Extended Data Fig. 5: Initial condition of N-body simulations.
From: Asteroid Kamo‘oalewa’s journey from the lunar Giordano Bruno crater to Earth 1:1 resonance
We start each set of simulation at a random lunar phase ϕ, which indicates the relative position of the Sun-Earth-Moon system, and launched 300 particles along a θ = 45∘ cone at random azimuths ζ and with a given velocity magnitude distribution v0 (following a power law distribution ranging from 2.38 to 6.0 km/s, and with the power of -4.0 according to Supplementary Fig. 7).
