Little Johnny carves out a ship shape from a material of density . When he puts the ship in the water of density it floats and stays stable (does not list or turn over), as shown on the left-hand side of the figure.
After a while, Johnny gets bored with his ship and decides to turn it upside down as in the right-hand side.
Will the ship be stable in that position, too?
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For each position of the ship floating on the water there is a well defined potential energy of the ship and the displaced water. This energy depends on the orientation of the ship, E = E ( u ) , where u is a unit vector attached to the ship. The ship is stable if this potential energy increases when the orientation of the ship is changed by a small amount. (This corresponds to a small rotation of u around one of the many horizontal axes going through it.) We will show that there is a general symmetry in the problem, and the potential energy of the inverted ship has a very simple and straightforward relationship to the ship in the normal position. In particular, we will show that for ρ = 0 . 5 E ( u ) = E ( − u ) and therefore if E ( u ) has a local minimum around u = u 0 , so does E ( − u ) around u = − u 0 .
We pick and arbitrary u in the vicinity of u 0 , the equilibrium position. For the calculation of the potential energy we need to add up all of the infinitesimal contributions of d E = z g ρ d V = = z g ρ A ( z ) d z . Here g is the acceleration of gravity and A ( z ) is the horizontal cross section area of the ship at elevation z . We will select the water surface for z = 0 . The potential energy of the ship is g ρ [ ∫ z m i n 0 z A ( z ) d z + ∫ 0 z m a x z A ( z ) d z ] . The potential energy of the displaced water is − g ρ w ∫ z m i n 0 z A ( z ) d z . The total energy is
E= g ( ρ − ρ w ) ∫ z m i n 0 z A ( z ) d z + g ρ ∫ 0 z m a x z A ( z ) d z . . . . . ( 1 ) .
We also need to make sure that we use the correct reference point for the z scale. The position of the waterline of the ship is determined by Archimedes' law:
g ( ρ − ρ w ) ∫ z m i n 0 A ( z ) d z + g ρ ∫ 0 z m a x A ( z ) d z = 0 . . . . . ( 2 ) .
Notice that the function A ( z ) is derived from the information we know about the shape of the ship. This function will depend on the orientation of the ship (i.e. u ) and it can be rather complicated. However, when we invert the ship, making u ′ = − u the A ( z ) function will be the same, except for a z ′ = − z replacement. The corresponding equations for the ship turned upside down are:
E'= g ( ρ − ρ w ) ∫ − z m a x 0 z A ( − z ) d z + g ρ ∫ 0 − z m i n z A ( − z ) d z .
g ( ρ − ρ w ) ∫ − z m a x 0 A ( − z ) d z + g ρ ∫ 0 − z m i n A ( − z ) d z =0.
Introducing z ′ = − z and ρ ′ = ρ w − ρ , we get
E'= g ρ ′ ∫ 0 z m a x z ′ A ( z ′ ) d z ′ + g ( ρ ′ − ρ w ) ∫ z m i n 0 z ′ A ( z ′ ) d z ′ . . . . . ( 3 ) .
g ρ ′ ∫ 0 z m a x A ( z ′ ) d z ′ + g ( ρ ′ − ρ w ) ∫ z m i n 0 A ( z ′ ) d z ′ = 0 . . . . . ( 4 ) .
Comparing these two expressions to Eqs. (1) and (2), we recognize that the inversion of the ship and changing the density from ρ to ρ ′ = ρ w − ρ yields the same waterline [Eqs. (2) and (4)] and the same potential energy [Eqs. (1) and (3)]. With ρ = 0 . 5 we have ρ ′ = ρ w − ρ = 0 . 5 as well. Accordingly, in our case the inverted ship is as stable as the upright ship.