Uniform circular motion is a specific type of motion in which an object travels in a circle with a constant speed. For example, any point on a propeller spinning at a constant rate is executing uniform circular motion.

While the magnitude of its velocity remains constant, the direction of its velocity is constantly changing.The acceleration causing this change in velocity is always directed towards the center of the circular path.

The period, T, is the time the object takes to make a complete circle. It is measured in seconds.

\begin{gather*}
v=\frac{2\pi r}{T} \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ a=\frac{4\pi ^{2} r}{T^{2}} =4\pi ^{2} rf^{2}\\
v=velocity,\ T=period,\ r=radius,\ f=frequency,\ a=acceleration
\end{gather*}

A centripetal force is a net force that acts on an object to keep it moving along a circular path.

The force vector is perpendicular to the velocity vector at each instant. It points towards the center of the circle.

Centripetal force is not a type of force; rather, it is just the name we give to the net force causing a circular motion.

\begin{gather}
F_{c} =\frac{mv^{2}}{r}\\
F_{c} =centripetal\ force,\ m=mass,\ v=velocity,\ r=radius\ of\ the\ circle \notag
\end{gather}

In uniform circular motion, the direction of the velocity changes constantly, so there is always an associated acceleration, even though the speed might be constant.

It is directed towards the center of the circular motion and is perpendicular to the instantaneous velocity of the object.

\begin{gather}
a=\omega ^{2} r\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ a=\frac{v^{2}}{r}\\
a=acceleration,\ \omega =angular\ velocity,\ v=velocity,\ r=radius \notag
\end{gather}

Great explanation of circular motion
\begin{gather}
F_{g} =\frac{Gm_{1} m_{2}}{r^{2}}\\
F_{g} =gravitational\ force,\ m=mass\ of\ object,\ r=distance\ between\ the\ center\ of\ the\ object \notag\\
G=gravitational\ constant\ \left( 6.67408\times 10^{-11}\right) \notag
\end{gather}

Sir Isaac Newton was an English mathematician and mathematician and physicist who lived from 1642-1727. The legend is that Newton discovered Gravity when he saw a falling apple while thinking about the forces of nature. Whatever really happened, Newton realized that some force must be acting on falling objects like apples because otherwise they would not start moving from rest. Newton also realized that the moon would fly off away from Earth in a straight line tangent to its orbit if some force was not causing it to fall toward the Earth. The moon is only a projectile circling around the Earth under the attraction of Gravity. Newton called this force "gravity" and determined that gravitational forces exist between all objects. Using the idea of Gravity, Newton was able to explain the astronomical observations of Kepler. The work of Galileo, Brahe, Kepler, and Newton proved once and for all that the Earth wasn't the center of the solar system. The Earth, along with all other planets, orbits around the sun. (Stanford)

Video explanationGravitational field strenght at a point is the force per unit mass experienced by a small point mass placed at that point.

\begin{gather}
g=\frac{F_{g}}{m}\\
g=gravitational\ field\ strenght,\ F_{g} =gravitational\ force,\ m=mass \notag
\end{gather}

g = 9.81ms^{-2} for Earth

The gravitational force is always attractive, proportional to 1/r^{2}, and proportional to m.

Laws that depend on 1/r^{2} are called inverse-square laws.

If the distance between the masses is **doubled** without changing mass, then the force between masses goes down to a **quarter** of its original value.

Which way is down? (optional)

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