(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

Classical Dynamics of Particles and Systems

5th Edition

ISBN:9780534408961

Author:Stephen T. Thornton, Jerry B. Marion

Publisher:Stephen T. Thornton, Jerry B. Marion

Chapter10: Motion In A Noninertial Reference Frame

Section: Chapter Questions

Problem 10.20P: Calculate the effective gravitational field vector g at Earths surface at the poles and the equator....

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