Sunlight heating and evaporating the disk of gas and dust around a young star (as seen in this illustration) may have triggered a shift in the orbits of the still-forming giant planets in the solar system’s early history.
JPL-Caltech/NASA
Sunlight heating and evaporating the disk of gas and dust around a young star (as seen in this illustration) may have triggered a shift in the orbits of the still-forming giant planets in the solar system’s early history.
JPL-Caltech/NASA