Yarkovsky effect detection from ground-based astrometric data for near-Earth asteroid (469219) Kamo’oalewa

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Fig. 1

Typical amplitudes of the accelerations acting on the HO3 in heliocentric J2000 ecliptic reference system. The SRP acceleration amplitude is derived from Eq. (2) based on an assumed area-to-mass ratio of 1.965 × 10⁻⁵ m² kg⁻¹ and a Bond albedo of 0.083. See Sect. 5 for details.

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