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<a accesskey="3" href="page.php?w=Mario_Hamuy&amp;p=2">3.Next</a>
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<p><b>Mario Andrés Hamuy Wackenhut</b> (born 1960) is a <a href="page.php?w=Astronomy_in_Chile">Chilean Astronomer</a> and Professor of Astronomy at the <a href="page.php?w=University_of_Chile">University of Chile</a> 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 <a href="page.php?w=Cosmic_distance_ladder">supernovae as measures of cosmic distance</a>.</p>

<p><big> Career </big></p>
<p>Mario Hamuy is the son of <a href="page.php?w=Mario_Hamuy_Berr">Mario Hamuy Berr</a>,</p><p>
<a accesskey="3" href="page.php?w=Mario_Hamuy&amp;p=2">3.Next</a>
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