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Mario Andrés Hamuy Wackenhut (born 1960) 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.

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  • Mario Hamuy (cs)
  • Mario Hamuy Wackenhut (es)
  • Mario Hamuy (en)
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  • Mario Andrés Hamuy Wackenhut (born 1960) 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. (en)
  • Mario Hamuy (* 25. květen 1960) je chilský astronom. Vyučuje astronomii na Universidad de Chile a Cerro Chalan Observatory. Profesně se zabývá pozorováním všech tříd supernov, zejména pozoruje supernovy typu Ia a II, které slouží k určování kosmických vzdáleností. Na Universidad de Chile studoval astronomii a fyziku. V únoru 1987 přišel do Cerro Tololo Inter-American Observatory a několik dní poté byla pozorována exploze supernovy typu II SN 1987A ve Velkém Magellanově oblaku, což odstartovalo velkou kampaň pro pozorování této důležité supernovy. (cs)
  • Mario Andrés Hamuy Wackenhut (Santiago, 25 de marzo de 1960) es un astrónomo chileno de ascendencia siria.​ Ha sido profesor de Astronomía de la Universidad de Chile y Director del Observatorio Cerro Calán. Presidente de la Fundación Chilena de Astronomía,​ es reconocido por su trabajo de observación de diferentes clases de supernovas, especialmente las supernovas de tipo Ia y II como medidas de distancia cósmica. En agosto de 2015 recibió el Premio Nacional de Ciencias Exactas.​ (es)
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  • Mario Hamuy (en)
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  • Mario Hamuy (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/MarioHamuy09.jpg
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