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Fundamentals of Naval Architecture | Chapter 1: Calculation of Displacement and Other Hydrostatic Properties 1.3 Calculation of Displacement Volume and Displacement

To determine a ship’s displacement, it is first necessary to calculate the volume of the hull below the waterline.

If the submerged cross-sectional area of the hull is known at each position, the total submerged volume of the hull can be determined by integrating these areas along the length of the ship.

This article explains how to determine displacement volume from cross-sectional areas and how to calculate displacement.

Calculating Displacement Volume from Cross-Sectional Areas

Let the distance measured forward from the aft perpendicular (A.P.) be x[m]x[\mathrm{m}], the draft be d[m]d[\mathrm{m}], and the submerged cross-sectional area of the hull at that position be A(x,d)[m2]A(x,d)[\mathrm{m^2}].

If the hull is divided longitudinally into infinitesimal sections of width dx[m]dx[\mathrm{m}], the submerged volume of each section is expressed as A(x,d)dx[m3]A(x,d)\,dx[\mathrm{m^3}].

Integrating these volumes from the aft perpendicular (A.P.) to the forward perpendicular (F.P.) gives the displacement volume (d)[m3]\nabla(d)[\mathrm{m^3}] at draft d[m]d[\mathrm{m}].

(d)=0LPPA(x,d)dx(1.31)\nabla(d)=\int_{0}^{L_{PP}}A(x,d)\,dx \quad (1.3\text{-}1)



Here, LPP[m]L_{PP}[\mathrm{m}] represents the length between perpendiculars, which is the horizontal distance from the aft perpendicular (A.P.) to the forward perpendicular (F.P.).

Here, the submerged portion of the hull is assumed to lie entirely between the aft perpendicular (A.P.) and the forward perpendicular (F.P.).
If any submerged portions extend beyond this range, their volumes must also be included.

Let the transverse distance from the ship’s centerline to the side of the hull on one side be b(x,z)[m]b(x,z)[\mathrm{m}], and let the height measured vertically upward from the baseline be z[m]z[\mathrm{m}].
For a hull that is symmetrical about its centerline, the displacement volume can also be expressed as follows.

(d)=0LPPA(x,d)dx=20LPP{0db(x,z)dz}dx(1.32)\begin{aligned} \nabla(d) &=\int_{0}^{L_{PP}}A(x,d)\,dx\\ &=2\int_{0}^{L_{PP}}\left\{\int_{0}^{d}b(x,z)\,dz\right\}dx \end{aligned} \quad (1.3\text{-}2)



The inner integral determines the submerged cross-sectional area at each longitudinal position, while the outer integral integrates these areas along the length of the ship.
The displacement volume \nabla is normally expressed in [m3][\mathrm{m^3}].

Figure 1.3-1 Method for Calculating Displacement Volume from Cross-Sectional Areas

Figure 1.3-1 Method for Calculating Displacement Volume from Cross-Sectional Areas

Relationship Between Displacement Volume and Displacement

When a ship floats on the water, the submerged portion of its hull displaces a volume of water equal to its own volume.
Therefore, the displacement volume [m3]\nabla[\mathrm{m^3}] is also the volume of water displaced by the ship.

Let the density of seawater be ρsw[kg/m3]\rho_{sw}[\mathrm{kg/m^3}], the gravitational acceleration be g[m/s2]g[\mathrm{m/s^2}], and the specific weight of seawater be γsw[N/m3]\gamma_{sw}[\mathrm{N/m^3}]. Their relationship is expressed as follows.

γsw=ρswg(1.33)\gamma_{sw}=\rho_{sw}g \quad (1.3\text{-}3)



If the weight of the displaced seawater is represented by Δ[N]\Delta[\mathrm{N}], the following equation applies.

Δ=ρswg=γsw(1.34)\Delta=\rho_{sw}\nabla g=\gamma_{sw}\nabla \quad (1.3\text{-}4)


This is the weight of the seawater corresponding to the displacement volume.

According to Archimedes’ principle, the magnitude of the buoyant force FB[N]F_B[\mathrm{N}] acting on the hull is equal to the weight of the seawater displaced by the ship.

FB=Δ(1.35)F_B=\Delta \quad (1.3\text{-}5)



Weight of a Floating Ship

When a ship is floating at rest, the upward buoyant force FB[N]F_B[\mathrm{N}] acting on the hull is in equilibrium with the downward weight of the ship W[N]W[\mathrm{N}].

W=FB(1.36)W=F_B \quad (1.3\text{-}6)


Since FB=ΔF_B=\Delta, the following relationship is obtained.

W=FB=Δ(1.37)W=F_B=\Delta \quad (1.3\text{-}7)


In other words, the weight of a floating ship is equal to the weight of the seawater displaced by the ship.

It is difficult to measure a ship’s weight directly. However, if the shape of the hull is known, the ship’s weight can be determined by calculating its displacement volume from its draft and then calculating the weight of the displaced water.

Units of Displacement

The expression Δ=ρswg\Delta=\rho_{sw}\nabla g used above represents the magnitude of the gravitational force acting on the displaced water.
If ρsw\rho_{sw} is expressed in kg/m3\mathrm{kg/m^3}, \nabla in m3\mathrm{m^3}, and gg in m/s2\mathrm{m/s^2}, the unit of Δ\Delta is N\mathrm{N}.

On the other hand, when a ship’s displacement is expressed in t\mathrm{t}, it represents the mass of the displaced water.
In this case, if the density is expressed in t/m3\mathrm{t/m^3}, the equation is written as follows.

Displacement[t]=ρsw[t/m3]×[m3](1.38)\text{Displacement}\;[\mathrm{t}] =\rho_{sw}\;[\mathrm{t/m^3}] \times\nabla\;[\mathrm{m^3}] \quad (1.3\text{-}8)



Thus, even though the same term “displacement” is used, the units must be checked to determine whether it represents weight as a force or mass.

Summary

A ship’s displacement volume is determined by integrating its submerged cross-sectional areas along its length.

When a ship is floating at rest, Archimedes’ principle states that the buoyant force is equal to the weight of the water corresponding to the displacement volume, and this force balances the weight of the ship.

Therefore, determining the displacement volume from the hull form and draft is the starting point for calculating both the ship’s displacement and its weight.

About This Article

Reference
An Introduction to Naval Architecture in One Volume, edited by the Maritime College Career Education Research Association


※This article was prepared with reference to the source listed above and organized based on the author’s understanding.


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