EN
We prove that if $ϱ_H$ and δ are the Hausdorff metric and the radial metric on the space 𝓢ⁿ of star bodies in ℝ, with 0 in the kernel and with radial function positive and continuous, then a family 𝓐 ⊂ 𝓢ⁿ that is meager with respect to $ϱ_H$ need not be meager with respect to δ. Further, we show that both the family of fractal star bodies and its complement are dense in 𝓢ⁿ with respect to δ.