Giventheobject’scomparativelyhighsurface-areatomassratio, other non-gravitational forces could play an important role. In particular, the Yarkovsky effect caused by delayed thermal emission as the object rotates causes a secular drift in the semi-major axis. Given the ∼ 4 m × 4 m × 2 m dimensions of the combined Tesla and Payload Attach Fitting (PAF), a useful point of comparison is 2009 BD, the smallest asteroid (4m across) with a measuredYarkovskydriftofda/dt≈0.05AU/Myr(Vokrouhlick´yetal. 2015). If we assume a density for the carbon-fibre surface of the Tesla of∼1000 kg m−3, a heat capacity of∼1000 J kg−1 K−1, and a thermal conductivity of∼100 W m−1 K−1, then the thermal inertiais∼104 inSIunits.Thisisroughlyanorderofmagnitudelarger than might be expected for 2009 BD. The Tesla rotates quickly compared to the thermal re-emission timescale with a period of 4.7589±0.0060 minutes2. Thus, similarly to small asteroids like 2009 BD, the Tesla is in the limit of large thermal parameter Θ, so the Yarkovsky drift scales inversely with the thermal inertia (Bottke et al. 2006). However, the effect also scales inversely with the density of the body. Assuming a total mass of ∼ 6000 kg for the combined Tesla and PAF, this yields a density of∼ 200 kg/m3, an order of magnitude lower than typical asteroids. Thus the effect of a larger thermal inertia is offset by the reduced density. In summary,areasonableestimateforthestrengthoftheYarkovskyeffect is∼0.05 AU/Myr, i.e. close to that of 2009 BD.