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
Earth and Planetary Science Letters 449, 302 –310 (2016) Albarède, F., 2009
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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