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Iron star

Hypothetical far-future compact star From Wikipedia, the free encyclopedia

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In astronomy, the term iron star has been used for two unrelated types of star:

Blue supergiant

An iron star is a type of blue supergiant which has a forest of forbidden FeII lines in its spectrum. They are potentially quiescent hot luminous blue variables. Eta Carinae has been described as a prototypical example.[1][2]

Compact iron star formation

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An iron star is a hypothetical type of compact star that could occur in the universe in the extremely far future, after perhaps 101500 years.

The premise behind the formation of iron stars states that muon-catalyzed fusion occurring via quantum tunnelling would cause the light nuclei in ordinary matter to fuse into iron-56 nuclei, due to its nature as the atomic nucleus with the lowest mass per nucleon.[3] Fission and alpha-particle emission would then make heavy nuclei decay into iron, converting stellar-mass objects to cold spheres of iron.[4] The formation of these stars is only a possibility if protons do not decay. Though the surface of a neutron star may be iron according to some predictions, it is distinct from an iron star.

By the end of 101026 to 101076 years, iron stars would have collapsed into neutron stars and black holes.[4]

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