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Fig. 1

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Potentially detectable currently-known exoplanets (coloured circles and histograms) compared to the total population of known exoplanets within 20 pc (grey dots and histograms), shown both as a function of their distance to the Solar System (top row) and their semimajor axis (bottom row). For LIFE (green), we assume the reference 4 × 2 m configuration with 5% throughput and consider planets as detectable if tint(S/N = 7) < 100 h. For the notional HWO (blue), potential targets in reflected starlight are those that meet our IWA, OWA and Cmin requirements (Sect. 2.3) and have Paccess > 25%. In all subplots, the value of Mp reported for the potential targets is the output of our statistical methodology (Sect. 2.1). For the non-detectable exoplanets we plot Mp or alternatively Mp sin i as reported in the NASA Archive. Horizontal lines indicate the masses of Neptune (blue), Earth (green) and Mars (red).

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