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      • The weight of an object mg is the gravitational force between it and Earth. Substituting mg for F in Newton’s universal law of gravitation gives mg = GmM r2, where M is the mass of the object, M is the mass of Earth, and r is the distance to the center of Earth (the distance between the centers of mass of the object and Earth).
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  2. For two bodies having masses m and M with a distance r between their centers of mass, the equation for Newton’s universal law of gravitation is. F = GmM r2 F = G m M r 2, where F is the magnitude of the gravitational force and G is a proportionality factor called the gravitational constant.

  3. Newton's law of universal gravitation states that every particle attracts every other particle in the universe with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

  4. Newton’s Law of Universal Gravitation. where W is the weight of an object with mass m due to the earth’s gravitational force, G is the universal gravitational constant = 6.67x10-11 m2/kg2, ME is the mass of the earth, r is the distance between the object and the center of mass of the earth.

  5. Apr 10, 2024 · Newton’s Law of Gravitation. Newton’s law of gravitation can be expressed as \[\vec{F}_{12} = G \frac{m_{1} m_{2}}{r^{2}} \hat{r}_{12} \label{13.1}\] where \(\vec{F}_{12}\) is the force on object 1 exerted by object 2 and \(\hat{r}_{12}\) is a unit vector that points from object 1 toward object 2.

  6. For two bodies having masses m and M with a distance r between their centers of mass, the equation for Newton’s universal law of gravitation is. F = G m M r 2 F = G m M r 2. where F is the magnitude of the gravitational force and G is a proportionality factor called the gravitational constant.

  7. Substituting mg for \(F\) in Newton’s universal law of gravitation gives \[mg = G\dfrac{mM}{r^2}, \] where \(m\) is the mass of the object, \(M\) is the mass of Earth, and \(r\) is the distance to the center of Earth (the distance between the centers of mass of the object and Earth).

  8. Sep 23, 2024 · In Newton’s law of universal gravitation, the attractive force between two objects (F) is equal to G times the product of their masses (m1m2) divided by the square of the distance between them (r2); that is, F = Gm1m2 / r2. The value of G is (6.6743 ± 0.00015) × 10 −11 m 3 kg −1 s −2.

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