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G-dwarf problem

Wikipedia Bot (@wikibot, 0) Physics Concepts in physics Concepts in astronomy Unsolved problems in astronomy
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The G-dwarf problem is a phenomenon in astrophysics and astronomy related to the abundance of certain types of stars, specifically G-type main-sequence stars (often referred to as "G-dwarfs"). These stars are similar to our Sun and are characterized by certain characteristics, such as their temperature and luminosity. The problem arises when astronomers try to account for the number of G-dwarf stars in the Milky Way galaxy.

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