After inventing a formula to describe gravity, Newton had this nice-looking formula,
but he couldn't do much with it because he didn't know any Calculus. He asked
around to find somebody who could fill him in on Calculus, and was surprised to
discover that nobody knew what he was talking about, because Calculus didn't
exist yet. So he did the only thing he could think of . . . he invented Calculus, and
then he was all set, and had everything he needed.
He took his formula for gravity, massaged it with Calculus, kneaded it with Geometry,
and came up with a bunch of really neat but weird predictions:
-- Planets travel around the sun in elliptical orbits, with the sun at one focus of
each ellipse.
-- The radius vector (line) from the sun to each planet sweeps out equal area
in equal intervals of time, so the planet has to travel faster when it's nearer
the sun, and slower when it's farther from the sun.
-- The ratio of the square of orbital period to the cube of the semi-major-axis
of the orbit is the same number for every object that orbits the sun.
These predictions didn't go over too well with the people in Newton's neighborhood,
for a variety of reasons. First of all, most of them couldn't read. The ones who
could read were also mostly left out in the cold, because they could only read
English, whereas Newton did his writing in Latin. And finally, even the people
who could read Latin, like his rector, his Bishop, his beadle, and his sexton, had
no idea what the heck he was talking about altogether.
But finally, after Newton had almost given up in despair and nailed his article
to the front door of the church, a tourist visiting his town happened to walk by
one day. He stopped to read Newton's paper, and hadn't gotten past the first
few paragraphs before he yelled out "Eureka!" and went running down the
street to Newton's house. He had to wait a while because Newton was taking
a bath with his gold crown, but he finally scored an audience with the old man
and breathlessly gave him the news:
His three predictions of planetary motion that he made up from his gravity and
his calculus were exactly the same as three popular Polish proverbs called
"Kepler's Laws". It seems that Kepler was a guy who had spent his whole life
going through the notebooks and diaries of Tycho who was a Danish hermit
who spent his life in the woods looking at the stars every night and . . . well,
it was all very complicated, but the bottom line was that Kepler came up with
the exact same three laws by going through years and years of actual factual
measurements of the real motions of the real planets, and now here came Newton
with his calculus and his geometry and his gravity and showed why the planets
must move in the way they actually do.
And that was the best proof of gravity that anybody could ask for, so Isaac said
to the visitor "Good day to you sir", and they all lived happily ever after.
(They Were Able To Find The Orbit Of a Comet And Predict The Year Of its Return)
Weight = mass x gravity. Weight (in newton) = mass (in kilogram) x gravity (in meter/second2, equivalent to newton/kilogram). Note: close to Earth's surface, gravity is about 9.8 meter/second2.
The metric unit for measuring human weight is actually the Newton (N). Newton's are a measure of force and weight is the product of the acceleration of gravity and an objects mass. The metric unit for measuring human mass is the kilogram (kg).
In Newton's law of universal gravitation, an object's weight is equal to the force of gravity acting on it. This force depends on the mass of the object and the acceleration due to gravity, typically 9.81 m/s^2 on Earth. The weight of an object can be calculated using the formula: weight = mass x acceleration due to gravity.
(They Were Able To Find The Orbit Of a Comet And Predict The Year Of its Return)
(They Were Able To Find The Orbit Of a Comet And Predict The Year Of its Return)
(They Were Able To Find The Orbit Of a Comet And Predict The Year Of its Return)
Isaac Newton with his law of universal gravitation is perhaps best known for explaining gravity, however in modern physics gravitation is described using Albert Einstein's general theory of relativity.
(They Were Able To Find The Orbit Of a Comet And Predict The Year Of its Return)
Kepler made discoveries regarding the planet's distance from the sun and how long it takes a planet to orbit the sun. In Newton's Version of Kepler's Third Law, Newton expands on these ideas by using his Theory of Gravity.
To calculate the mass of an object using a Newton meter, you would measure the force of gravity acting on the object in Newtons, and then divide this force by the acceleration due to gravity (9.8 m/s^2) to find the mass in kilograms. The formula is mass = force of gravity / acceleration due to gravity.
Weight is the measure of the pull of gravity. Weight is the mass of an object and can be measured by using a scale.
Weight = mass x gravity. Weight (in newton) = mass (in kilogram) x gravity (in meter/second2, equivalent to newton/kilogram). Note: close to Earth's surface, gravity is about 9.8 meter/second2.
Edmond Halley and Alexis Clairaut made significant contributions to the understanding of the orbits of comets and the shape of the Earth using Newton's ideas of mathematics and gravity. Halley famously predicted the return of Comet Halley by applying Newton's laws of motion and universal gravitation. Clairaut extended this work by using Newtonian principles to determine that the Earth is not a perfect sphere but an oblate spheroid, confirming that the planet's equatorial diameter is larger than its polar diameter due to its rotation. These discoveries laid the foundation for modern celestial mechanics and geophysics.
Use the formula: weight = mass x gravity. Since you are using SI units, use 9.8 for gravity.
You need differential equations and partial differential equations to describe and predict the dynamic behaviour of systems. Newton and Laplace developed differential equations originally and simultaneously (using different notation) to work with gravity and the movement of the moon and planets.
Some demonstration ideas for Newton's second law include using different masses on a frictionless surface to show how force affects acceleration, using a pulley system to vary the force applied to an object, or using a spring scale to measure the force required to accelerate an object.