Station
Similar stations in HIP 110397
Outpost (Civilian) - 128 Ls
Neutron Exploration Systems
Tilman Installation
Surface Port - 6,264 Ls
Neutron Exploration Systems
Abell Hub
Outpost (Civilian) - 6,432 Ls
Neutron Exploration Systems
Jones Silo
Surface Port - 6,432 Ls
HIP 3470 as one
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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