Black Hole Apocalypse | Stellar Life Cycles
Learn how the life cycles of low-mass and high-mass stars differ, in this video from NOVA: Black Hole Apocalypse. After a high-mass star begins to fuse iron, there is not enough outward pressure to remain stable, and the star collapses rapidly. Use this resource to stimulate thinking about stellar nucleosynthesis and evolution and to communicate explanations with others. This resource is part of the NOVA: Black Hole Apocalypse Collection. CREDITS: https://www.pbslearningmedia.org/credits/nvbh-sci-stellarlife/ LICENSE: https://www.pbslearningmedia.org/help/full-license-for-section-3c-of-terms-of-use-download-and-share/
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