The Strange Case of Eta Carinae A

The video explores the fascinating characteristics of Eta Carinae A, a massive star that defies physics with its brightness and mass. It details the star's historical eruptions, which led to the formation of the homunculus nebula, and explains the nature of Luminous Blue Variables (LBVs), stars that undergo significant mass loss. The video also discusses the 3D modeling of the nebula and the potential for Eta Carinae A to go supernova. Finally, it invites viewers to support and subscribe to SciShow Space.

What makes Eta Carinae A one of the brightest stars in the galaxy?

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Describe the phenomenon that occurred with Eta Carinae A in the early 1800s.

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What is the significance of the homunculus nebula created by Eta Carinae A?

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How do Luminous Blue Variables (LBVs) differ from other stars in terms of mass loss?

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What are some of the unanswered questions regarding the LBV phase in high mass stars?

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