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Fig. 1

image

Left panel, Top: comparing terms in Eq. (24) for 1 Earth-mass planet. Left panel, Bottom: corresponding time scales. The dotted line indicates when the “migration” time scale τm becomes negative, which could lead to an artificial outward migration if τm is used in place of τa in Eq. (21). Right panel: normalised torques for various planetary masses in the inner region of a disc. The torque becomes positive for an Earth-mass planet. The discontinuity around 0.1 AU is caused by the treatment of the inner disc edge (see Sect. 2.1).

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