Relative change of the median escape times for asteroids due to the Yarkovsky effect. Vertical coordinates are obtained by comparing computations with and without YORP for each asteroid from Kankiewicz & Włodarczyk (2016, 2018). Colour-coding distinguishes between the two datasets, as well as integration into the past or the future. The horizontal axis is the relative distance to the closest planet from the asteroid’s pericentre, apocentre, or semi-major axis (see text for details). The 1σ and 2σ areas for the shot noise are shaded in yellow.