Distribution of thermal conductivity K (left columns) and thermal inertia Γ (right column) of Kamo’oalewa, obtained with the ASTERIA method. Different rows correspond to different physical parameter modeling listed in Table 2. Blue histograms correspond to results obtained with the nominal orbit solution of Table 3. Red histograms are results obtained with the lower S/N Yarkovsky detection of A₂ = (−136.28 ± 15.82) × 10⁻¹⁵ au d⁻², which does not take into account the measured astrometric errors for specific observations.