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Aleksandr-060686 [28]
3 years ago
15

Which scientists contributed to discovering the universal law of gravitation? Check all that apply. Tycho Brahe Albert Einstein

Johannes Kepler Nicolaus Copernicus Sir Isaac Newton Robert Hooke
Physics
2 answers:
stich3 [128]3 years ago
6 0
<span>Johannes Kepler
</span>Isaac Newton

<span>Scientists who contributed to discovering the universal law of gravitation are Isaac Newton and Johannes Kepler. While, historically speaking, the discovery of gravitation is given to Newton, he said that he based his work on the law of motion, discovered by Kepler.  </span>
jekas [21]3 years ago
4 0
Scientists who contributed to discovering the universal law of gravitation are isaac newton and Johannes Kepler. While, traditionally speaking, the invention of gravitation is given to Newton, the same that he based mostly his work on the law of motion, discovered by <span>Johan Kepler.

Explanation:
</span>Sir Isaac<span> Newton: The Universal Law of Gravitation. </span>there's a well-liked<span> story that Newton was sitting </span>underneath a fruit tree<span>, </span>an apple<span> fell on his head, and he suddenly thought of the Universal Law of Gravitation</span>

Kepler's laws explain how the planets moved around the sun but not why. Newton filled in that gap by supposing there was a force acting between the bodies that were moving around each other.

The story goes that Newton saw an apple fall to the ground and it made him wonder why the fruit always fell straight to the ground; why did it not veer off to the left or right? According to his own laws of motion, anything that begins moving from a standing start is undergoing acceleration and, where there is acceleration, there must be a force.

 The apple started in the tree and landed on the Earth, which means there must be a force of attraction between the apple and the Earth.


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What is the difference between mutual flux, leakage flux and magnetizing flux<br> ​
Lemur [1.5K]

In simple words, flux can be stated as the rate of flow of a fluid, radiant energy, or particles across a given area.

<u>Explanation:</u>

<u>Mutual Flux:</u>

  • The magnetic lines present in among two magnets or solenoid is mutual flux.
  • These are the lines in which the attraction and repulsion happens.
  • The SI unit of mutual flux is the Henry

<u>Leakage Flux:</u>

  • In simple words, it can be stated as  the magnetic flux which does not follow the specially designed way in a magnetic circuit.
  • Leakage flux in the induction motor takes spot due to current runs through the essence of the induction motor.
  • The SI unit of Leakage flux is the Weber

<u>Magnetizing flux</u>

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3 0
3 years ago
What is the maximum number of lines per centimeter a diffraction grating can have and produce a complete first-order spectrum fo
Pachacha [2.7K]

Answer:

14,300 lines per cm

Explanation:

Answer:

14,300 cm per line

Explanation:

λ400 nm to 400nm

We can find the maximum number of lines per centimeter, which is reciprocal of the least distance separating two adjacent slits, using the following equation.

mλ = dsin (θ)

In this equation,

m is the order of diffraction.

λ is the wavelength of the incident light.

d is the distance separating the centers of the two slits.

θ is the angle at which the mth order would diffract.

To find the least separation that allows the observation of one complete order of spectrum of the visible region, we use the maximum wavelength of the visible region is 700 nm.

d =  mλ / sin (θ)

As we want the distance d to be the smallest then sin (θ) must be the greatest, and the greatest value of the sin (θ) is 1. For that we also use the longest wavelength because using the smallest wavelength, the longest wavelength would not be diffracted.

d =  mλ / sin (θ)

d =  1 x 700nm / 1

  = 700 nm

So, the least separation that would allow for the possibility of observing complete first order of the visible region spectra is 700 nm, and knowing the least separation we can find the maximum number of lines per cm, which is the reciprocal of the number of lines per cm.

n = 1/d

   = 1 / 700 x 10^{-9}

  = 1, 430,000 lines per m  

  =  14,300 lines per cm

<u>The maximum number of lines per cm, that would allow for the observation of the complete first order visible spectra.</u>

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