Planetesimal Impact Loss
Sinclair & Wyatt (2021)
Calculation steps and references
- The impact regime is classified with \(H_{1/2}\) and \(H_{\mathrm{fr}}\) using the modified Sinclair and Wyatt (2021) coefficients.
- Cratering loss uses the erosional efficiency \(\xi\) and \(\chi_a(\xi)\) prescription from Shuvalov (2009).
- The single-impact atmospheric cap uses the polar-cap limit from Schlichting et al. (2015).
- Aerial-burst loss uses the Shuvalov et al. (2014) scaling.
- Collective-mass mode integrates over a power-law size distribution \(dN/dD \propto D^{-q}\) using the bounds and \(q\) values discussed in the notes: Hartmann (1964), Dohnanyi (1969), Neukum et al. (2001), and Schlichting and Mukhopadhyay (2018).
Collective mode uses a deterministic size-distribution integration, not a random draw, so repeated calculations are stable.