G. J. Consolmagno
Papers
1
Total Citations
184
H-Index
1
About
Brother G. J. Consolmagno, a Jesuit astronomer and planetary scientist at the Vatican Observatory, has fundamentally shaped our understanding of the Solar System’s smallest building blocks. His research centers on the physical and chemical properties of meteorites, asteroid-meteorite connections, and the evolution of small bodies. His most cited work, "Physical properties of the stone meteorites" (184 citations), systematically characterizes the density, porosity, and magnetic susceptibility of these extraterrestrial rocks, revealing how they reflect the formation and collisional history of their asteroidal parent bodies. This foundational dataset is critical for interpreting spacecraft data and modeling the early Solar System. Beyond this, Consolmagno’s contributions include pioneering studies on meteorite porosity—showing that many asteroids are highly porous, "rubble piles"—and co-authoring the widely used textbook *The Small Bodies of the Solar System*. A Fellow of the Meteoritical Society, he has also bridged science and faith through popular books and lectures, making him a unique and influential voice in planetary science. His work remains essential for any student seeking to connect meteorite samples to their cosmic origins.
Research Focus
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Top Papers
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