The Mystery of the Floating Sphere
Imagine you are handed a solid sphere, but it's not an ordinary one. Its density isn't uniform; it's denser at the core and gets lighter as you move towards the surface. The question asks us to find the minimum density of a liquid in which this peculiar sphere will float.
This is a classic test of Archimedes' Principle, but with a calculus twist!
Decoding "Minimum Density"
Why does the question specifically ask for the minimum density?
Think about how buoyancy works. The buoyant force pushing up on the sphere is equal to the weight of the liquid displaced. If the liquid is very dense, like mercury, the sphere might only need to displace a tiny volume to balance its weight, floating high above the surface.
But as we decrease the liquid's density, the sphere must sink deeper to displace more volume and generate enough buoyant force. The absolute limit—the minimum possible liquid density—occurs when the sphere is fully submerged but just barely touching the surface. At this point, it is displacing its maximum possible volume.
Setting Up the Master Equation
At this critical floating condition, the forces are perfectly balanced:
Wsphere=FB
The buoyant force
FB is straightforward. Since the sphere is fully submerged, the displaced volume is the total volume of the sphere.
FB=Vsphere⋅ρl⋅g=34πR3⋅ρl⋅g
The weight of the sphere, however, requires a bit more finesse. Because the density ρ(r) changes with the radius r, we can't just multiply a single density value by the total volume. We must integrate!
The Power of Integration
We imagine the sphere as a collection of infinitely many thin, concentric spherical shells, like the layers of an onion. Let's take one such shell at a distance r from the center, with a tiny thickness dr.
The volume of this shell is its surface area multiplied by its thickness:
4πr2dr.
The mass of this shell
dm is its volume multiplied by the density at that specific radius:
dm=ρ(r)⋅4πr2dr
To find the total mass, we integrate this expression from the center (
r=0) to the surface (
r=R):
∫0Rρ0(1−R2r2)⋅4πr2dr=34πR3ρl
Executing the Math
Now, let's roll up our sleeves and solve the integral. We can pull the constants
ρ0 and
4π outside the integral:
ρ0⋅4π∫0R(r2−R2r4)dr=34πR3ρl
Integrating term by term using the power rule:
ρ0⋅4π[3r3−5R2r5]0R=34πR3ρl
Applying the upper limit
R (the lower limit
0 just gives
0):
ρ0⋅4π(3R3−5R2R5)=34πR3ρl
ρ0⋅4π(3R3−5R3)=34πR3ρl
Finding a common denominator to subtract the fractions:
ρ0⋅4π(155R3−3R3)=34πR3ρl
ρ0⋅4π(152R3)=34πR3ρl
The Final Reveal
We are almost there! Let's clean up the equation by canceling the common terms
π and
R3 from both sides:
ρ0⋅158=34ρl
Solving for our target, the liquid density
ρl:
ρl=ρ0⋅158⋅43
ρl=52ρ0
And there we have it! The minimum density of the liquid must be 52ρ0. This beautiful result shows how calculus and physical principles intertwine to solve complex, non-uniform problems.