Harvard College Observatory, and from continued as postdoc and lecturer at MIT. Upon his return to the US in he became an assistant professor of physics at Lafayette College, in Easton, Pennsylvania, where he taught until his entry into the Jesuit order in He took vows as a Jesuit brother inand studied philosophy and theology at Loyola University Chicago, and physics at the University of Chicago before his assignment to the Vatican Observatory in He has coauthored two astronomy books: Schaefer; Prentice Hall, With Paul Mueller, Image, Would You Baptize an Extraterrestrial?


Astronomy and the Vatican. Edited by Guy Consolmagno. Our Sunday Visitor, Adventures of a Vatican Scientist. The Way to the Dwelling of Light.

Br. Guy Consolmagno, SJ – Biography

Guy Consolmagno and Martha Schaefer. A Textbook in Planetary Sciences.

Guy Consolmagno and Dan M. Turn Left at Orion: Cambridge University Press, ; fourth edition, The period of rotation, shape, density, and homogeneous surface color of the Centaur Pholus. An impact origin for the foliation of chondrites. Density, magnetic susceptibility, and the characterization of ordinary chondrite falls and showers.

The significance of meteorite density and porosity. Evidence of N2-Ice on the surface of the icy dwarf planet FY9. The exploration history of Europa. Colors of inner disk classical Kuiper belt objects. The thermal conductivity of meteorites: New measurements and analysis.

Guy Joseph Consolmagno

Enstatite chondrite density, magnetic susceptibility and porosity. Density, porosity and magnetic susceptibility of achondritic meteorites.

Stony meteorite thermal properties and their relationship to meteorite chemical and physical states. The density and porosity of lunar rocks.


The measurement of meteorite heat capacity at low gyy using liquid nitrogen vaporization. The contamination of the surface of Vesta by impacts and the delivery of the dark material. Heterogeneity in lunar anorthosite meteorites: Is Vesta an intact and pristine protoplanet?