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Fig. C.5.


Distribution of eccentricities of planets captured by a NS. Each data point represents the mean value of the eccentricity of a specific planet (Mercury ☿ to Neptune ♆) if it was captured by a NS. The data were compiled from all pre-evolved states of the SS for a given set of initial conditions (impact parameter, bNS, encounter velocity, vNS, and the incidence angle, θNS) – i.e. the panels do not show how many planets were captured in total (see Fig. C.1 for reference). No planets were captured in the fastest scenario.

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