Fig. 7

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Magnitude of (a) transverse and (b) radial Yarkovsky accelerations produced by DeepONet for a sphere asteroid shown in different parameter spaces, spanned by the specific heat capacity, C, the density, ρ, the distance from the Sun, r, the rotational inclination, β, the radius, R, and the thermal conductivity, κ. For the three situations, except for the two studied parameters, other parameters are fixed. The magnitude of acceleration is shown in the color bar.
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