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Learning Goal

‹2 of 2 in this chapter

Newton's Law of Universal Gravitation and Einstein's Theory of General Relativity

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7.2

"Expressed in modern language, Newton's universal law of gravitation states that every object in the universe attracts every other object with a force that is directed along a line joining them. The force is directly proportional to the product of their masses and inversely proportional to the square of the distance between them." "G is a universal constant, meaning that it is thought to be the same everywhere in the universe. It has been measured experimentally to be G = 6.673 × 10⁻¹¹ N·m²/kg²." "Einstein based his theory on the postulate that acceleration and gravity have the same effect and cannot be distinguished from each other. He concluded that light must fall in both a gravitational field and in an accelerating reference frame." "To summarize the two views of gravity, Newton envisioned gravity as a tug of war along the line connecting any two objects in the universe. In contrast, Einstein envisioned gravity as a bending of space-time by mass."

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"Expressed in modern language, Newton's universal law of gravitation states that every object in the universe attracts every other object with a force that is directed along a line joining them. The force is directly proportional to the product of their masses and inversely proportional to the square of the distance between them."
"G is a universal constant, meaning that it is thought to be the same everywhere in the universe. It has been measured experimentally to be G = 6.673 × 10⁻¹¹ N·m²/kg²."
"Einstein based his theory on the postulate that acceleration and gravity have the same effect and cannot be distinguished from each other. He concluded that light must fall in both a gravitational field and in an accelerating reference frame."
"To summarize the two views of gravity, Newton envisioned gravity as a tug of war along the line connecting any two objects in the universe. In contrast, Einstein envisioned gravity as a bending of space-time by mass."

What you'll learn

  1. State Newton's law of universal gravitation and write its equation F = GmM/r²
  2. Explain the gravitational constant G and distinguish it from the local acceleration due to gravity, g
  3. Derive g = GM/r² and use it to explain why weight (not mass) varies from body to body
  4. Perform calculations using F = GmM/r² and the orbital relation r³/T² = GM/4π²
  5. Describe the Cavendish experiment and why measuring G was difficult
  6. Explain Einstein's theory of general relativity at a conceptual level and contrast it with Newton's view of gravity

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