Analyzing the Setup
Imagine placing a solid block of iron into a pool of liquid mercury. Because mercury is incredibly dense—nearly 13.6 g/cm3 compared to iron's 7.8 g/cm3—the iron block floats easily, like an ice cube in water.
At any given temperature, the block settles into a state of translational equilibrium. The downward gravitational force acting on the block (its weight) is perfectly balanced by the upward buoyant force exerted by the mercury (the upthrust).
Let V be the total volume of the iron block, and ρFe be its density. The weight of the block is:
If a fraction k of the block's volume is submerged, the volume of mercury displaced is kV. The buoyant force is equal to the weight of this displaced mercury:
Equating these two forces gives us our master relation:
VρFeg=kVρHgg⟹k=ρHgρFe
This simple, elegant equation tells us that the submerged fraction k is purely determined by the ratio of the density of the floating solid to the density of the liquid.
The Master Equation at Different Temperatures
Now, let's look at how this system behaves at two different temperatures: 0∘C and 60∘C.
At 0∘C, the submerged fraction is k1. Using our master relation, we can write:
At 60∘C, the temperature of the system is raised. Both the iron block and the mercury expand, causing their densities to decrease. The new submerged fraction is k2:
To find the ratio k1/k2, we need to understand how density varies with temperature.
Thermal Expansion of Density
When a material is heated, its molecules vibrate more intensely, pushing each other slightly further apart. This causes the volume of the material to expand. The volume Vθ at a temperature θ is related to the initial volume V0 by:
where γ is the coefficient of volume expansion.
Since mass m is conserved during heating, the density ρθ must decrease as volume increases:
ρθ=Vθm=V0(1+γθ)m=1+γθρ0
Applying this physical law to both iron and mercury for a temperature rise of θ=60∘C, we get:
(ρFe)60=1+60γFe(ρFe)0
(ρHg)60=1+60γHg(ρHg)0
Final Calculation
Let's substitute these temperature-dependent densities back into our expression for k2:
k2=1+60γHg(ρHg)01+60γFe(ρFe)0=(ρHg)0(ρFe)0×1+60γFe1+60γHg
Notice that the term (ρHg)0(ρFe)0 is exactly equal to k1. Therefore, we can write:
k2=k1×1+60γFe1+60γHg
Rearranging this equation to find the ratio k1/k2 yields:
k2k1=1+60γHg1+60γFe
This beautifully matches option (a).