By Newton's universal law of gravitation the free-fall acceleration a of a body, such as the satellite shown in the figure, falling a great distance to the surface is not the constant g. Rather, the acceleration a is inversely proportional to the square of the distance from the center of the Earth, a = k/r2, where k is the constant of proportionality. Use the fact that at the surface of the Earth r = R and a = g determine k. If t positive direction is upward, use Newton's second law and his universal law of gravitation to find a differential equation for the distance r. k= 6.255-10 x d²r dr² = k R² X satellite of mass m surface

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
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Chapter4: Polynomial And Rational Functions
Section4.3: Zeros Of Polynomials
Problem 68E
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By Newton's universal law of gravitation the free-fall acceleration a of a body, such as the satellite shown in the figure, falling a great distance to the surface is not the constant g. Rather, the acceleration a is
inversely proportional to the square of the distance from the center of the Earth, a = k/r², where k is the constant of proportionality. Use the fact that at the surface of the Earth r = R and a = g to determine k. If the
positive direction is upward, use Newton's second law and his universal law of gravitation to find a differential equation for the distance r.
K = 6.255.107
d²r
dt²
k
R²
X
satellite of
mass m
surface
R
Earth of mass M
Transcribed Image Text:By Newton's universal law of gravitation the free-fall acceleration a of a body, such as the satellite shown in the figure, falling a great distance to the surface is not the constant g. Rather, the acceleration a is inversely proportional to the square of the distance from the center of the Earth, a = k/r², where k is the constant of proportionality. Use the fact that at the surface of the Earth r = R and a = g to determine k. If the positive direction is upward, use Newton's second law and his universal law of gravitation to find a differential equation for the distance r. K = 6.255.107 d²r dt² k R² X satellite of mass m surface R Earth of mass M
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