Mathematics · Book 4 · Bachelor Year 2

University Mathematics — Year 2

University Mathematics — Year 2 · Bachelor Year 2

19Surfaces

After curves, surfaces: two-parameter objects in R3\R^3. The differential calculus of Chapter 15 provides everything we need — partial derivatives give tangent vectors, the cross product gives the normal, determinants give areas. We define regular parametrized surfaces, their tangent planes, and the first fundamental form, which encodes all length and area measurements on the surface. Surfaces also arise as level sets f(x,y,z)=cf(x, y, z) = c; the gradient then directs the normal.

19.1 Parametrized surfaces

Definition 19.1 (Regular parametrized surface)

Let UR2U \subseteq \R^2 be open. A parametrized surface of class Ck\mathcal{C}^k (k1k \geq 1) is a map σ ⁣:UR3\sigma \colon U \to \R^3, (u,v)σ(u,v)(u, v) \mapsto \sigma(u, v), of class Ck\mathcal{C}^k. A point is regular if the partial derivative vectors

σu(u,v)=σu(u,v),σv(u,v)=σv(u,v)\sigma_u(u, v) = \frac{\partial\sigma}{\partial u}(u,v), \qquad \sigma_v(u, v) = \frac{\partial\sigma}{\partial v}(u,v)

are linearly independent, i.e. σuσv0\sigma_u \wedge \sigma_v \neq 0; the surface is regular if every point is.

Example 19.2 (The three standard descriptions)

  1. Graph: σ(u,v)=(u, v, f(u,v))\sigma(u, v) = (u,\ v,\ f(u, v)) for fC1(U)f \in \mathcal{C}^1(U). Always regular: σu=(1,0,fu)\sigma_u = (1, 0, f_u) and σv=(0,1,fv)\sigma_v = (0, 1, f_v) are independent.
  2. Sphere (spherical coordinates): for the sphere of radius RR,

    σ(θ,φ)=(Rcosθcosφ, Rsinθcosφ, Rsinφ),(θ,φ)R×(π2,π2),\sigma(\theta, \varphi) = (R\cos\theta\cos\varphi,\ R\sin\theta\cos\varphi,\ R\sin\varphi), \qquad (\theta, \varphi) \in \R \times \bigl(-\tfrac\pi2, \tfrac\pi2\bigr),

    with θ\theta the longitude and φ\varphi the latitude. One checks σθσφ=R2cosφ>0\norm{\sigma_\theta \wedge \sigma_\varphi} = R^2\cos\varphi > 0: regular away from the poles (which this chart omits).

  3. Level set: S={(x,y,z):f(x,y,z)=c}S = \{(x,y,z) : f(x, y, z) = c\} where ff is C1\mathcal{C}^1 and f0\nabla f \neq 0 on SS. Near each point, one coordinate can be expressed as a function of the other two by the implicit function theorem (Chapter 15), so SS is locally a graph.

Example 19.3 (From level set to graph)

The implicit function theorem in item 3 deserves one explicit run. Take the sphere x2+y2+z2=R2x^2 + y^2 + z^2 = R^2 near its north pole (0,0,R)(0, 0, R): there fz=2z=2R0\frac{\partial f}{\partial z} = 2z = 2R \neq 0, and solving for zz gives the graph chart

z=R2x2y2,x2+y2<R2,z = \sqrt{R^2 - x^2 - y^2}, \qquad x^2 + y^2 < R^2 ,

regular everywhere on its (open) domain — including the pole that the spherical chart missed. Near an equator point like (R,0,0)(R, 0, 0) the same theorem solves for xx instead (fx=2R0\frac{\partial f}{\partial x} = 2R \neq 0). The rule of thumb: a level surface is a graph over the coordinate plane orthogonal to the largest component of the gradient, and by covering the sphere with six such graph charts one checks its smoothness everywhere with no trigonometry at all.

19.2 Tangent plane and normal

Definition 19.4 (Tangent plane)

Let σ\sigma be regular at (u0,v0)(u_0, v_0), M0=σ(u0,v0)M_0 = \sigma(u_0, v_0). The tangent plane TM0ST_{M_0}S is the plane through M0M_0 directed by Vect(σu,σv)\operatorname{Vect}(\sigma_u, \sigma_v) (partials at (u0,v0)(u_0, v_0)). The unit normal is

n(u0,v0)=σuσvσuσv.n(u_0, v_0) = \frac{\sigma_u \wedge \sigma_v} {\norm{\sigma_u \wedge \sigma_v}} .

Proposition 19.5 (Tangent vectors are velocity vectors)

The direction of TM0ST_{M_0}S is exactly the set of vectors γ(0)\gamma'(0), where γ=σc\gamma = \sigma \circ c ranges over the C1\mathcal{C}^1 curves drawn on the surface through M0M_0 (i.e. c ⁣:(ε,ε)Uc \colon (-\varepsilon, \varepsilon) \to U is C1\mathcal{C}^1 with c(0)=(u0,v0)c(0) = (u_0, v_0)).

Proof. If c(t)=(u(t),v(t))c(t) = (u(t), v(t)), the chain rule (Chapter 15) gives

γ(0)=u(0)σu+v(0)σvVect(σu,σv).\gamma'(0) = u'(0)\,\sigma_u + v'(0)\,\sigma_v \in \operatorname{Vect}(\sigma_u, \sigma_v).

Conversely, the vector aσu+bσva\sigma_u + b\sigma_v is attained by the curve c(t)=(u0+at, v0+bt)c(t) = (u_0 + at,\ v_0 + bt), which stays in the open set UU for t\abs t small.

Example 19.6 (The helicoid’s tangent plane)

For the helicoid σ(u,v)=(vcosu, vsinu, au)\sigma(u, v) = (v\cos u,\ v\sin u,\ au), at the point σ(0,1)=(1,0,0)\sigma(0, 1) = (1, 0, 0):

σu=(0, 1, a),σv=(1, 0, 0),σuσv=(0, a, 1),\sigma_u = (0,\ 1,\ a), \qquad \sigma_v = (1,\ 0,\ 0), \qquad \sigma_u \wedge \sigma_v = (0,\ a,\ -1),

so the tangent plane is ay=za\,y = z. It contains the whole horizontal ruling {(t,0,0)}\{(t, 0, 0)\} (direction σv\sigma_v): as for the cone of Exercise 19.1, a surface ruled by straight lines has each ruling lying inside the tangent plane along it. The other tangent direction σu\sigma_u is the velocity of the helix uσ(u,1)u \mapsto \sigma(u, 1): one chart, two drawn curves, and the whole tangent plane is spanned — Proposition 19.5 in action.

Proposition 19.7 (Normal of a level surface)

Let S={f=c}S = \{f = c\} with ff of class C1\mathcal{C}^1 and f(M0)0\nabla f(M_0) \neq 0. Then the tangent plane of SS at M0M_0 is the plane through M0M_0 orthogonal to f(M0)\nabla f(M_0):

TM0S:f(M0), MM0=0.T_{M_0}S :\quad \langle \nabla f(M_0),\ M - M_0\rangle = 0 .

Proof. For any curve γ\gamma drawn on SS through M0M_0, f(γ(t))=cf(\gamma(t)) = c identically, so the chain rule gives f(M0),γ(0)=0\langle \nabla f(M_0), \gamma'(0)\rangle = 0: all velocity vectors are orthogonal to the gradient, so the tangent direction is contained in the plane f(M0)\nabla f(M_0)^\perp. Both are 22-dimensional subspaces — the tangent direction because SS is locally a regular graph (Example 19.2), the orthogonal complement because f(M0)0\nabla f(M_0) \neq 0 — hence they are equal.

Example 19.8

For the sphere x2+y2+z2=R2x^2 + y^2 + z^2 = R^2: f=2(x,y,z)\nabla f = 2(x, y, z), so the tangent plane at M0M_0 is orthogonal to the radius OM0\vect{OM_0} — the classical fact that radius and tangent plane are perpendicular, with equation M0,M=R2\langle M_0, M\rangle = R^2.

Example 19.9 (Graph tangent plane)

For z=f(x,y)z = f(x, y) at (x0,y0)(x_0, y_0): applying Proposition 19.7 to F(x,y,z)=f(x,y)zF(x,y,z) = f(x,y) - z,

z=f(x0,y0)+fx(x0,y0)(xx0)+fy(x0,y0)(yy0),z = f(x_0, y_0) + f_x(x_0, y_0)(x - x_0) + f_y(x_0, y_0)(y - y_0) ,

the affine part of the first-order Taylor expansion — the tangent plane is the graph of the differential, as it must be.

Example 19.10 (The closest point of a surface)

Which point of the paraboloid z=x2+y2z = x^2 + y^2 is nearest to P=(0,0,1)P = (0, 0, 1)? Minimize the squared distance along the surface: with ρ2=x2+y2\rho^2 = x^2 + y^2,

g(ρ2)=ρ2+(ρ21)2,g(ρ2)=1+2(ρ21)=0    ρ2=12,g(\rho^2) = \rho^2 + (\rho^2 - 1)^2, \qquad g'(\rho^2) = 1 + 2(\rho^2 - 1) = 0 \iff \rho^2 = \tfrac12 ,

giving the circle of points at height z=12z = \frac12 and distance 12+14=32\sqrt{\tfrac12 + \tfrac14} = \frac{\sqrt3}2. The geometric signature of minimality: at such a point MM, the vector MP\vect{MP} must be normal to the surface — otherwise sliding along a drawn curve with velocity having a component toward PP would decrease the distance. Check: (zx2y2)=(2x,2y,1)\nabla(z - x^2 - y^2) = (-2x, -2y, 1) at M=(x,y,12)M = (x, y, \tfrac12), while MP=(x,y,12)=12(2x,2y,1)\vect{MP} = (-x, -y, \tfrac12) = \tfrac12(-2x, -2y, 1): parallel, as predicted. The first-order condition “foot of the perpendicular” is the same one that will drive extrema on level sets in Exercise 19.12.

Example 19.11 (Tangent planes of quadrics: the polarization rule)

Let S:xy+yz+zx=1S : xy + yz + zx = 1 and M0=(1,1,0)SM_0 = (1, 1, 0) \in S. Here f=(y+z, x+z, x+y)\nabla f = (y + z,\ x + z,\ x + y), so f(M0)=(1,1,2)\nabla f(M_0) = (1, 1, 2) and the tangent plane is

(x1)+(y1)+2z=0,i.e.x+y+2z=2.(x - 1) + (y - 1) + 2z = 0, \qquad\text{i.e.}\qquad x + y + 2z = 2 .

The same answer comes from the polarization rule that generalizes Example 19.8 and Exercise 19.2: in the quadric’s equation, replace x2x^2 by x0xx_0x, and each product xyxy by x0y+y0x2\frac{x_0y + y_0x}2 (and cyclically):

x0y+y0x2+y0z+z0y2+z0x+x0z2=1   M0=(1,1,0)   x+y2+z2+z2=1,\frac{x_0y + y_0x}2 + \frac{y_0z + z_0y}2 + \frac{z_0x + x_0z}2 = 1 \;\xrightarrow{\ M_0 = (1,1,0)\ }\; \frac{x + y}2 + \frac z2 + \frac z2 = 1 ,

which is x+y+2z=2x + y + 2z = 2 again. The rule works because \nabla of a quadratic form is the associated bilinear form evaluated against the base point — tangency to a quadric is polarization, one more face of Chapter 12.

19.3 The first fundamental form

Definition 19.12 (First fundamental form)

Let σ ⁣:UR3\sigma \colon U \to \R^3 be a regular C1\mathcal{C}^1 surface. Its first fundamental form at (u,v)(u,v) is the positive definite quadratic form on R2\R^2

I(h,k)=hσu+kσv2=Eh2+2Fhk+Gk2,I(h, k) = \norm{h\,\sigma_u + k\,\sigma_v}^2 = E\,h^2 + 2F\,hk + G\,k^2,

where

E=σu2,F=σu,σv,G=σv2.E = \norm{\sigma_u}^2, \qquad F = \langle \sigma_u, \sigma_v\rangle, \qquad G = \norm{\sigma_v}^2 .

Remark 19.13

II is the restriction of the ambient Euclidean scalar product to the tangent plane, read in the basis (σu,σv)(\sigma_u, \sigma_v): it is positive definite precisely because σu,σv\sigma_u, \sigma_v are independent (Chapter 12). Every metric quantity on the surface — lengths of drawn curves, angles between them, areas — is computed from E,F,GE, F, G alone. Two surfaces with the same E,F,GE, F, G in suitable parameters are isometric even if they sit differently in space: this is the starting point of intrinsic geometry.

Example 19.14 (Angles between coordinate curves)

The first fundamental form also measures angles: the coordinate curves uσ(u,v0)u \mapsto \sigma(u, v_0) and vσ(u0,v)v \mapsto \sigma(u_0, v) meet at the angle θ\theta with

cosθ=σu,σvσuσv=FEG:\cos\theta = \frac{\langle\sigma_u, \sigma_v\rangle}{\norm{\sigma_u}\,\norm{\sigma_v}} = \frac{F}{\sqrt{EG}} :

the single coefficient FF decides orthogonality of the parameter net. For the sphere chart and the helicoid, F=0F = 0: meridians cut parallels, and helices cut the horizontal rulings, at right angles — which is why their area integrands collapsed to EG\sqrt{EG}. For a graph chart, F=fxfyF = f_xf_y vanishes only where a partial derivative does: the coordinate net of a tilted graph is not orthogonal, even though the (x,y)(x, y)-net downstairs is. When computations on a surface look heavy, the first move is to seek a chart with F=0F = 0.

Example 19.15 (The saddle chart)

For the saddle z=xyz = xy with chart σ(u,v)=(u,v,uv)\sigma(u, v) = (u, v, uv):

σu=(1,0,v),σv=(0,1,u),E=1+v2,F=uv,G=1+u2,\sigma_u = (1, 0, v), \qquad \sigma_v = (0, 1, u), \qquad E = 1 + v^2, \quad F = uv, \quad G = 1 + u^2 ,

and EGF2=1+u2+v2>0EG - F^2 = 1 + u^2 + v^2 > 0: regular everywhere. The two coordinate curves through a point are straight lines of R3\R^3 (fix uu or fix vv: the rulings of the doubly ruled saddle), yet F0F \neq 0 off the axes: rulings through a generic point are not orthogonal. Both rulings lie in the tangent plane, which they span — so the tangent plane cuts the surface along two whole lines, the extreme opposite of the sphere, whose tangent planes touch at one point only. The sign of the “second-order contact” between a surface and its tangent planes is a curvature story, taken up in the Year 3 volume.

Proposition 19.16 (Length of a curve drawn on a surface)

If γ(t)=σ(u(t),v(t))\gamma(t) = \sigma(u(t), v(t)), t[a,b]t \in [a, b], is C1\mathcal{C}^1, then

L(γ)=abEu2+2Fuv+Gv2   ⁣dt,L(\gamma) = \int_a^b \sqrt{E\,u'^2 + 2F\,u'v' + G\,v'^2}\;\dd t ,

with E,F,GE, F, G evaluated at (u(t),v(t))(u(t), v(t)).

Proof. γ=uσu+vσv\gamma' = u'\sigma_u + v'\sigma_v by the chain rule, so γ2=I(u,v)=Eu2+2Fuv+Gv2\norm{\gamma'}^2 = I(u', v') = Eu'^2 + 2Fu'v' + Gv'^2; integrate γ\norm{\gamma'} (Definition 18.6).

Example 19.17 (Why airliners fly over the pole)

Two airports sit at latitude φ0\varphi_0 and opposite longitudes: A=σ(0,φ0)A = \sigma(0, \varphi_0) and B=σ(π,φ0)B = \sigma(\pi, \varphi_0) on the sphere of radius RR. Along the parallel (φφ0\varphi \equiv \varphi_0), the length is 0πRcosφ0 ⁣dθ=πRcosφ0\int_0^\pi R\cos\varphi_0\,\dd\theta = \pi R\cos\varphi_0. Along the route over the pole (up the meridian θ=0\theta = 0, down the meridian θ=π\theta = \pi), it is 2R(π2φ0)2R(\frac\pi2 - \varphi_0). At latitude φ0=π3\varphi_0 = \frac\pi3 (sixty degrees): parallel route πR/21.571R\pi R/2 \approx 1.571\,R, polar route πR/31.047R\pi R/3 \approx 1.047\,R — a third shorter. In fact πcosφ0π2φ0\pi\cos\varphi_0 \geq \pi - 2\varphi_0 on [0,π/2]\intcc0{\pi/2} (the function πcosφπ+2φ\pi\cos\varphi - \pi + 2\varphi vanishes at both ends and its derivative 2πsinφ2 - \pi\sin\varphi changes sign once, so it is first increasing then decreasing, hence nonnegative): the polar route never loses. The first fundamental form turned a navigation question into two one-line integrals; Exercise 19.6 pushes the idea to a genuine minimality proof for meridians.

Lemma 19.18 (Lagrange identity)

For all a,bR3a, b \in \R^3: ab2=a2b2a,b2\norm{a \wedge b}^2 = \norm a^2 \norm b^2 - \langle a, b\rangle^2. In particular

σuσv=EGF2.\norm{\sigma_u \wedge \sigma_v} = \sqrt{EG - F^2}.

Proof. Both sides are unchanged if we replace bb by its component b=ba,ba2ab_\perp = b - \frac{\langle a, b\rangle}{\norm a^2}a orthogonal to aa (for a0a \neq 0; the case a=0a = 0 is trivial): the left side because aa=0a \wedge a = 0, the right side by expanding b2=b2a,b2a2\norm {b_\perp}^2 = \norm b^2 - \frac{\langle a,b\rangle^2}{\norm a^2} and a,b=0\langle a, b_\perp\rangle = 0. So it suffices to prove the identity for orthogonal a,ba, b, where it reads ab=ab\norm{a \wedge b} = \norm a \norm b: true, since for orthogonal vectors the cross product has norm absinπ2\norm a\norm b\,\abs{\sin\frac\pi2}. The displayed formula is the case a=σua = \sigma_u, b=σvb = \sigma_v.

Remark 19.19

The Lagrange identity says EGF2=det(EFFG)EG - F^2 = \det\left(\begin{smallmatrix} E & F\\ F & G\end{smallmatrix}\right) is the Gram determinant of (σu,σv)(\sigma_u, \sigma_v): the squared area of the parallelogram they span. Regularity, positive definiteness of the first fundamental form, and positivity of the Gram determinant are three phrasings of one condition — which is why the area integrand below never vanishes on a regular chart.

Definition 19.20 (Area)

Let σ ⁣:UR3\sigma \colon U \to \R^3 be a regular injective C1\mathcal{C}^1 surface and KUK \subseteq U a compact domain on which double integrals make sense (Chapter 20). The area of the piece σ(K)\sigma(K) is

A=Kσuσv ⁣du ⁣dv=KEGF2   ⁣du ⁣dv.\mathcal{A} = \iint_K \norm{\sigma_u \wedge \sigma_v}\,\dd u\,\dd v = \iint_K \sqrt{EG - F^2}\;\dd u\,\dd v .

Remark 19.21 (Why this formula)

The rectangle [u,u+ ⁣du]×[v,v+ ⁣dv][u, u + \dd u] \times [v, v + \dd v] is mapped, to first order, onto the parallelogram spanned by σu ⁣du\sigma_u\,\dd u and σv ⁣dv\sigma_v\,\dd v, whose area is σuσv ⁣du ⁣dv\norm{\sigma_u \wedge \sigma_v}\,\dd u\,\dd v: the definition integrates the local area-distortion factor, exactly as arc length integrates the local speed. Consistency with change of parameters is Exercise 19.8; consistency with the change-of-variables formula for double integrals is discussed in Chapter 20.

Example 19.22 (Two different graphs, one area)

Over the unit disk, compare the bowl z=12(x2+y2)z = \frac12(x^2 + y^2) and the saddle z=xyz = xy. Their area integrands (Exercise 19.5) are

1+x2+y2and1+y2+x2:\sqrt{1 + x^2 + y^2} \qquad\text{and}\qquad \sqrt{1 + y^2 + x^2} :

identical. The two surfaces — one curving the same way in all directions, the other saddle-shaped — have exactly equal areas over every domain, 2π3(221)\frac{2\pi}3(2\sqrt2 - 1) over the unit disk. The area element only sees the length of the gradient, not the arrangement of the bending; telling the bowl from the saddle requires second-order data (the sign structure exhibited in Figure 19.1), which no amount of area measurement detects. First fundamental form: metric, blind to shape; the shape-seeing second form belongs to Year 3.

Example 19.23 (Area of the sphere)

For the spherical chart of Example 19.2:

σθ=R(sinθcosφ, cosθcosφ, 0),σφ=R(cosθsinφ, sinθsinφ, cosφ),\sigma_\theta = R(-\sin\theta\cos\varphi,\ \cos\theta\cos\varphi,\ 0), \qquad \sigma_\varphi = R(-\cos\theta\sin\varphi,\ -\sin\theta\sin\varphi,\ \cos\varphi),

so E=R2cos2φE = R^2\cos^2\varphi, F=0F = 0, G=R2G = R^2 and EGF2=R2cosφ\sqrt{EG - F^2} = R^2\cos\varphi. Hence

A=π/2π/2 ⁣ ⁣02πR2cosφ   ⁣dθ ⁣dφ=2πR2[sinφ]π/2π/2=4πR2.\mathcal{A} = \int_{-\pi/2}^{\pi/2}\!\!\int_0^{2\pi} R^2\cos\varphi\;\dd\theta\,\dd\varphi = 2\pi R^2\,\bigl[\sin\varphi\bigr]_{-\pi/2}^{\pi/2} = \boxed{4\pi R^2} .

Example 19.24 (The cone, checked against the school formula)

For the cone z=x2+y2z = \sqrt{x^2 + y^2} over the annulus aρba \leq \rho \leq b, the graph formula of Exercise 19.5 gives 1+fx2+fy2=21 + f_x^2 + f_y^2 = 2 (compute fx=x/ρf_x = x/\rho, fy=y/ρf_y = y/\rho), so

A=2π(b2a2).\mathcal A = \sqrt2\,\pi\,(b^2 - a^2) .

Consistency check with the slant-height formula πρ\pi\rho\ell of Example 19.26: the full cones of base radii bb and aa have lateral areas πbb2\pi b\cdot b\sqrt2 and πaa2\pi a\cdot a\sqrt2, whose difference is exactly 2π(b2a2)\sqrt2\pi(b^2 - a^2). Two charts, two formulas, one area — the invariance proved in Exercise 19.8, seen in the wild.

Remark 19.25 (Sanity checks for areas)

Three instant checks catch most errors in an area computation. Scaling: dilating a surface by λ\lambda multiplies E,F,GE, F, G by λ2\lambda^2 and the area by λ2\lambda^2 — an answer whose dependence on RR is not quadratic (like 4πR24\pi R^2) is wrong. Positivity of the element: EGF2\sqrt{EG - F^2} must be strictly positive on the chart’s interior; a vanishing value flags a chart degeneracy, to be excised as in the sphere’s poles. Symmetry: a computation over a symmetric piece must be consistent with summing its congruent parts — the hemisphere had better give 2πR22\pi R^2.

Example 19.26 (Surface of revolution)

Rotate the curve z(r(z),0,z)z \mapsto (r(z), 0, z), r>0r > 0 of class C1\mathcal{C}^1, around the zz-axis:

σ(θ,z)=(r(z)cosθ, r(z)sinθ, z).\sigma(\theta, z) = (r(z)\cos\theta,\ r(z)\sin\theta,\ z).

Then E=r(z)2E = r(z)^2, F=0F = 0, G=1+r(z)2G = 1 + r'(z)^2, so

A=ab ⁣ ⁣02πr(z)1+r(z)2   ⁣dθ ⁣dz=2πabr(z)1+r(z)2 ⁣dz,\mathcal{A} = \int_a^b\!\!\int_0^{2\pi} r(z)\sqrt{1 + r'(z)^2}\;\dd\theta\,\dd z = 2\pi\int_a^b r(z)\sqrt{1 + r'(z)^2}\,\dd z ,

the classical formula (circumference 2πr2\pi r times the slant length element). For the cone r(z)=kzr(z) = kz, z[0,h]z \in [0, h]: A=2πk1+k2h22=πρ\mathcal A = 2\pi k\sqrt{1 + k^2}\,\frac{h^2}{2} = \pi \rho \ell with ρ=kh\rho = kh the base radius and =h1+k2\ell = h\sqrt{1 + k^2} the slant height — the school formula, now derived rather than admitted.

Example 19.27 (The catenoid)

Rotate the catenary r(z)=coshzr(z) = \cosh z, z[1,1]z \in \intcc{-1}{1}, around its axis: the resulting catenoid has, by the revolution formula and 1+sinh2z=cosh2z1 + \sinh^2 z = \cosh^2 z,

A=2π11coshz1+sinh2z ⁣dz=2π11cosh2z ⁣dz=π[z+sinhzcoshz]11,\mathcal A = 2\pi\int_{-1}^1\cosh z\,\sqrt{1 + \sinh^2z}\, \dd z = 2\pi\int_{-1}^1\cosh^2z\,\dd z = \pi\bigl[z + \sinh z\cosh z\bigr]_{-1}^{1},

that is

A=2π+πsinh217.68.\mathcal A = 2\pi + \pi\sinh 2 \approx 17.68 .

The slant factor 1+r2\sqrt{1 + r'^2} merged with the radius into a perfect square — the same identity that made the catenary’s arc length elementary in the curves chapter. This is no accident of algebra: among all surfaces of revolution spanning the two boundary circles, the catenoid minimizes area (it is the shape of a soap film between two rings), and this variational property is precisely what singles out cosh\cosh; the Year 3 volume proves it with the calculus of variations.

The saddle z = x2 - y2 near the origin, with its coordinate curves (u-curves in blue, v-curves in green), the tangent plane at M_0 = (0,0,0) (dashed) and the unit normal n. The surface crosses its tangent plane — the two-dimensional analogue of an inflection.
Figure 19.1. The saddle z=x2y2z = x^2 - y^2 near the origin, with its coordinate curves (uu-curves in blue, vv-curves in green), the tangent plane at M0=(0,0,0)M_0 = (0,0,0) (dashed) and the unit normal nn. The surface crosses its tangent plane — the two-dimensional analogue of an inflection.

Remark 19.28 (Common pitfalls)

(i) Chart singularities are not surface singularities: the spherical chart degenerates at the poles (cosφ=0\cos\varphi = 0), but the sphere is perfectly smooth there — another chart (exchange the roles of the axes) is regular at the poles. Before declaring a point singular, try a second parametrization. (ii) Regularity of σ\sigma concerns the parametrization, not the image: σ(u,v)=(u3,v,0)\sigma(u, v) = (u^3, v, 0) is non-regular along u=0u = 0 although its image is a plane. (iii) The area formula requires σ\sigma injective on KK: a chart covering a piece twice counts it twice (θ\theta running over [0,4π]\intcc0{4\pi} doubles the sphere’s area). (iv) The unit normal is defined up to sign by the surface but is chosen by the chart (order of u,vu, v); statements involving orientation must fix that choice. (v) Finally, EGF2>0EG - F^2 > 0 is not an extra hypothesis: it is exactly regularity, by the Lagrange identity — if it vanishes somewhere, the problem is the chart, and no area or tangent-plane formula applies there.

Remark 19.29 (Perspectives within this volume)

Forward links from here. The area element EGF2 ⁣du ⁣dv\sqrt{EG - F^2}\,\dd u\,\dd v is a two-dimensional Jacobian in disguise, and Chapter 20 makes the analogy exact with the change-of-variables theorem — the surface integrals there are this chapter’s areas with an integrand on board. The first fundamental form is a field of positive quadratic forms, handled pointwise by the tools of Chapter 12, whose spectral theorem also powers this chapter’s weekend classification of quadrics. And the normal line drives extremum problems on constraint sets (Example 19.10), the geometric germ of the Lagrange multiplier method sketched with Theorem 15.11.

Four of the nine quadric surfaces classified in the weekend problem, sketched by their silhouettes and a level curve (red): the bounded ellipsoid, the doubly ruled one-sheet hyperboloid with its waist, the bowl of the elliptic paraboloid, and the saddle, whose two parabolic sections bend in opposite directions. Four of the nine quadric surfaces classified in the weekend problem, sketched by their silhouettes and a level curve (red): the bounded ellipsoid, the doubly ruled one-sheet hyperboloid with its waist, the bowl of the elliptic paraboloid, and the saddle, whose two parabolic sections bend in opposite directions. Four of the nine quadric surfaces classified in the weekend problem, sketched by their silhouettes and a level curve (red): the bounded ellipsoid, the doubly ruled one-sheet hyperboloid with its waist, the bowl of the elliptic paraboloid, and the saddle, whose two parabolic sections bend in opposite directions. Four of the nine quadric surfaces classified in the weekend problem, sketched by their silhouettes and a level curve (red): the bounded ellipsoid, the doubly ruled one-sheet hyperboloid with its waist, the bowl of the elliptic paraboloid, and the saddle, whose two parabolic sections bend in opposite directions.
Four of the nine quadric surfaces classified in the weekend problem, sketched by their silhouettes and a level curve (red): the bounded ellipsoid, the doubly ruled one-sheet hyperboloid with its waist, the bowl of the elliptic paraboloid, and the saddle, whose two parabolic sections bend in opposite directions.

Remark 19.30 (Where this is used)

The area element σuσv ⁣du ⁣dv\norm{\sigma_u\wedge\sigma_v}\,\dd u\,\dd v is the surface-integral measure of Chapter 20, where it meets Green’s formula; the first fundamental form is the prototype of a field of quadratic forms, studied pointwise with the tools of Chapter 12; and this chapter’s weekend problem classifies all quadric surfaces with the spectral theorem. The Year 3 volume returns to surfaces with differential forms and the divergence theorem, and intrinsic curvature — what E,F,GE, F, G know about bending — is the gateway to differential geometry proper.

19.4 Exercises

Exercise 19.1

Show that the tangent planes of the cone z=x2+y2z = \sqrt{x^2 + y^2} (minus its apex) all pass through the apex. (Parametrize by σ(θ,r)=(rcosθ,rsinθ,r)\sigma(\theta, r) = (r\cos\theta, r\sin\theta, r), r>0r > 0.)

Solution

Solution of Exercise 19.1.

With σ(θ,r)=(rcosθ, rsinθ, r)\sigma(\theta, r) = (r\cos\theta,\ r\sin\theta,\ r):

σθ=(rsinθ, rcosθ, 0),σr=(cosθ, sinθ, 1),\sigma_\theta = (-r\sin\theta,\ r\cos\theta,\ 0), \qquad \sigma_r = (\cos\theta,\ \sin\theta,\ 1),

independent for r>0r > 0. The tangent plane at M0=σ(θ0,r0)M_0 = \sigma(\theta_0, r_0) passes through M0M_0 with directions σθ,σr\sigma_\theta, \sigma_r. Now M0O=r0(cosθ0,sinθ0,1)=r0σr(θ0,r0)M_0 - O = r_0(\cos\theta_0, \sin\theta_0, 1) = r_0\,\sigma_r(\theta_0, r_0) is itself a tangent direction: the apex OO lies on the tangent plane. (This is the general behaviour of cones: they are ruled by lines through the apex, and a tangent plane contains the ruling line through the point of tangency.)

Exercise 19.2

Find the tangent plane of the ellipsoid x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1 at a point (x0,y0,z0)(x_0, y_0, z_0) of the surface.

Solution

Solution of Exercise 19.2.

Apply Proposition 19.7 to f(x,y,z)=x2a2+y2b2+z2c2f(x,y,z) = \frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2}: f(x0,y0,z0)=2(x0a2,y0b2,z0c2)0\nabla f(x_0,y_0,z_0) = 2\bigl(\frac{x_0}{a^2}, \frac{y_0}{b^2}, \frac{z_0}{c^2}\bigr) \neq 0 on the surface. The tangent plane is

x0a2(xx0)+y0b2(yy0)+z0c2(zz0)=0,i.e.x0xa2+y0yb2+z0zc2=1,\frac{x_0}{a^2}(x - x_0) + \frac{y_0}{b^2}(y - y_0) + \frac{z_0}{c^2}(z - z_0) = 0, \qquad\text{i.e.}\qquad \frac{x_0\,x}{a^2} + \frac{y_0\,y}{b^2} + \frac{z_0\,z}{c^2} = 1,

using that (x0,y0,z0)(x_0, y_0, z_0) satisfies the ellipsoid equation — the “split the squares” rule generalizing the sphere’s M0,M=R2\langle M_0, M \rangle = R^2.

Exercise 19.3

Compute E,F,GE, F, G for the helicoid σ(u,v)=(vcosu, vsinu, au)\sigma(u, v) = (v\cos u,\ v\sin u,\ au), a>0a > 0, and the area of the piece 0u2π0 \leq u \leq 2\pi, 0v10 \leq v \leq 1, as an integral (evaluate it using v2+a2 ⁣dv=12(vv2+a2+a2ln(v+v2+a2))+C\int\sqrt{v^2 + a^2}\,\dd v = \frac12\bigl(v\sqrt{v^2+a^2} + a^2\ln(v + \sqrt{v^2 + a^2})\bigr) + C).

Solution

Solution of Exercise 19.3.

σu=(vsinu, vcosu, a)\sigma_u = (-v\sin u,\ v\cos u,\ a) and σv=(cosu, sinu, 0)\sigma_v = (\cos u,\ \sin u,\ 0), so

E=v2+a2,F=0,G=1,EGF2=v2+a2>0E = v^2 + a^2, \qquad F = 0, \qquad G = 1, \qquad \sqrt{EG - F^2} = \sqrt{v^2 + a^2} > 0

(the helicoid is regular everywhere, including on its axis v=0v = 0). Area of the piece:

A=02π ⁣ ⁣01v2+a2   ⁣dv ⁣du=2π12[vv2+a2+a2ln(v+v2+a2)]01,\mathcal{A} = \int_0^{2\pi}\!\!\int_0^1 \sqrt{v^2 + a^2}\;\dd v\,\dd u = 2\pi\cdot\frac12\Bigl[v\sqrt{v^2 + a^2} + a^2\ln\bigl(v + \sqrt{v^2 + a^2}\bigr)\Bigr]_0^1 ,

i.e. A=π(1+a2+a2ln1+1+a2a)\mathcal{A} = \pi\Bigl(\sqrt{1 + a^2} + a^2\ln\frac{1 + \sqrt{1 + a^2}}{a}\Bigr).

Exercise 19.4 ★★

(Torus) Parametrize the torus obtained by rotating the circle of center (R,0,0)(R, 0, 0) and radius r<Rr < R in the xzxz-plane around the zz-axis:

σ(θ,ψ)=((R+rcosψ)cosθ, (R+rcosψ)sinθ, rsinψ).\sigma(\theta, \psi) = \bigl((R + r\cos\psi)\cos\theta,\ (R + r\cos\psi)\sin\theta,\ r\sin\psi\bigr).

Compute E,F,GE, F, G, check regularity, and show that the area is 4π2Rr4\pi^2 R r (Pappus: mean circumference 2πR2\pi R times circle length 2πr2\pi r).

Solution

Solution of Exercise 19.4.

Derivatives:

σθ=((R+rcosψ)sinθ, (R+rcosψ)cosθ, 0),σψ=(rsinψcosθ, rsinψsinθ, rcosψ).\sigma_\theta = \bigl(-(R + r\cos\psi)\sin\theta,\ (R + r\cos\psi)\cos\theta,\ 0\bigr), \qquad \sigma_\psi = \bigl(-r\sin\psi\cos\theta,\ -r\sin\psi\sin\theta,\ r\cos\psi\bigr).

Then

E=(R+rcosψ)2,F=rsinψcosψ(R+rcosψ)(sinθcosθsinθcosθ)=0,G=r2,E = (R + r\cos\psi)^2, \qquad F = r\sin\psi\cos\psi\,(R + r\cos\psi) \bigl(\sin\theta\cos\theta - \sin\theta\cos\theta\bigr) = 0, \qquad G = r^2 ,

so EGF2=r(R+rcosψ)r(Rr)>0\sqrt{EG - F^2} = r(R + r\cos\psi) \geq r(R - r) > 0: regular everywhere. Area:

A=02π ⁣ ⁣02πr(R+rcosψ) ⁣dθ ⁣dψ=2πr(2πR+r02πcosψ ⁣dψ)=4π2Rr,\mathcal{A} = \int_0^{2\pi}\!\!\int_0^{2\pi} r(R + r\cos\psi) \,\dd\theta\,\dd\psi = 2\pi r \Bigl(2\pi R + r\int_0^{2\pi}\cos\psi\,\dd\psi\Bigr) = 4\pi^2 R r ,

the cosψ\cos\psi term integrating to zero — Pappus’ theorem: area == (length of the rotated circle) ×\times (distance travelled by its center).

Exercise 19.5 ★★

Show that the area of the graph of fC1(K)f \in \mathcal{C}^1(K) is K1+fx2+fy2 ⁣dx ⁣dy\iint_K \sqrt{1 + f_x^2 + f_y^2}\,\dd x\,\dd y, and compute it for the paraboloid piece z=12(x2+y2)z = \frac12(x^2 + y^2) over the disk x2+y21x^2 + y^2 \leq 1 (polar coordinates, Chapter 20).

Solution

Solution of Exercise 19.5.

For σ(x,y)=(x,y,f(x,y))\sigma(x, y) = (x, y, f(x,y)): σx=(1,0,fx)\sigma_x = (1, 0, f_x), σy=(0,1,fy)\sigma_y = (0, 1, f_y), so E=1+fx2E = 1 + f_x^2, F=fxfyF = f_xf_y, G=1+fy2G = 1 + f_y^2 and

EGF2=(1+fx2)(1+fy2)fx2fy2=1+fx2+fy2,EG - F^2 = (1 + f_x^2)(1 + f_y^2) - f_x^2f_y^2 = 1 + f_x^2 + f_y^2 ,

giving the stated area formula. For f=12(x2+y2)f = \frac12(x^2 + y^2) on the unit disk: 1+fx2+fy2=1+x2+y21 + f_x^2 + f_y^2 = 1 + x^2 + y^2, and in polar coordinates (x=ρcosαx = \rho\cos\alpha, y=ρsinαy = \rho\sin\alpha, Jacobian ρ\rho, Chapter 20):

A=02π ⁣ ⁣011+ρ2  ρ ⁣dρ ⁣dα=2π[13(1+ρ2)3/2]01=2π3(221).\mathcal{A} = \int_0^{2\pi}\!\!\int_0^1 \sqrt{1 + \rho^2}\;\rho \,\dd\rho\,\dd\alpha = 2\pi\Bigl[\tfrac13(1 + \rho^2)^{3/2}\Bigr]_0^1 = \frac{2\pi}{3}\bigl(2\sqrt2 - 1\bigr).

Exercise 19.6 ★★

A drawn curve γ(t)=σ(u(t),v(t))\gamma(t) = \sigma(u(t), v(t)) on the sphere of radius RR (spherical chart) has u=θ(t)u = \theta(t), v=φ(t)v = \varphi(t). Write its length as an integral in θ,φ\theta, \varphi and prove that among curves joining two points of the same meridian θ=θ0\theta = \theta_0, the meridian arc is the shortest. (Bound the integrand below by RφR\abs{\varphi'}.)

Solution

Solution of Exercise 19.6.

From Example 19.23’s computation, E=R2cos2φE = R^2\cos^2\varphi, F=0F = 0, G=R2G = R^2, so by Proposition 19.16

L=abRcos2φ(t)θ(t)2+φ(t)2   ⁣dt.L = \int_a^b R\sqrt{\cos^2\varphi(t)\,\theta'(t)^2 + \varphi'(t)^2}\;\dd t .

Let the endpoints be (θ0,φ1)(\theta_0, \varphi_1) and (θ0,φ2)(\theta_0, \varphi_2), φ1<φ2\varphi_1 < \varphi_2. For any joining curve,

LabRφ(t) ⁣dtRabφ(t) ⁣dt=R(φ2φ1),L \geq \int_a^b R\,\abs{\varphi'(t)}\,\dd t \geq R\,\Bigl|\int_a^b \varphi'(t)\,\dd t\Bigr| = R\,(\varphi_2 - \varphi_1),

dropping the nonnegative cos2φθ2\cos^2\varphi\,\theta'^2 term and using the triangle inequality for integrals. The meridian arc θθ0\theta \equiv \theta_0, φ\varphi increasing from φ1\varphi_1 to φ2\varphi_2, has length exactly R(φ2φ1)R(\varphi_2 - \varphi_1): it is shortest. (Meridians are great circles; this is the first, elementary case of the fact that geodesics of the sphere are great circles.)

Exercise 19.7 ★★★

(Normal lines of a sphere) Let SS be a regular level surface {f=c}\{f = c\}, connected, all of whose normal lines pass through a fixed point Ω\Omega. Show that SS is contained in a sphere centered at Ω\Omega. (Show that MΩ2\norm{M - \Omega}^2 has zero derivative along every curve drawn on SS.)

Solution

Solution of Exercise 19.7.

Fix a curve γ\gamma drawn on SS and let g(t)=γ(t)Ω2g(t) = \norm{\gamma(t) - \Omega}^2. Then g(t)=2γ(t), γ(t)Ωg'(t) = 2\langle \gamma'(t),\ \gamma(t) - \Omega\rangle. The normal line at M=γ(t)M = \gamma(t) passes through Ω\Omega by hypothesis, so γ(t)Ω\gamma(t) - \Omega is a normal vector, orthogonal to the tangent plane, in particular to the velocity γ(t)\gamma'(t) (Proposition 19.5): g=0g' = 0, and gg is constant along every drawn curve.

Now the set Sc={MS:MΩ2=c}S_c = \{M \in S : \norm{M - \Omega}^2 = c\} is closed in SS; it is also open in SS: near any of its points, SS is a regular graph, so any nearby point of SS is joined to it by a drawn curve (a lifted segment), along which gg is constant. As SS is connected and ScS_c nonempty for the right cc, S=ScS = S_c \subseteq the sphere of center Ω\Omega and radius c\sqrt c (Chapter 4: connectedness argument).

Exercise 19.8 ★★★

(Area is geometric) Let Φ ⁣:UU\Phi \colon U' \to U be a C1\mathcal{C}^1 diffeomorphism between open sets of R2\R^2 and σ~=σΦ\tilde\sigma = \sigma \circ \Phi. Show that

σ~uσ~v=detJΦ(σuσv)Φ,\norm{\tilde\sigma_{u'} \wedge \tilde\sigma_{v'}} = \abs{\det J_\Phi}\, \norm{(\sigma_u \wedge \sigma_v)\circ\Phi} ,

and deduce, using the change-of-variables formula of Chapter 20, that the area of Definition 19.20 does not depend on the chosen regular parametrization.

Solution

Solution of Exercise 19.8.

Write Φ(u,v)=(u,v)\Phi(u', v') = (u, v). By the chain rule,

σ~u=uuσu+vuσv,σ~v=uvσu+vvσv,\tilde\sigma_{u'} = \frac{\partial u}{\partial u'}\sigma_u + \frac{\partial v}{\partial u'}\sigma_v, \qquad \tilde\sigma_{v'} = \frac{\partial u}{\partial v'}\sigma_u + \frac{\partial v}{\partial v'}\sigma_v ,

partials of σ\sigma evaluated at Φ(u,v)\Phi(u',v'). Expanding the cross product bilinearly and using σuσu=σvσv=0\sigma_u \wedge \sigma_u = \sigma_v \wedge \sigma_v = 0, σvσu=σuσv\sigma_v \wedge \sigma_u = -\sigma_u \wedge \sigma_v:

σ~uσ~v=(uuvvvuuv)σuσv=detJΦ(σuσv)Φ.\tilde\sigma_{u'} \wedge \tilde\sigma_{v'} = \Bigl(\frac{\partial u}{\partial u'} \frac{\partial v}{\partial v'} - \frac{\partial v}{\partial u'} \frac{\partial u}{\partial v'}\Bigr)\, \sigma_u \wedge \sigma_v = \det J_\Phi \cdot (\sigma_u \wedge \sigma_v)\circ\Phi .

Taking norms gives the identity. Then, by the change-of-variables formula (Chapter 20) applied to the map Φ\Phi on K=Φ1(K)K' = \Phi^{-1}(K):

Kσ~uσ~v ⁣du ⁣dv=KσuσvΦ  detJΦ ⁣du ⁣dv=Kσuσv ⁣du ⁣dv:\iint_{K'} \norm{\tilde\sigma_{u'} \wedge \tilde\sigma_{v'}} \,\dd u'\dd v' = \iint_{K'} \norm{\sigma_u \wedge \sigma_v}\circ\Phi\; \abs{\det J_\Phi}\,\dd u'\dd v' = \iint_K \norm{\sigma_u \wedge \sigma_v}\,\dd u\,\dd v :

the two parametrizations assign the same area to the same piece of surface.

Exercise 19.9

(Archimedes’ hat-box theorem) On the sphere of radius RR, the zone between the latitudes with z1zz2z_1 \leq z \leq z_2 (Rz1<z2R-R \leq z_1 < z_2 \leq R) has area 2πR(z2z1)2\pi R\,(z_2 - z_1): prove it with the spherical chart, and conclude that a zone’s area depends only on its height — slicing an orange into equal-thickness slices gives equal amounts of peel.

Solution

Solution of Exercise 19.9.

In the spherical chart, z=Rsinφz = R\sin\varphi, and the zone corresponds to φ1φφ2\varphi_1 \leq \varphi \leq \varphi_2 with zi=Rsinφiz_i = R\sin\varphi_i. With the area element R2cosφ ⁣dθ ⁣dφR^2\cos\varphi\,\dd\theta\,\dd\varphi (Example 19.23):

A=φ1φ2 ⁣ ⁣02πR2cosφ ⁣dθ ⁣dφ=2πR2(sinφ2sinφ1)=2πR(z2z1).\mathcal A = \int_{\varphi_1}^{\varphi_2}\!\!\int_0^{2\pi} R^2\cos\varphi\,\dd\theta\,\dd\varphi = 2\pi R^2(\sin\varphi_2 - \sin\varphi_1) = 2\pi R\,(z_2 - z_1) .

The result depends only on the height z2z1z_2 - z_1: slices of equal thickness carry equal areas, whether cut at the equator or at the pole — Archimedes’ hat-box theorem, and the reason the lateral area of the circumscribed cylinder (2πR2R=4πR22\pi R \cdot 2R = 4\pi R^2) equals the area of the sphere.

Exercise 19.10 ★★

Show that every normal line of a surface of revolution σ(θ,z)=(r(z)cosθ, r(z)sinθ, z)\sigma(\theta, z) = (r(z)\cos\theta,\ r(z)\sin\theta,\ z) (r>0r > 0 of class C1\mathcal C^1) meets the axis of revolution, and locate the intersection point.

Solution

Solution of Exercise 19.10.

σθ=(rsinθ, rcosθ, 0)\sigma_\theta = (-r\sin\theta,\ r\cos\theta,\ 0) and σz=(rcosθ, rsinθ, 1)\sigma_z = (r'\cos\theta,\ r'\sin\theta,\ 1), so

σθσz=(rcosθ, rsinθ, rr),\sigma_\theta \wedge \sigma_z = (r\cos\theta,\ r\sin\theta,\ -r\,r') ,

a normal vector at M=(rcosθ,rsinθ,z)M = (r\cos\theta, r\sin\theta, z). The normal line is

t(r(1+t)cosθ, r(1+t)sinθ, ztrr),t \mapsto \bigl(r(1 + t)\cos\theta,\ r(1 + t)\sin\theta,\ z - t\,r\,r'\bigr),

which at t=1t = -1 reaches (0, 0, z+r(z)r(z))(0,\ 0,\ z + r(z)\,r'(z)): every normal line meets the axis, at the height z+rrz + rr'. (This is the three-dimensional reason rotational symmetry survives in the normal field.)

Exercise 19.11 ★★

(Unrolling the cylinder) The chart σ(u,v)=(cosu, sinu, v)\sigma(u, v) = (\cos u,\ \sin u,\ v) of the unit cylinder has E=G=1E = G = 1, F=0F = 0: verify this, and explain why every drawn curve tσ(u(t),v(t))t \mapsto \sigma(u(t), v(t)) has the same length as the plane curve t(u(t),v(t))t \mapsto (u(t), v(t)). Deduce that the helix from (1,0,0)(1, 0, 0) to (1,0,2πc)(1, 0, 2\pi c) making one turn has length 2π1+c22\pi\sqrt{1 + c^2}, and that no drawn curve with the same endpoints and one full turn is shorter.

Solution

Solution of Exercise 19.11.

σu=(sinu,cosu,0)\sigma_u = (-\sin u, \cos u, 0), σv=(0,0,1)\sigma_v = (0, 0, 1): E=1E = 1, F=0F = 0, G=1G = 1. By Proposition 19.16 the length of a drawn curve is u2+v2 ⁣dt\int\sqrt{u'^2 + v'^2}\,\dd t — the length of its parameter shadow (u(t),v(t))(u(t), v(t)) in the plane: the chart is a local isometry (the unrolling of the cylinder). The helix t(cost,sint,ct)t \mapsto (\cos t, \sin t, ct), t[0,2π]t \in \intcc0{2\pi}, has shadow the segment from (0,0)(0,0) to (2π,2πc)(2\pi, 2\pi c), of length 2π1+c22\pi\sqrt{1 + c^2}. Any drawn curve from (1,0,0)(1,0,0) to (1,0,2πc)(1, 0, 2\pi c) making one full turn has a continuous shadow joining (0,0)(0, 0) to (2π,2πc)(2\pi, 2\pi c), of plane length \geq the straight segment; since lengths agree, the helix is shortest.

Exercise 19.12 ★★★

Let S={f=c}S = \{f = c\} be a compact regular level surface and M0SM_0 \in S a point at maximal distance from the origin. Show that f(M0)\nabla f(M_0) is collinear with OM0\vect{OM_0} — the normal at the farthest point is radial. Apply to the ellipsoid x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1 (a>b>c>0a > b > c > 0): find all points where the normal is radial, and identify the farthest ones.

Solution

Solution of Exercise 19.12.

The function g(M)=M2g(M) = \norm{M}^2 is continuous on the compact SS, so it attains its maximum at some M0M_0. For every curve γ\gamma drawn on SS with γ(0)=M0\gamma(0) = M_0, the function tγ(t)2t \mapsto \norm{\gamma(t)}^2 has a maximum at t=0t = 0, so its derivative 2γ(0),M02\langle\gamma'(0), M_0\rangle vanishes: M0M_0 is orthogonal to every tangent vector, i.e. normal to SS at M0M_0. As f(M0)0\nabla f(M_0) \neq 0 also directs the normal line (Proposition 19.7), f(M0)\nabla f(M_0) and OM0\vect{OM_0} are collinear. For the ellipsoid, radiality means

(x0a2,y0b2,z0c2)=μ(x0,y0,z0):\Bigl(\frac{x_0}{a^2}, \frac{y_0}{b^2}, \frac{z_0}{c^2}\Bigr) = \mu\,(x_0, y_0, z_0) :

each coordinate satisfies x0(1a2μ)=0x_0(\frac1{a^2} - \mu) = 0, etc.; since a2,b2,c2a^{-2}, b^{-2}, c^{-2} are distinct, at most one coordinate is nonzero, and the solutions on the surface are the six axis endpoints (±a,0,0)(\pm a, 0, 0), (0,±b,0)(0, \pm b, 0), (0,0,±c)(0, 0, \pm c). The farthest points are (±a,0,0)(\pm a, 0, 0), at distance a=max(a,b,c)a = \max(a,b,c).

19.5 Problem: the classification of quadrics of R3\R^3

Problem 19.1

Weekend problem — every quadric surface, sorted by the spectral theorem

A quadric is the zero set in R3\R^3 of a degree-two polynomial

q(X)=XT ⁣AX+2b,X+c,AS3(R), A0, bR3, cR.q(X) = X^{\mathsf T}\!AX + 2\,\langle b, X\rangle + c, \qquad A \in \mathcal S_3(\R),\ A \neq 0,\ b \in \R^3,\ c \in \R .

The surfaces of this chapter’s figures — spheres, ellipsoids, saddles, cones, cylinders — are all quadrics. This problem classifies them all: the spectral theorem (Theorem 12.13) straightens the quadratic part, affine translations (Chapter 17) absorb the linear part, and what remains is a short, complete list of normal forms.

Part I — The reduction machine.

  1. Let X=PY+tX = PY + t with PO(3)P \in O(3) and tR3t \in \R^3 (a rigid change of coordinates). Show that q(PY+t)=YT ⁣AY+2b,Y+cq(PY + t) = Y^{\mathsf T}\!A'Y + 2\langle b', Y\rangle + c' with

    A=PT ⁣AP,b=PT(At+b),c=q(t).A' = P^{\mathsf T}\!AP, \qquad b' = P^{\mathsf T}(At + b), \qquad c' = q(t) .

    Deduce that the spectrum of AA (hence its rank and signature) is a rigid invariant of the equation, and explain why the equation of a given quadric is only determined up to a nonzero scalar factor.

  2. Using the spectral theorem, show that after a rotation the equation becomes iλiyi2+2iβiyi+c=0\sum_i \lambda_i y_i^2 + 2\sum_i\beta_iy_i + c = 0 with λ1,λ2,λ3\lambda_1, \lambda_2, \lambda_3 the eigenvalues of AA.
  3. For every ii with λi0\lambda_i \neq 0, absorb βiyi\beta_iy_i by a translation (yiyiβi/λiy_i \mapsto y_i - \beta_i/\lambda_i). Write the reduced equation when rankA=r\operatorname{rank} A = r: irλizi2+2i>rβizi+c=0\sum_{i\leq r}\lambda_i z_i^2 + 2\sum_{i > r}\beta_iz_i + c'' = 0.
  4. A center of the quadric of equation q=0q = 0 is a point Ω\Omega with q(2ΩX)=q(X)q(2\Omega - X) = q(X) for all XX: the point reflection in Ω\Omega preserves the equation, hence the surface. Show that q(2ΩX)q(X)=4AΩ+b,X+4AΩ+b,Ωq(2\Omega - X) - q(X) = -4\langle A\Omega + b, X\rangle + 4\langle A\Omega + b, \Omega\rangle, and deduce: the centers are exactly the solutions of AΩ=bA\Omega = -b; they exist iff bimAb \in \operatorname{im}A, and the center is unique iff AA is invertible.

Part II — Central quadrics (rankA=3\operatorname{rank}A = 3). Here the reduced equation is λ1z12+λ2z22+λ3z32=δ\lambda_1z_1^2 + \lambda_2z_2^2 + \lambda_3z_3^2 = \delta.

  1. Multiplying by 1-1 if needed, assume at least two λi>0\lambda_i > 0. Enumerate the possibilities: signature (3,0)(3, 0) with δ>0\delta > 0, =0= 0, <0< 0, and signature (2,1)(2, 1) with δ>0\delta > 0, =0= 0, <0< 0; name the six resulting sets (ellipsoid, point, empty set, one-sheet hyperboloid, cone, two-sheet hyperboloid) and put each in its Euclidean normal form (x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1, etc.).
  2. Classify x2+y2+z2+4xy+4yz+4zx=1x^2 + y^2 + z^2 + 4xy + 4yz + 4zx = 1: show A=2JIA = 2J - I with JJ the all-ones matrix, compute the spectrum {5,1,1}\{5, -1, -1\}, and identify a two-sheet hyperboloid of revolution about the axis R(1,1,1)\R(1,1,1).
  3. (Rulings) For the one-sheet hyperboloid x2a2+y2b2z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} - \frac{z^2}{c^2} = 1, factor

    (xazc)(xa+zc)=(1yb)(1+yb)\Bigl(\frac xa - \frac zc\Bigr) \Bigl(\frac xa + \frac zc\Bigr) = \Bigl(1 - \frac yb\Bigr)\Bigl(1 + \frac yb\Bigr)

    and produce two one-parameter families of straight lines lying on the surface.

  4. Show that through every point of the one-sheet hyperboloid passes exactly one line of each family: the surface is doubly ruled.
  5. The asymptotic cone of the one-sheet hyperboloid is C:x2a2+y2b2z2c2=0C : \frac{x^2}{a^2} + \frac{y^2}{b^2} - \frac{z^2}{c^2} = 0. With ρ2=x2a2+y2b2\rho^2 = \frac{x^2}{a^2} + \frac{y^2}{b^2}, show that any point of the hyperboloid is at distance at most c(ρρ21)=cρ+ρ21c\bigl(\rho - \sqrt{\rho^2 - 1}\bigr) = \frac{c}{\rho + \sqrt{\rho^2 - 1}} from CC, so the surface hugs its cone at infinity. What are the sections of the hyperboloid by the planes x=±ax = \pm a?

Part III — Rank 22 and rank 11: paraboloids, cylinders, planes.

  1. Suppose rankA=2\operatorname{rank}A = 2, say λ1,λ20=λ3\lambda_1, \lambda_2 \neq 0 = \lambda_3. Starting from question 3, split into two cases according to β30\beta_3 \neq 0 (no center, by question 4) or β3=0\beta_3 = 0 (a line of centers), and reduce to

    λ1z12+λ2z22+2β3z3=0orλ1z12+λ2z22+c=0:\lambda_1z_1^2 + \lambda_2z_2^2 + 2\beta_3z_3 = 0 \qquad\text{or}\qquad \lambda_1z_1^2 + \lambda_2z_2^2 + c'' = 0 :

    elliptic/hyperbolic paraboloids in the first case, cylinders over central conics (or pairs of intersecting planes, a line, the empty set) in the second.

  2. Show that the saddle z=xyz = xy is a hyperbolic paraboloid: rotate by π/4\pi/4 in the xyxy-plane to reach z=12(u2v2)z = \tfrac12(u^2 - v^2), the surface of Figure 19.1 up to scale.
  3. Show that the saddle z=xyz = xy carries the two line families {x=x0, z=x0y}\{x = x_0,\ z = x_0y\} and {y=y0, z=xy0}\{y = y_0,\ z = xy_0\}, with exactly one line of each through every point: the second doubly ruled quadric.
  4. Classify x2+y22x+4y+3=0x^2 + y^2 - 2x + 4y + 3 = 0 in R3\R^3 (complete the squares; identify a right circular cylinder, and give its axis and radius).
  5. Now let rankA=1\operatorname{rank}A = 1, say λ10=λ2=λ3\lambda_1 \neq 0 = \lambda_2 = \lambda_3. Rotating within the kernel plane and translating, reduce to

    λ1z12+2βz2=0(β0)orλ1z12+c=0:\lambda_1z_1^2 + 2\beta z_2 = 0 \quad (\beta \neq 0) \qquad\text{or}\qquad \lambda_1z_1^2 + c'' = 0 :

    a parabolic cylinder, or a pair of parallel planes, a double plane, or the empty set. Classify (x+y)2=z(x + y)^2 = z completely (normal form, axis of translation invariance).

Part IV — The classification theorem.

  1. Assemble Parts I–III into a theorem: every quadric of R3\R^3 is mapped by a rigid motion onto exactly one normal form. List the seventeen affine types (count the empty variants and degenerate sets), and single out the nine quadric surfaces: ellipsoid, one- and two-sheet hyperboloids, cone, elliptic and hyperbolic paraboloids, elliptic, hyperbolic and parabolic cylinders.
  2. Write the classification algorithm: given (A,b,c)(A, b, c), which quantities do you compute, in which order, and which branch decides which type? Justify that each step is effective (eigenvalues of a symmetric 3×33\times3 matrix, rank, solvability of AΩ=bA\Omega = -b).
  3. Run the algorithm on x2+y2+z22xy2yz2zx=1x^2 + y^2 + z^2 - 2xy - 2yz - 2zx = 1: show A=2IJA = 2I - J has spectrum {2,2,1}\{2, 2, -1\} and conclude: a one-sheet hyperboloid of revolution about R(1,1,1)\R(1,1,1).
  4. Run it on x2+y2z22x+4y+2z+4=0x^2 + y^2 - z^2 - 2x + 4y + 2z + 4 = 0: find the center and identify the quadric.
  5. Run it on x2+4xy+y2=2zx^2 + 4xy + y^2 = 2z: diagonalize the xyxy-block (u=x+y2u = \frac{x+y}{\sqrt2}, v=xy2v = \frac{x-y}{\sqrt2}) and identify the quadric.
  6. Euclidean versus affine. Show that two central quadrics in normal form are rigidly equivalent iff they have the same coefficient lists (up to permutation and a common positive scalar on the equation), while affinely, only the signature data survives: every ellipsoid is an affine image of the round sphere. Which theorem guarantees that the signature cannot change along the way (Theorem 12.6)?

Part V — Dividends.

  1. Show that every section of a quadric by an affine plane is a conic (possibly degenerate) of that plane. Identify the sections of the saddle z=xyz = xy by the planes z=cz = c (c0c \neq 0 and c=0c = 0).
  2. Which quadric surfaces contain straight lines? Show that the ellipsoid, the two-sheet hyperboloid and the elliptic paraboloid contain none (restrict qq to a line and use the Cauchy–Schwarz inequality for the two-sheet case); that cone and cylinders are ruled by one family; and conclude that the doubly ruled quadric surfaces are exactly the one-sheet hyperboloid and the hyperbolic paraboloid.
  3. When only the affine type is wanted, Gauss’s reduction (Theorem 12.5) is cheaper than diagonalizing. Redo question 17 with Gauss’s algorithm and check the signature (2,1)(2, 1); what Euclidean information does Gauss lose?
  4. All eigenvalues of a symmetric matrix are real; show that consequently the signs of the eigenvalues of AA can be read from the characteristic polynomial by Descartes’ rule of signs, and verify it on question 6: χA(λ)=λ33λ29λ5\chi_A(\lambda) = \lambda^3 - 3\lambda^2 - 9\lambda - 5 has exactly one sign change, hence signature (1,2)(1, 2).
  5. Synthesis. Summarize the algorithm in a few lines; state the exact role played by (i) the spectral theorem, (ii) the center equation AΩ=bA\Omega = -b, (iii) Sylvester’s inertia theorem, (iv) Gauss’s reduction. What does the same machine yield in R2\R^2, and what changes in Rn\R^n?
Solution

Solution of Problem 19.1.

1. Expanding, and using the symmetry of AA (tT ⁣APY=(At)TPYt^{\mathsf T}\!APY = (At)^{\mathsf T}PY):

q(PY+t)=YTPT ⁣APY+2(At+b)TPY+(tT ⁣At+2bTt+c),q(PY + t) = Y^{\mathsf T}P^{\mathsf T}\!APY + 2\,(At + b)^{\mathsf T}PY + \bigl(t^{\mathsf T}\!At + 2b^{\mathsf T}t + c\bigr),

which is the displayed triple. A=PT ⁣AP=P1APA' = P^{\mathsf T}\!AP = P^{-1}AP is similar to AA: same characteristic polynomial, spectrum, rank, signature. Finally {q=0}={sq=0}\{q = 0\} = \{sq = 0\} for s0s \neq 0, so only the equation up to a scalar is attached to the set; scaling by ss multiplies all eigenvalues by ss.

2. The spectral theorem provides PO(3)P \in O(3) with PT ⁣AP=diag(λ1,λ2,λ3)P^{\mathsf T}\!AP = \operatorname{diag}(\lambda_1, \lambda_2, \lambda_3); question 1 with t=0t = 0 turns the equation into λiyi2+2βiyi+c=0\sum\lambda_iy_i^2 + 2\sum\beta_iy_i + c = 0, where β=PTb\beta = P^{\mathsf T}b.

3. For λi0\lambda_i \neq 0: λiyi2+2βiyi=λi(yi+βiλi)2βi2λi\lambda_iy_i^2 + 2\beta_iy_i = \lambda_i\bigl(y_i + \frac{\beta_i}{\lambda_i}\bigr)^2 - \frac{\beta_i^2}{\lambda_i}; the translation zi=yi+βi/λiz_i = y_i + \beta_i/\lambda_i (and zi=yiz_i = y_i for i>ri > r) gives

irλizi2+2i>rβizi+c=0,c=cirβi2λi.\sum_{i \leq r}\lambda_iz_i^2 + 2\sum_{i > r}\beta_iz_i + c'' = 0, \qquad c'' = c - \sum_{i\leq r}\frac{\beta_i^2}{\lambda_i}.

4. q(2ΩX)=(2ΩX)TA(2ΩX)+2bT(2ΩX)+cq(2\Omega - X) = (2\Omega - X)^{\mathsf T} A(2\Omega - X) + 2b^{\mathsf T}(2\Omega - X) + c; expanding and subtracting q(X)q(X), the quadratic terms cancel and

q(2ΩX)q(X)=4AΩ+b, X+4AΩ+b, Ω.q(2\Omega - X) - q(X) = -4\,\langle A\Omega + b,\ X\rangle + 4\,\langle A\Omega + b,\ \Omega\rangle .

If AΩ+b=0A\Omega + b = 0 this vanishes identically: the point reflection preserves qq, hence the quadric. Conversely, “q(2ΩX)=q(X)q(2\Omega - X) = q(X) for all XX” says that the affine function above vanishes on all of R3\R^3, which forces its linear part AΩ+bA\Omega + b to be zero. So centers == solutions of AΩ=bA\Omega = -b: a nonempty set iff bimAb \in \operatorname{im}A (an affine subspace directed by kerA\ker A), and a single point iff AA is invertible.

5. Signature (3,0)(3,0) (all λi>0\lambda_i > 0): δ>0\delta > 0 gives x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1 with a=δ/λ1a = \sqrt{\delta/\lambda_1}, etc. — an ellipsoid; δ=0\delta = 0: the single point OO; δ<0\delta < 0: empty. Signature (2,1)(2,1) (λ1,λ2>0>λ3\lambda_1, \lambda_2 > 0 > \lambda_3): δ>0\delta > 0: x2a2+y2b2z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} - \frac{z^2}{c^2} = 1, the one-sheet hyperboloid; δ=0\delta = 0: the cone x2a2+y2b2=z2c2\frac{x^2}{a^2} + \frac{y^2}{b^2} = \frac{z^2}{c^2}; δ<0\delta < 0: z2c2x2a2y2b2=1\frac{z^2}{c^2} - \frac{x^2}{a^2} - \frac{y^2}{b^2} = 1, the two-sheet hyperboloid (zc\abs z \geq c: two components).

6. The quadratic part has matrix AA with diagonal 11 and off-diagonal 22: A=2JIA = 2J - I. Since JJ has spectrum {3,0,0}\{3, 0, 0\} (eigenvector (1,1,1)(1,1,1) for 33), AA has spectrum {5,1,1}\{5, -1, -1\}, the eigenvalue 55 carried by R(1,1,1)\R(1,1,1). In the rotated coordinates: 5u2v2w2=15u^2 - v^2 - w^2 = 1, i.e. u21/5v2w2=1\frac{u^2}{1/5} - v^2 - w^2 = 1: a two-sheet hyperboloid, of revolution (equal eigenvalues 1-1) about the axis R(1,1,1)\R(1,1,1).

7. The surface is (xazc)(xa+zc)=(1yb)(1+yb)\bigl(\frac xa - \frac zc\bigr)\bigl(\frac xa + \frac zc\bigr) = \bigl(1 - \frac yb\bigr)\bigl(1 + \frac yb\bigr). For (λ:μ)(0:0)(\lambda : \mu) \neq (0:0) define the line

Dλ:μ:λ(xazc)=μ(1yb),μ(xa+zc)=λ(1+yb)D_{\lambda:\mu} :\quad \lambda\Bigl(\frac xa - \frac zc\Bigr) = \mu\Bigl(1 - \frac yb\Bigr), \qquad \mu\Bigl(\frac xa + \frac zc\Bigr) = \lambda\Bigl(1 + \frac yb\Bigr)

(two independent affine equations: a line). Multiplying the two equations shows every point of Dλ:μD_{\lambda:\mu} lies on the surface when λμ0\lambda\mu \neq 0; the cases λ=0\lambda = 0 or μ=0\mu = 0 are checked directly (e.g. λ=0\lambda = 0: y=by = b, xa=zc\frac xa = -\frac zc, which satisfies the equation). The second family Dλ:μD'_{\lambda:\mu} swaps the two right-hand factors.

8. Fix MM on the surface. The conditions for MDλ:μM \in D_{\lambda:\mu} form a 2×22\times2 homogeneous linear system in (λ,μ)(\lambda, \mu) whose determinant is

(x2a2z2c2)(1y2b2)=0\Bigl(\frac{x^2}{a^2} - \frac{z^2}{c^2}\Bigr) - \Bigl(1 - \frac{y^2}{b^2}\Bigr) = 0

precisely because MM lies on the quadric: a nontrivial solution (λ:μ)(\lambda : \mu) exists. The coefficient matrix is never zero (that would force 1yb=1+yb=01 - \frac yb = 1 + \frac yb = 0), so its rank is 11 and the solution is unique up to scale: exactly one line of the family passes through MM. The same holds for the second family, and the two lines are distinct (at (a,0,0)(a, 0, 0) they are {x=a, zc=yb}\{x = a,\ \frac zc = \frac yb\} and {x=a, zc=yb}\{x = a,\ \frac zc = -\frac yb\}): the one-sheet hyperboloid is doubly ruled.

9. Let M=(x,y,z)M = (x, y, z) on the hyperboloid, ρ2=x2a2+y2b2=1+z2c21\rho^2 = \frac{x^2}{a^2} + \frac{y^2}{b^2} = 1 + \frac{z^2}{c^2} \geq 1. The point N=(x, y, εcρ)N = (x,\ y,\ \varepsilon c\rho) with ε\varepsilon the sign of zz satisfies x2a2+y2b2(cρ)2c2=0\frac{x^2}{a^2} + \frac{y^2}{b^2} - \frac{(c\rho)^2}{c^2} = 0: NCN \in C, and

d(M,C)zεcρ=c(ρρ21)=cρ+ρ21.d(M, C) \leq \abs{z - \varepsilon c\rho} = c\bigl(\rho - \sqrt{\rho^2 - 1}\bigr) = \frac{c}{\rho + \sqrt{\rho^2 - 1}} .

If M\norm M \to \infty then ρ\rho \to \infty (all three coordinates are bounded by multiples of ρ\rho), so d(M,C)0d(M, C) \to 0. The section x=ax = a: y2b2z2c2=0\frac{y^2}{b^2} - \frac{z^2}{c^2} = 0, the pair of crossing lines of question 8 — and likewise at x=ax = -a.

10. With λ3=0\lambda_3 = 0, question 3 leaves λ1z12+λ2z22+2β3z3+c=0\lambda_1z_1^2 + \lambda_2z_2^2 + 2\beta_3z_3 + c'' = 0. In the eigenbasis, imA=Vect(e1,e2)\operatorname{im}A = \operatorname{Vect}(e_1, e_2), so by question 4 centers exist iff β3=0\beta_3 = 0. If β30\beta_3 \neq 0: the translation z3z3c/(2β3)z_3 \mapsto z_3 - c''/(2\beta_3) removes the constant, leaving λ1z12+λ2z22+2β3z3=0\lambda_1z_1^2 + \lambda_2z_2^2 + 2\beta_3z_3 = 0, i.e. z3=px2+qy2z_3 = px^2 + qy^2 after renaming: an elliptic paraboloid if λ1λ2>0\lambda_1\lambda_2 > 0, a hyperbolic paraboloid if λ1λ2<0\lambda_1\lambda_2 < 0 — and indeed no center. If β3=0\beta_3 = 0: the equation λ1z12+λ2z22+c=0\lambda_1z_1^2 + \lambda_2z_2^2 + c'' = 0 does not involve z3z_3: the quadric is a cylinder over the corresponding plane conic — elliptic cylinder, line, or empty set when λ1λ2>0\lambda_1\lambda_2 > 0; hyperbolic cylinder or pair of intersecting planes when λ1λ2<0\lambda_1\lambda_2 < 0 — with a whole line of centers {(z1,z2)}×R\{(z_1^*, z_2^*)\} \times \R.

11. xyz=0xy - z = 0. Substituting x=u+v2x = \frac{u + v}{\sqrt2}, y=uv2y = \frac{u - v}{\sqrt2} (rotation by π/4\pi/4): xy=u2v22xy = \frac{u^2 - v^2}2, so the equation becomes z=12(u2v2)z = \frac12(u^2 - v^2): a hyperbolic paraboloid — the saddle of the figure, up to the factor 12\frac12.

12. The line {x=x0, z=x0y}\{x = x_0,\ z = x_0y\} (parametrized by yy) clearly lies on z=xyz = xy, as does {y=y0, z=xy0}\{y = y_0,\ z = xy_0\}; through (x0,y0,x0y0)(x_0, y_0, x_0y_0) pass the two of them. Uniqueness: if t(x0+tv1,y0+tv2,z0+tv3)t \mapsto (x_0 + tv_1, y_0 + tv_2, z_0 + tv_3) stays on the surface, the coefficient of t2t^2 in (x0+tv1)(y0+tv2)z0tv3(x_0 + tv_1)(y_0 + tv_2) - z_0 - tv_3 gives v1v2=0v_1v_2 = 0, so v1=0v_1 = 0 or v2=0v_2 = 0, landing in one of the two families: one line of each through each point — the second doubly ruled quadric.

13. Completing squares: (x1)2+(y+2)2=2(x - 1)^2 + (y + 2)^2 = 2, with no condition on zz: a right circular cylinder of radius 2\sqrt2 and axis the vertical line {(1,2,z):zR}\{(1, -2, z) : z \in \R\} — a line of centers, as question 10 predicts.

14. With λ2=λ3=0\lambda_2 = \lambda_3 = 0 the reduced equation is λ1z12+2β2z2+2β3z3+c=0\lambda_1z_1^2 + 2\beta_2z_2 + 2\beta_3z_3 + c'' = 0. A rotation of the kernel plane (z2,z3)(z_2, z_3) aligns the linear form: 2β2z2+2β3z3=2βw2\beta_2z_2 + 2\beta_3z_3 = 2\beta w with β=β22+β32\beta = \sqrt{\beta_2^2 + \beta_3^2}. If β0\beta \neq 0, translate ww to absorb cc'': λ1z12+2βw=0\lambda_1z_1^2 + 2\beta w = 0, a parabolic cylinder; if β=0\beta = 0: λ1z12=c\lambda_1z_1^2 = -c'' gives two parallel planes (cλ1<0c'' \lambda_1 < 0), a double plane (c=0c'' = 0), or the empty set. For (x+y)2=z(x + y)^2 = z: with u=x+y2u = \frac{x + y}{\sqrt2} the equation reads z=2u2z = 2u^2: a parabolic cylinder, invariant under translations along (1,1,0)(1, -1, 0).

15. Every quadric is carried by a rotation plus translations onto one of: (rank 3) ellipsoid, point, empty set, one-sheet hyperboloid, cone, two-sheet hyperboloid; (rank 2) elliptic paraboloid, hyperbolic paraboloid, elliptic cylinder, line, empty set, hyperbolic cylinder, pair of intersecting planes; (rank 1) parabolic cylinder, pair of parallel planes, double plane, empty set. Identifying the three empty variants as distinct affine types of equations, the count is seventeen; among them nine are honest surfaces: ellipsoid, the two hyperboloids, the cone, the two paraboloids, and the three cylinders.

16. Algorithm. (i) Read off (A,b,c)(A, b, c); compute the characteristic polynomial of AA, its eigenvalues (real, by the spectral theorem) and r=rankAr = \operatorname{rank}A. (ii) Solve AΩ=bA\Omega = -b (Gaussian elimination): solvable or not — centers or not. (iii) If solvable, translate to a center: the equation becomes λizi2+c=0\sum\lambda_iz_i^2 + c'' = 0 with c=c+b,Ωc'' = c + \langle b, \Omega\rangle; sort by rr, the signature, and the sign of cc'' using questions 5, 10, 14. (iv) If not solvable (r2r \leq 2), rotate and reduce as in questions 10 and 14: paraboloid (r=2r = 2) or parabolic cylinder (r=1r = 1), elliptic/hyperbolic according to the sign of λ1λ2\lambda_1\lambda_2. Each step is a finite computation: roots of a cubic with real roots, ranks, linear systems.

17. AA has diagonal 11, off-diagonal 1-1: A=2IJA = 2I - J, spectrum {23, 2, 2}={1,2,2}\{2 - 3,\ 2,\ 2\} = \{-1, 2, 2\} with 1-1 on R(1,1,1)\R(1,1,1). Signature (2,1)(2,1), b=0b = 0, right side δ=1>0\delta = 1 > 0: 2u2+2v2w2=12u^2 + 2v^2 - w^2 = 1, a one-sheet hyperboloid of revolution about the axis R(1,1,1)\R(1,1,1).

18. Complete squares: (x1)2+(y+2)2(z1)2+(14+1+4)=0(x-1)^2 + (y+2)^2 - (z-1)^2 + (-1 - 4 + 1 + 4) = 0, i.e.

(x1)2+(y+2)2=(z1)2:(x-1)^2 + (y+2)^2 = (z-1)^2 :

the constant vanished — a right circular cone with vertex (and unique center) (1,2,1)(1, -2, 1) and axis parallel to OzOz.

19. The quadratic part x2+4xy+y2x^2 + 4xy + y^2 has matrix (1221)\left(\begin{smallmatrix}1 & 2\\ 2 & 1\end{smallmatrix}\right) (in the xyxy-plane), eigenvalues 33 (on (1,1)(1,1)) and 1-1 (on (1,1)(1,-1)): with u=x+y2u = \frac{x+y}{\sqrt2}, v=xy2v = \frac{x-y}{\sqrt2} it equals 3u2v23u^2 - v^2, and the quadric is

z=32u212v2:z = \tfrac32u^2 - \tfrac12v^2 :

a hyperbolic paraboloid (AA has rank 22 and bb has a component along kerA=Rez\ker A = \R e_z: no center).

20. A rigid motion transforms the equation’s data by APT ⁣APA \mapsto P^{\mathsf T}\!AP (same eigenvalues) and the normal forms have no residual freedom except permuting coordinates and multiplying the whole equation by a scalar (>0> 0 to preserve the writing): two central normal forms coincide up to isometry iff the coefficient lists agree up to permutation and common positive factor — for the ellipsoid, iff the semiaxes (a,b,c)(a, b, c) agree. Affinely, one may also scale each coordinate separately (ziziλiz_i \mapsto z_i\sqrt{\abs {\lambda_i}}), which erases the eigenvalues and leaves only their signs: every ellipsoid becomes u2+v2+w2=1u^2 + v^2 + w^2 = 1, the sphere. Sylvester’s inertia theorem (Theorem 12.6) guarantees the signature survives any invertible linear change: the affine types of question 15 are genuinely distinct.

21. Parametrize the plane affinely: M=P+su+tvM = P + su + tv. Then q(P+su+tv)q(P + su + tv) is a polynomial of degree 2\leq 2 in (s,t)(s, t) (expand the quadratic form bilinearly), so the section {q=0}\{q = 0\} is a conic of the plane, possibly degenerate. For z=xyz = xy and the plane z=cz = c: xy=cxy = c, a hyperbola for c0c \neq 0, and for c=0c = 0 the two coordinate lines — the pair of rulings through the origin.

22. Ellipsoid: bounded, contains no line. Two-sheet hyperboloid z2c2x2a2y2b2=1\frac{z^2}{c^2} - \frac{x^2}{a^2} - \frac{y^2}{b^2} = 1: restrict to p+tvp + tv; the t2t^2 coefficient v32c2v12a2v22b2\frac{v_3^2}{c^2} - \frac{v_1^2}{a^2} - \frac{v_2^2}{b^2} must vanish, so v30v_3 \neq 0 (else v=0v = 0); the tt coefficient gives p3v3c2=p1v1a2+p2v2b2\frac{p_3v_3}{c^2} = \frac{p_1v_1}{a^2} + \frac{p_2v_2}{b^2}, and Cauchy–Schwarz yields

p32c2=c2v32(p1v1a2+p2v2b2)2c2v32(p12a2+p22b2)v32c2=p12a2+p22b2,\frac{p_3^2}{c^2} = \frac{c^2}{v_3^2}\Bigl(\frac{p_1v_1}{a^2} + \frac{p_2v_2}{b^2}\Bigr)^2 \leq \frac{c^2}{v_3^2}\Bigl(\frac{p_1^2}{a^2} + \frac{p_2^2}{b^2}\Bigr)\frac{v_3^2}{c^2} = \frac{p_1^2}{a^2} + \frac{p_2^2}{b^2},

so the constant term is 01\leq 0 \neq 1: no line. Elliptic paraboloid z=x2a2+y2b2z = \frac{x^2}{a^2} + \frac{y^2}{b^2}: the t2t^2 coefficient forces v1=v2=0v_1 = v_2 = 0, then the equation is linear nonconstant in tt: no line. Cone x2+y2=z2x^2 + y^2 = z^2: a line on it satisfies q(p)=q(v)=B(p,v)=0q(p) = q(v) = B(p, v) = 0 for the Lorentz form; equality in the plane Cauchy–Schwarz p1v1+p2v2=p3v3=(p12+p22)(v12+v22)\abs{p_1v_1 + p_2v_2} = \abs{p_3v_3} = \sqrt{(p_1^2 + p_2^2)(v_1^2 + v_2^2)} forces (p1,p2)(v1,v2)(p_1, p_2) \parallel (v_1, v_2) and then p=kvp = kv: all lines pass through the vertex — one family. Cylinders: for the elliptic and parabolic cylinders the t2t^2 coefficient forces v1=v2=0v_1 = v_2 = 0 (rulings only); for the hyperbolic cylinder x2a2y2b2=1\frac{x^2}{a^2} - \frac{y^2}{b^2} = 1, v1a=±v2b\frac{v_1}a = \pm \frac{v_2}b with v20v_2 \neq 0 leads via the tt coefficient to p12a2=p22b2\frac{p_1^2}{a^2} = \frac{p_2^2}{b^2}, contradicting the constant term 11: again only the vertical rulings. So the doubly ruled quadric surfaces are exactly the one-sheet hyperboloid and the hyperbolic paraboloid.

23. Gauss: x22xy2zx=(xyz)2y2z22yzx^2 - 2xy - 2zx = (x - y - z)^2 - y^2 - z^2 - 2yz, so

q=(xyz)24yz=(xyz)2+(yz)2(y+z)2:q = (x - y - z)^2 - 4yz = (x - y - z)^2 + (y - z)^2 - (y + z)^2 :

three independent squares with signs (+,+,)(+, +, -) — signature (2,1)(2, 1), matching question 17, with no eigenvalue computation. Gauss loses the metric data: the new coordinates are not orthonormal, so the eigenvalues (the shape of the hyperboloid, its axes and their lengths) are gone; only the affine type remains.

24. Let pp, nn, zz be the numbers of positive, negative and zero eigenvalues, p+n+z=3p + n + z = 3. Descartes’ rule bounds pp by the number VV of sign changes of χA\chi_A, and nn by the number VV' of sign changes of χA(λ)\chi_A(-\lambda); moreover each pair of consecutive nonzero coefficients produces a change in exactly one of the two polynomials, so V+V3zV + V' \leq 3 - z (zero roots are visible as vanishing trailing coefficients). Then p+n=3zV+Vp+np + n = 3 - z \geq V + V' \geq p + n: equality, so p=Vp = V exactly — the signs of the eigenvalues can be read off. For χA(λ)=λ33λ29λ5\chi_A(\lambda) = \lambda^3 - 3\lambda^2 - 9\lambda - 5: signs +,,,+,-,-,- give V=1V = 1, and χA(λ)=λ33λ2+9λ5\chi_A(-\lambda) = -\lambda^3 - 3\lambda^2 + 9\lambda - 5 has signs ,,+,-,-,+,-: V=2V' = 2. Signature (1,2)(1, 2) — consistent with the exact factorization χA=(λ5)(λ+1)2\chi_A = (\lambda - 5)(\lambda + 1)^2 of question 6.

25. Algorithm: diagonalize the quadratic part orthonormally (spectral theorem: this is the only analytically deep step, and it is what makes the classification Euclidean); solve AΩ=bA\Omega = -b to decide central versus parabolic types and to translate away the linear part where possible (affine geometry); read the type from rank, signature and the constant (Sylvester guarantees these are invariants); when only the affine type matters, Gauss’s reduction replaces the spectral theorem at the cost of the metric information. In R2\R^2 the same machine classifies conics: ellipse, hyperbola, parabola, plus pairs of lines, a line, a point, and empty sets. In Rn\R^n nothing changes but bookkeeping: the types are indexed by the signature of AA, the position of bb relative to imA\operatorname{im}A, and one constant — with the (n+2)(n{+}2)-dimensional bordered matrix of (A,b,c)(A, b, c) providing a compact invariant.