Evidence for Universality in the Initial Planetesimal Mass Function

Planetesimals may form from the gravitational collapse of dense particle clumps initiated by the streaming instability. We use simulations of aerodynamically coupled gas-particle mixtures to investigate whether the properties of planetesimals formed in this way depend upon the sizes of the particles that participate in the instability. Based on three high-resolution simulations that span a range of dimensionless stopping times 6 ×10^-3 ≤ τ ≤ 2, no statistically significant differences in the initial planetesimal mass function are found. The mass functions are fit by a power law, dN/ dM_p ∝ M^-p_p, with P = 1.5-1.7 and errors of Δp ≈ 0.1. Comparing the particle density fields prior to collapse, we find hat the high-wavenumber power spectra are similarly indistinguishable, though the large-scale geometry of structures induced via the streaming instability is significantly different between all three cases. We interpret the results as evidence for a near-universal slope to the mass function, arising from the small-scale structure of streaming-induced turbulence.