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https://youtu.be/cMWMtLGGg6o
340,000 L
MKK Luminosity Class 0
M4la
Strengths
Weaknesses
When UY Scuti began to die, it entered the red supergiant phase and its core shrunk and became much hotter and denser. UY Scuti will evolve into either a yellow hypergiant, a luminous blue variable, or a Wolf-Rayet star. Eventually, its core will get so hot and dense that it will start fusing carbon into weaker elements: neon, oxygen, and silicon. After all the elements in UY Scuti have fused, only iron will remain at the core. The star will be so large that it cannot support itself, and its core will heat up to 100 billion degrees and collapse, electrons will be smashed into neutrons, protons, gamma rays, and neutrinos, and UY Scuti will finally explode and go supernova. When a star goes supernova, it has the brightness of one million Suns. During its supernova, UY Scuti will create a stellar wind and expel all of its outer layers and become either a neutron star or a black hole.
Benefits:
Costs:
Whitworth, N. John. “UY Scuti.” Universe Guide, 5 Apr. 2016, 5:03:44 PM, www.universeguide.com/star/uyscuti.
“The Largest Star We Know.” Telescope Observer, Telescope Review Guide, 24 Jan. 2018, telescopeobserver.com/uy-scuti/.
Cai, Zheluo. “UY Scuti, The Largest Known Star.” LIVING CORAM DEO, 21 Aug. 2017, www.livingcoramdeo.com/2016/10/07/uy-scuti-largest-known-star/.
“UY Scuti.” UY Scuti, 12 Apr. 2016, ipfs.io/ipfs/QmXoypizjW3WknFiJnKLwHCnL72vedxjQkDDP1mXWo6uco/wiki/UY_Scuti.html.
“Life Cycle of a Massive Star.” Astronomy Is Awesome, 23 Aug. 2015, astronomyisawesome.com/galaxies/life-cycle-of-a-massive-star/.