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  1. Gravity field surrounding Earth from a macroscopic perspective. Newton's law of universal gravitation can be written as a vector equation to account for the direction of the gravitational force as well as its magnitude. In this formula, quantities in bold represent vectors.

  2. Apr 10, 2024 · 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.

  3. Feb 20, 2022 · 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 \[ F = G\dfrac{mM}{r^2},\] where \(F\) is the magnitude of the gravitational force and \(G\) is a proportionality factor called the gravitational constant. \(G\) is a universal ...

    • Figure \(\PageIndex{1}\): According to early accounts, Newton was inspired to make the connection between falling bodies and astronomical motions when he saw an apple fall from a tree and realized that if the gravitational force could extend above the ground to a tree, it might also reach the Sun.
    • Figure \(\PageIndex{2}\): Gravitational attraction is along a line joining the centers of mass of these two bodies. The magnitude of the force is the same on each, consistent with Newton’s third law.
    • Figure \(\PageIndex{3}\): The distance between the centers of mass of Earth and an object on its surface is very nearly the same as the radius of Earth, because Earth is so much larger than the object.
    • Figure \(\PageIndex{4}\): The Moon causes ocean tides by attracting the water on the near side more than Earth, and by attracting Earth more than the water on the far side.
    • Overview
    • Newton’s law of universal gravitation
    • How to find gravitational field strength
    • What else should I know about Newton’s law of universal gravitation?

    Review your understanding of Newton's law of universal gravitation in this free article aligned to NGSS standards.

    Gravitational force Fg‍  is always attractive, and it depends only on the masses involved and the distance between them. Every object in the universe attracts every other object with a force along an imaginary line between them.

    The equation for Newton’s law of gravitation is:

    Fg=Gm1m2r2‍ 

    where:

    Fg‍  is the gravitational force between m1‍  and m2‍ ,

    G‍  is the gravitational constant equal to 6.67×10−11m3kg⋅s2‍ , and

    All objects attract other objects by producing a gravitational field g‍ , which is defined as gravitational force per unit mass. We can find the strength of the gravitational field of mass m1‍  on any object with mass m2‍  by dividing the above equation by m2‍ , and simplifying.

    g=Fgm2=Gm1m2r2m2=Gm1r2‍

    •Gravity causes attraction between all objects. Every mass attracts every other mass. That means you are gravitationally attracted to your friend, your pet, and even your pizza.

    •The variable r‍  is the distance between the centers of mass. We measure the distance between the objects from their centers, not their surfaces.

  4. 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.

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  6. Feb 9, 2021 · Summary. Newton's three dynamical equations describe the motion of a body with mass m under the influence of a force F. They form the heart of Newton's principal work, the Principia Mathematica, where for the first time motion is defined and described in precise mathematical terms using derivatives. These equations were the starting point for ...

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