HD 41004

Autorius (-iai): Trappist-1F_Ce

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HD 41004 is a binary star system composed of a K-type star and a red dwarf, located about 137 light-years from Earth. Component A (left) has a gas giant planet with a mass about 2.54 times that of Jupiter, while component B (right) has a low-mass brown dwarf with an orbital period of less than two Earth days.

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Atidaryti naudojant Celestia (rekomenduojama) arba Atsisiųsti

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