Section 9.7

Surface Integrals, Coordinates of Centers of Gravity, and Moments of Inertia of Surfaces

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Problem 3661

A surface integral is called an integral of the form ∬σP dy dz+Q dz dx+R dx dy\displaystyle \iint \limits_{\sigma } P \, dy \, dz+Q \, dz \, dx+R \, dx \, dy. In computing it, the variables xx, yy, and zz are expressed in terms of two independent variables, using the equation of the surface f(x,y,z)=0f(x,y,z)=0 or its parametric equations x=φ(u,v)x=\varphi (u,v), y=ψ(u,v)y=\psi (u,v), z=ω(u,v)z=\omega (u,v). Another, more explicit way of writing surface integrals is ∬σ(Pcos⁡α+Qcos⁡β+Rcos⁡γ) dσ\displaystyle \iint \limits_{\sigma }(P\cos \alpha +Q\cos \beta +R\cos \gamma ) \, d\sigma, where α\alpha, β\beta, γ\gamma are the angles of the normal with the coordinate axes; here dσ=dx dycos⁡γd\sigma =\dfrac {dx\, dy}{\cos \gamma }.

The coordinates of the centers of gravity of parts of homogeneous surfaces having mass are found using surface integrals by the formulas:

Sxc=∬Sx ds,Syc=∬Sy ds,Szc=∬Sz ds;S=∬Sds. Sx_{c}=\iint \limits _{S} x \, ds, \qquad Sy_{c}=\iint \limits _{S} y \, ds, \qquad Sz_{c}=\iint \limits _{S} z \, ds; \qquad S=\iint \limits _{S} ds.

Here SS is the given part of the surface.

Find the coordinates of the center of gravity of the part of the shell of the sphere x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} for x>0x>0, y>0y>0, z>0z>0.

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Problem 3662

Find the coordinates of the center of gravity of the surface of a segment of the same sphere x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} for h<z<ah<z<a.

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Problem 3663

Find the coordinates of the center of gravity of the surface of the helicoid x=ucos⁡vx=u\cos v, y=usin⁡vy=u\sin v, z=hvz=hv for 0<u<a0<u<a, 0<v<π0<v<\pi.

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Problem 3664

Find the coordinates of the center of gravity of the part of the surface 3z=2(xx+yy)3z=2(x\sqrt{x}+y\sqrt{y}) bounded by the planes x=0x=0, y=0y=0, x+y=1x+y=1.

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Problem 3665

Find the coordinates of the center of gravity of the surface x2=2c(c−z)x^{2}=2c(c-z), bounded by the surfaces: y=kxy=kx, y=0y=0, z=0z=0.

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Problem 3666

Find the coordinates of the center of gravity of the part of the surface x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} bounded by the surfaces: x2+y2=axx^{2}+y^{2}=ax, z=0z=0.

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Problem 3667

Find the coordinates of the center of gravity of the part of the surface x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} bounded by the planes: x+y=±ax+y=\pm a, x−y=±ax-y=\pm a.

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Problem 3668

Find the moments of inertia of the part of the homogeneous surface of the cone h2(x2+y2)=a2z2h^{2}(x^{2}+y^{2})=a^{2}z^{2} for 0<z<h0<z<h relative to the axis OzOz.

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Problem 3669

Find the moment of inertia of the surface of the sphere x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} relative to a diameter.

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Problem 3670

Find the moment of inertia of the surface of the paraboloid x2+y2=2azx^{2}+y^{2}=2az relative to OzOz for 0<z<a0<z<a.

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Problem 3671

Find the moment of inertia of the surface of the spherical segment x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2} for h<z<ah<z<a relative to OzOz.

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Problem 3672

Compute the double integral ∬dsρ\displaystyle \iint \dfrac {ds}{\rho }, taken over the surface of the ellipsoid x2a2+y2b2+z2c2=1\dfrac {x^{2}}{a^{2}}+\dfrac {y^{2}}{b^{2}}+\dfrac {z^{2}}{c^{2}}=1, where ρ\rho is the distance from the center of the ellipsoid to the plane tangent to the element dsds of the surface of the ellipsoid.

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Problem 3673

Compute the integral ∬dsρn\displaystyle \iint \dfrac {ds}{\rho^{n}}, taken over the surface of the sphere x2+y2+z2=a2x^{2}+y^{2}+z^{2}=a^{2}, if ρ\rho is the distance from the surface element to the point (0,0,c)(0,0,c), located outside the sphere.

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Problem 3674

Show that the integral w=∬Scos⁡(r→,n→)r2 ds=∬S∂1r∂n ds\displaystyle w=\iint \limits_{S} \dfrac {\cos (\overrightarrow {r},\overrightarrow {n})}{r^{2}} \, ds=\iint \limits_{S} \dfrac {\partial \frac{1}{r}}{\partial n} \, ds, taken over the surface SS, equals the solid angle at which the surface SS is seen from the origin. Here r→\overrightarrow {r} is the radius vector from the origin to the surface element dsds; n→\overrightarrow {n} is the normal to the surface, forming an acute angle with the vector r→\overrightarrow {r} drawn from the origin. The quantity ∂u∂n\dfrac {\partial u}{\partial n} is defined by the equality

∂u∂n=∂u∂xcos⁡(n→,x)+∂u∂ycos⁡(n→,y)+∂u∂zcos⁡(n→,z). \frac{\partial u}{\partial n}=\frac{\partial u}{\partial x}\cos (\overrightarrow {n},x)+\frac{\partial u}{\partial y}\cos (\overrightarrow {n},y)+\frac{\partial u}{\partial z}\cos (\overrightarrow {n},z).
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