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Solutions to the final exam of m408m course, covering topics such as conic sections, parametrized curves, lines and planes in 3d space, position, velocity and acceleration, surfaces, max-min, and iterated integrals. It includes detailed calculations and answers to various problems.
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M408M Final Exam Solutions, December 14, 2006
r = 10 1 + sin(θ)
a) Is this a circle, ellipse, parabola or hyperbola? It is a parabola. If you don’t see this from the polar form of the equation, see part (c). b) Find the (Cartesian) coordinates of the point closest to the origin. “Closest the the origin” means the smallest value of r, which means the biggest denominator, which means θ = π/2. In polar coordinates our point is (5, π/2), while in Cartesian coordinates the point is (0,5). c) Express the equation of the curve in Cartesian coordinates. Multiplying both sides by 1 + sin(θ) gives 10 = r + r sin(θ) = r + y, so r = 10 − y, so r^2 = 100 − 20 y + y^2. But r^2 = x^2 + y^2 , so x^2 = 100 − 20 y, or y = 5 − (x^2 /20).
2 x + y − 3 z = 3. c) Find the equation of the line through (1,1,0) that is perpendicular to the plane you found in part (b). x− 1 − 2 =^ y− 1 − 1 =^ z/3.
Extra Credit) Find the average velocity between times t = 0 and t = π. This is (~r(π) − ~r(0))/π =< (^) π^6 , 4 , 12 >.
c) Evaluate the resulting iterated integral.
= ∫ (^1) 0 yey
(^2) dy = 1 2 e y^2 ∣∣ ∣ 1 0 =^
e− 1
Consider the dome-shaped region above the plane z = 0 and below the parabaloid z = 1 − x^2 − y^2. Call this region R. a) Write
∫ ∫ ∫ R e−z^ dV^ as an iterated integral.^ You are free to do this in Cartesian, cylindrical or spherical coordinates, or something even stranger, and you may integrate over your variables in whatever order you wish. How- ever, you MUST make clear your order of integration and limits of inte- gration, and express the integrand (and if necessary, the Jacobian) in the coordinates you have chosen.
There are many possible answers. My favorite is ∫ (^1) r=
∫ (^2) π θ=
∫ (^1) −r 2 z=0 e−z^ rdzdθdr. b) Evaluate the integral. [N.B. For part (a), all coordinate systems are equally good and will get full credit, as long as you set up the integral correctly. However, part (b) will be a lot easier if you make a sensible choice in part (a).] Integrating over z gives ∫ (^1) 0
∫ (^2) π 0 r(1^ −^ er
(^2) − (^1) )dθ dr = 2π ∫^1 0 r(1^ −^ er
(^2) − (^1) )dr.
Using the substitution u = r^2 − 1, this evaluates to π(u − eu)|^0 − 1 = π/e.