v will be used as the escape velocity from the astroid, vₑ = √(2GM/r).
So, √(2gh) = √(2GM/r); and
r = (MG/g)h⁻¹
M, the mass of the asteroid is vol • density; and the volume is 4.189r³; and, substituting known values:
r = ((3.5[3] kg/m³ • 4.189r³ • 6.67[-11 N (m/kg)²]/9.81 m/s²)h⁻¹
r = 9.968[-8]h⁻¹r³ (Round this off.)
1 = [-7]h⁻¹r²
r² = [7]h
r = √([7]h)
r = [3.5]√h
r = 3.16[3]√h
.