Three uniform spheres of masses m1 = 3.50 kg, m2 = 4.00 kg, and m3 = 6.50 kg are placed at the corners of a right triangle (see figure below). Calculate the resultant gravitational force on the object of mass m2, assuming the spheres are isolated from the rest of the Universe. 103756 Note that the positive direction of x is defined to be to the right. î + 108387 Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. 10-11 (0, 3.00) m т 12 -4.00, 0) m х т2

Principles of Physics: A Calculus-Based Text
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Chapter11: Gravity, Planetary Orbits, And The Hydrogen Atom
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Three uniform spheres of masses m1 = 3.50 kg, m2 = 4.00 kg, and m3 = 6.50 kg are placed at the corners of a right
triangle (see figure below). Calculate the resultant gravitational force on the object of mass m2, assuming the spheres are
isolated from the rest of the Universe.
103756
Note that the positive direction of x is defined to be to the right. î + 108387
Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results
together. 10-11
(0, 3.00) m
т
12
-4.00, 0) m
х
т2
Transcribed Image Text:Three uniform spheres of masses m1 = 3.50 kg, m2 = 4.00 kg, and m3 = 6.50 kg are placed at the corners of a right triangle (see figure below). Calculate the resultant gravitational force on the object of mass m2, assuming the spheres are isolated from the rest of the Universe. 103756 Note that the positive direction of x is defined to be to the right. î + 108387 Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. 10-11 (0, 3.00) m т 12 -4.00, 0) m х т2
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