(0, 3.00) m (-4.00, 0) m m1 F12 F32 0 m2 mg -x Three uniform spheres of masses m₁ = 1.50 kg, m₂ = 4.00 kg, and m3 = 5.00 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. 4.449 Note that the positive direction of x is defined to be to the right. I + 8.343 x Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. ĵ) × 10-11 N

(0, 3.00) m (-4.00, 0) m m1 F12 F32 0 m2 mg -x Three uniform spheres of masses m₁ = 1.50 kg, m₂ = 4.00 kg, and m3 = 5.00 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. 4.449 Note that the positive direction of x is defined to be to the right. I + 8.343 x Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. ĵ) × 10-11 N

Physics for Scientists and Engineers: Foundations and Connections

1st Edition

ISBN:9781133939146

Author:Katz, Debora M.

Publisher:Katz, Debora M.

Chapter7: Gravity

Section: Chapter Questions

Problem 53PQ: Two black holes (the remains of exploded stars), separated by a distance of 10.0 AU (1 AU = 1.50 ...

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