Published Jul 10, 2021

Supernovas: They're a Blast

Gary Arndt delves into the captivating history and science of supernovas, unraveling their types and cosmic significance. Discover how these stellar explosions serve as "standard candles" for measuring astronomical distances and contribute to the universe's heavy elements, shaping our understanding of the cosmos.
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  • Type-I Supernovas

    Type-I supernovas occur in binary star systems where one star becomes a white dwarf. This white dwarf accumulates matter from its companion star until it reaches the Chandrasekhar limit, leading to a catastrophic explosion. These explosions are crucial for measuring cosmic distances due to their consistent luminosity.

    Every type one supernova explodes with the exact same mass and thus have the exact same luminosity.

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    Additionally, Type-I supernovas contribute to the creation of heavy elements, enriching the universe with materials like gold and uranium 1 2.

       

    Type-II Supernovas

    Type-II supernovas result from the collapse of a single massive star that has exhausted its nuclear fuel. When fusion stops, the star collapses under its own gravity, leading to a massive explosion. The remnants of such explosions can form neutron stars or black holes, depending on the star's initial mass.

    Once a star starts producing iron, it will no longer give off energy by fusing with other atoms.

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    These supernovas play a vital role in dispersing elements throughout the cosmos, contributing to the formation of new stars and planets 1.

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