Nu Octantis

Autor(es): Gurren Lagann

Data de publicación:

Nu Octantis is a nearby binary star system of a K-type subgiant star and a white dwarf about 63.28 light-years away in the constellation Octans. The larger star has a large gaseous planet about 2.4 times more massive than Jupiter orbiting it

Nu Octantis Ab and its parent subgiant star

The white dwarf Nu Octantis B

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