Station

Star system
Station distance
375 Ls
Landing pad
Large
Station type
Starport (Ocellus)

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Minor faction

Station update
15 Oct 2024, 10:46am
Location update
09 Sep 2024, 5:57pm
Market update
07 Sep 2024, 7:12pm
Shipyard update
07 Sep 2024, 7:11pm
Outfitting update
07 Sep 2024, 7:11pm

Galpedia

Mario Hamuy

Mario Hamuy is a Chilean Astronomer and Professor of Astronomy at the University of Chile and Cerro Calan Observatory. He is well known for his observational work on all classes of supernovae, especially the use of Type Ia and Type II supernovae as measures of cosmic distance. He was a student in astronomy and physics at the University of Chile working with Jorge Melnick. In February 1987, he came to the Cerro Tololo Inter-American Observatory and within a few days of his arrival when the Type II supernova SN1987A exploded in the Large Magellanic Cloud, he began a major campaign at CTIO to monitor this important supernova.

In 1989, in collaboration with Jose Maza, Mark M. Phillips, and Nicholas Suntzeff, he began the Calán/Tololo Supernova Survey which led to the pioneering work on the standard candle luminosities of Type Ia supernovae. This work led to the precise measurements of the Hubble Constant H0 and the deceleration parameter q0, the latter indicating the presence of a dark energy or cosmological constant dominating the mass/energy of the Universe.



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