What About High-Mass Stars? | Evolution Of Stars

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After the red giant phase, they may go through successive stages of fusing heavier elements. Once iron is formed in the core, fusion can no longer release energy, leading to core collapse and a <a href="">supernova</a> explosion. The remnant core may become a <a href="">neutron star</a> or, if the star was massive enough, a <a href="">black hole</a>.</div></div> </div> <hr /> <h3 class="rq-heading">Frequently asked queries:</h3> <div class="qa-container"> <div class="qa-item"> <a href="https://theastrophysics.com/knowledgebase/how-do-stars-form" title="How Do Stars Form?">How Do Stars Form?</a> </div> <div class="qa-item"> <a href="https://theastrophysics.com/knowledgebase/what-happens-during-a-star-s-main-sequence-phase" title="What Happens During a Star鈥檚 Main Sequence Phase?">What Happens During a Star鈥檚 Main Sequence Phase?</a> </div> <div class="qa-item"> <a href="https://theastrophysics.com/knowledgebase/what-is-stellar-nucleosynthesis" title="What is Stellar Nucleosynthesis?">What is Stellar Nucleosynthesis?</a> </div> <div class="qa-item"> <a href="https://theastrophysics.com/knowledgebase/what-happens-when-a-star-exhausts-its-fuel" title="What Happens When a Star Exhausts Its Fuel?">What Happens When a 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What About High-Mass Stars? | Evolution Of Stars