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The Life of Stars

In Our Time

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The Cosmic Orchestra of Stellar Evolution

The chapter explores the fusion process in stars, detailing how hydrogen fuses to form helium and the subsequent production of energy. It delves into the life cycle of stars, from hydrogen exhaustion to the creation of elements like carbon and iron, culminating in the explosive formation of heavier elements during supernovae. Neutron stars, the dense remnants of massive star cores, and historical supernova sightings in 1054 and 1987 are also discussed, painting a vivid picture of the intricate cosmic dance of element creation and stellar demise.

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