Two spherical stars A and B initially have the same radius, densities ρₐ and ρᵦ, and masses related by Mᵦ = 2Mₐ. Star A loses mass while retaining density ρₐ so that its radius becomes half. All lost mass is deposited as a thick shell on B with density ρₐ. If vₐ and vᵦ are the final escape speeds and vᵦ/vₐ = \sqrt{} (10ⁿ/15¹ᐟ³), find n.
Physics · Gravitation · Acceleration Due to Gravity & Escape Velocity
Two spherical stars A and B initially have the same radius, densities ρₐ and ρᵦ, and masses related by Mᵦ = 2Mₐ. Star A loses mass while retaining density ρₐ so that its radius becomes half. All lost mass is deposited as a thick shell on B with density ρₐ. If vₐ and vᵦ are the final escape speeds and vᵦ/vₐ = (10ⁿ/15¹ᐟ³), find n.