Meteorite records indicate solar system formation featured steady condensation of solids from a cooling nebula, early planetesimal creation by streaming instabilities that opened disk gaps, later chondrule accretion, and Earth's assembly from volatile-poor material followed by a Mars-sized impactor撞
The Astrophysical Journal, 910, 70
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From Dust to Planets -- A Chemical Perspective
Meteorite records indicate solar system formation featured steady condensation of solids from a cooling nebula, early planetesimal creation by streaming instabilities that opened disk gaps, later chondrule accretion, and Earth's assembly from volatile-poor material followed by a Mars-sized impactor撞