Three uniform spheres of masses m₁ = 3.50 kg, m₂ = 4.00 kg, and m3 = 5.50 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. -9.17 Î+ 1.03 X Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. 1) × 10-11 N ✓ (0, 3.00) m (-4.00, 0) m ma Fa m₁ F12 0 m₂
Three uniform spheres of masses m₁ = 3.50 kg, m₂ = 4.00 kg, and m3 = 5.50 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. -9.17 Î+ 1.03 X Remember that superposition allows us to calculate the forces do to each sphere separately and then add the results together. 1) × 10-11 N ✓ (0, 3.00) m (-4.00, 0) m ma Fa m₁ F12 0 m₂
Principles of Physics: A Calculus-Based Text
5th Edition
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Raymond A. Serway, John W. Jewett
Chapter11: Gravity, Planetary Orbits, And The Hydrogen Atom
Section: Chapter Questions
Problem 10P
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![Three uniform spheres of masses m₁ = 3.50 kg, m₂ = 4.00 kg, and m3 = 5.50 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.
-9.17
B✓ Î+1.03
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
m3
0
y
m₁
F12
m₂
x](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F59becfc2-4192-4132-a546-669cd63aafbe%2F2177dc94-452c-4a2f-a410-1a5cdc36771b%2Fyzcmmy7_processed.png&w=3840&q=75)
Transcribed Image Text:Three uniform spheres of masses m₁ = 3.50 kg, m₂ = 4.00 kg, and m3 = 5.50 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.
-9.17
B✓ Î+1.03
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
m3
0
y
m₁
F12
m₂
x
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