Atmospheric Loss Calculator

Atmospheric erosion from planetesimal impacts and giant impacts using the prescriptions from existing studies.

Planetesimal Impact Loss

Sinclair & Wyatt (2021)

Calculation steps and references
  1. The impact regime is classified with \(H_{1/2}\) and \(H_{\mathrm{fr}}\) using the modified Sinclair and Wyatt (2021) coefficients.
  2. Cratering loss uses the erosional efficiency \(\xi\) and \(\chi_a(\xi)\) prescription from Shuvalov (2009).
  3. The single-impact atmospheric cap uses the polar-cap limit from Schlichting et al. (2015).
  4. Aerial-burst loss uses the Shuvalov et al. (2014) scaling.
  5. 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.

Giant Impact Loss

Kegerreis et al. (2020)