An infrared survey of white dwarfs concluded that many dead stars are surrounded by dead planets that hurl smaller rocky masses toward the stars, where they are torn apart by gravitational tides. Issue
An infrared survey of white dwarfs concluded that many dead stars are surrounded by dead planets that hurl smaller rocky masses toward the stars, where they are torn apart by gravitational tides.
An infrared survey of white dwarfs concluded that many dead stars are surrounded by dead planets that hurl smaller rocky masses toward the stars, where they are torn apart by gravitational tides.