Habitable Worlds Around White Dwarf Stars?
In The Astrophysical Journal Letters, astronomer Eric Agol argues that searches for exoplanets should be expanded to include white dwarf stars, because planets orbiting those stars would be easier to spot: white dwarfs are small enough that a transiting planet would eclipse the stellar disc significantly, and the star’s habitable zone would be so close that a habitable planet would transit within 32 hours. I’d be interested to know how white dwarfs, which are supposed to be stars at the end of their lives, could have planets that close; they started out as much bigger stars, and a close-in habitable planet would have had to come from somewhere further out, wouldn’t it? Via 80beats.









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