Examples of Newton in the following topics:

 Newton's Method is a method for finding successively better approximations to the roots (or zeroes) of a realvalued function.
 In numerical analysis, Newton's method (also known as the Newton–Raphson method), named after Isaac Newton and Joseph Raphson, is a method for finding successively better approximations to the roots (or zeroes) of a realvalued function.
 Use "Newton's Method" to find successively more accurate estimates for a function's $x$intercept

 Newton's rings are a series of concentric circles centered at the point of contact between a spherical and a flat surface.
 Although first observed by Robert Hooke in 1664, this pattern is called Newton's rings, as Newton was the first to analyze and explain the phenomena.
 Newton's rings appear as a series of concentric circles centered at the point of contact between the spherical and flat surfaces.
 An example of Newton's rings when viewed with white light is shown in the figure below .
 Newton's rings seen in two planoconvex lenses with their flat surfaces in contact.

 In the most general form, Newton's 2nd law can be written as $F = \frac{dp}{dt}$ .
 This fact, known as the law of conservation of momentum, is implied by Newton's laws of motion.
 Newton actually stated his second law of motion in terms of momentum: The net external force equals the change in momentum of a system divided by the time over which it changes.
 This statement of Newton's second law of motion includes the more familiar $F_{net} = ma$ as a special case.
 So for constant mass, Newton's second law of motion becomes

 Finally, Newton's Laws of motion address BODY as the system model; much worthwhile has resulted.
 Newton used vector mathematics to establish his Laws of Motion (1687,.
 To explain velocity, Newton needed first to explain vectors then he needed to explain calculus.
 Newton used vectors and calculus because he needed that mathematics.
 Newton's system was the simplest of all perspectives of matter ~ the BODY.

 Sir Isaac Newton was a scientist from England who was interested in the motion of objects under various conditions.
 Newton used these laws to explain and explore the motion of physical objects and systems.
 Newton's three laws are:
 Newton's third law basically states that for every action, there is an equal and opposite reaction.
 As your mom if she's clear on Newton's Third.

 Just like Newton's Second Law, which is force is equal to the mass times the acceleration, torque obeys a similar law.
 If you replace torque with force and rotational inertia with mass and angular acceleration with linear acceleration, you get Newton's Second Law back out.
 In fact, this equation is Newton's second law applied to a system of particles in rotation about a given axis.
 Similar to Newton's Second Law, angular motion also obeys Newton's First Law.

 Newton’s first law of motion describes inertia.
 Newton used these laws to explain and explore the motion of physical objects and systems.
 You have most likely heard Newton's first law of motion before.
 Newton's first law in effect on the driver of a car
 Newton's first law is hugely counterintuitive.

 During the 17th century, a revolution took place in what constituted science, particularly with the work of Isaac Newton in physics .
 Newton made a sharp distinction between the natural world, which he asserted was an independent reality that operated by its own laws, and the human or spiritual world.
 Newton, along with others, changed the basic framework by which individuals understood what was scientific .
 Kepler's law, which describes planet orbit, is an example of the sort of laws Newton believed science should seek.
 Isaac Newton was a key figure in the process which split the natural sciences from the humanities.

 While an apple might not have struck Sir Isaac Newton's head as myth suggests, the falling of one did inspire Newton to one of the great discoveries in mechanics: The Law of Universal Gravitation.
 Pondering why the apple never drops sideways or upwards or any other direction except perpendicular to the ground, Newton realized that the Earth itself must be responsible for the apple's downward motion.
 Theorizing that this force must be proportional to the masses of the two objects involved, and using previous intuition about the inversesquare relationship of the force between the earth and the moon, Newton was able to formulate a general physical law by induction.
 While Newton was able to articulate his Law of Universal Gravitation and verify it experimentally, he could only calculate the relative gravitational force in comparison to another force.
 where $F$ represents the force in Newtons, $M$ and $m$ represent the two masses in kilograms, and $r$ represents the separation in meters.

 Newton's universal law of gravitation states that every particle attracts every other particle with a force along a line joining them.
 Newton's universal law of gravitation states that every particle in the universe attracts every other particle with a force along a line joining them.
 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:
 Historically, Kepler discovered his 3 laws (called Kepler's law of planetary motion) long before the days of Newton.
 We shall derive Kepler's third law, starting with Newton's laws of motion and his universal law of gravitation.