Exam 10: Parametric Equations and Polar Coordinates

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Find the area of the indicated region. Round to the nearest ten-thousandth. Inner loop of Find the area of the indicated region. Round to the nearest ten-thousandth. Inner loop of

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Find the speed of the object each time it crosses the x-axis. Show all your work. Find the speed of the object each time it crosses the x-axis. Show all your work.

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Plot the given polar point. Plot the given polar point.    Plot the given polar point.

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Find all slopes of the curve at the given point. [It may be helpful to graph the curve.] Find all slopes of the curve at the given point. [It may be helpful to graph the curve.]

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Use a graphing utility to graph the conic section with focus (0, 0) and the given directrix and eccentricity. Use a window size of [-3, 3] by [-3, 3]. Directrix x = 2, e = 1

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Identify a range of values of Identify a range of values of   that produces one copy of the graph.  that produces one copy of the graph. Identify a range of values of   that produces one copy of the graph.

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Find the arc length of the curve exactly. Find the arc length of the curve exactly.

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Find an x-y equation for the given parametric equations. Find an x-y equation for the given parametric equations.

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For the given parametric equations, find a corresponding x-y equation for the curve. For the given parametric equations, find a corresponding x-y equation for the curve.

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For the given parametric equations, find a corresponding x-y equation for the curve. For the given parametric equations, find a corresponding x-y equation for the curve.

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Find a polar equation for the conic section with focus (0, 0) and the given directrix and eccentricity. Directrix x = -2, e = 4

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The time required for a skier, initially at rest, to ski from point A to point B on an inclined plane (where B is not directly downhill from A ) 5.4802k

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The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation   . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by   , where   is a constant such that   . Describe how the inclusion of the factor   affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits. . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation   . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by   , where   is a constant such that   . Describe how the inclusion of the factor   affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits. , where The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation   . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by   , where   is a constant such that   . Describe how the inclusion of the factor   affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits. is a constant such that The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation   . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by   , where   is a constant such that   . Describe how the inclusion of the factor   affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits. . Describe how the inclusion of the factor The orbits of the planets can be modeled easily by assuming i). that the sun is a perfect sphere and ii). that each planet is influenced only by the gravitational field of the sun (that is, each planet is unperturbed by gravitational forces from other planets, distant stars, etc.). According to Newton's (classical) theory of gravity, these assumptions result in elliptical planetary orbits with the sun at one focus. That is, the orbit can be described by the polar equation   . However, according to Einstein's (relativistic) theory of gravitation, the orbits are more accurately described by   , where   is a constant such that   . Describe how the inclusion of the factor   affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits. affects the orbit. That is, compare the classical orbit to the relativistic orbit. How do they differ? Draw figures that summarize the differences in the classical and relativistic orbits.

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Parametric equations for the position of an object are given. Find the object's velocity and speed at the given time. Parametric equations for the position of an object are given. Find the object's velocity and speed at the given time.

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Find all polar coordinate representations of the given rectangular point. Find all polar coordinate representations of the given rectangular point.

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Compute the surface area of the surface obtained by revolving the given curve about the indicated axis. Compute the surface area of the surface obtained by revolving the given curve about the indicated axis.

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Find the arc length of the curve exactly. Find the arc length of the curve exactly.

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Find all points of intersection of the two curves. Find all points of intersection of the two curves.

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Find parametric equations describing the given curve. The line segment from Find parametric equations describing the given curve. The line segment from   to  to Find parametric equations describing the given curve. The line segment from   to

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Find a polar equation corresponding to the given rectangular equation. Find a polar equation corresponding to the given rectangular equation.

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