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Calculus and Newton’s 2 nd Law Sometimes, we want to find a formula for the velocity (or position) of an object as a function of time. 公式
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(1) Solve Newton’s 2 nd Law for the acceleration.
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(2) Find the velocity by integrating the expression for the acceleration. 求它的积分
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(2) Find the velocity by integrating the expression for the acceleration.
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(3) If necessary, integrate again to find the position.
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Example What is the least speed for a projectile launched vertically upward from the Earth’s surface, such that it will continue into space and never return to Earth? Assume that gravity is the only force felt after launch.
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GIVEN: Mass of the object m Mass of the Earth m E Height of the object from the center of the Earth y(t) Gravitational force F g = Gm E m/y 2 (down) FIND: Initial speed v i such that the object never returns to the Earth.
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PROCEDURE: (1) Use Newton’s 2 nd Law to find the acceleration of the object. (2) Integrate the acceleration to get an expression for the speed as a function of time. (3) Analyze this expression to find the minimum launch speed such that the velocity never changes direction.
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Example When a small sphere, starting from rest, falls through a liquid, it experiences a drag force F D in addition to the force of gravity. F D is directed upwards and has a magnitude F D = bv, where b is a constant. Find the speed of the sphere as a function of time, v(t).
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TRANSLATION: An object of known mass accelerates from rest, subject to known forces; find an expression for its speed as a function of time.
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GIVEN: Mass of the object m Weight force F g = mg (down) Drag force F d = bv (up) FIND: Velocity v(t)
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PROCEDURE: (1) Use Newton’s 2 nd Law to find the acceleration of the object. (2) Integrate the acceleration to get an expression for the velocity as a function of time.
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It is nice to solve Newton’s 2 nd Law with calculus… but usually it doesn’t work! Example: The motion of three planets, interacting via gravity, has no analytical solution.
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In such cases, we must solve Newton’s 2 nd Law numerically, using computers.
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Newton’s 2 nd Law (update form): (Assumes that Δt is small enough for F to be almost constant.)
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Example: compute the Earth’s motion around the Sun.
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Step 1:
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Step 2:
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Step 3:
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And so on…
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