When discussing Newton's laws of motion, particularly Newton's third law of motion, the terms that almost everyone will use are "action" and "reaction".
You must not take this to mean that they understand what they're talking about.
Answer:
First, as you may know, the light travels at a given velocity.
In vaccum, this velocity is c = 3x10^8 m/s.
And we know that:
distance = velocity*time
Now, if some object (like a star ) is really far away, the light that comes from that star may take years to reach the Earth.
This means that the images that the astronomers see today, actually happened years and years ago (So the night sky is like a picture of the "past" of the universe)
Also, for example, if an astronomer sees some particular thing, he can apply a model (a "simplification" of some phenomena that is used to simplify it an explain it) and with the model, the scientist can infer the information of the given thing some time before it was seen.
Answer:
W = 1418.9 J = 1.418 KJ
Explanation:
In order to find the work done by the pull force applied by Karla, we need to can use the formula of work done. This formula tells us that work done on a body is the product of the distance covered by the object with the component of force applied in the direction of that displacement:
W = F.d
W = Fd Cosθ
where,
W = Work Done = ?
F = Force = 151 N
d = distance covered = 10 m
θ = Angle with horizontal = 20°
Therefore,
W = (151 N)(10 m) Cos 20°
<u>W = 1418.9 J = 1.418 KJ</u>
Answer:
The distance is ![D = 2.6 \ m](https://tex.z-dn.net/?f=D%20%20%3D%20%202.6%20%5C%20m)
Explanation:
From the question we are told that
The wavelength of the light is ![\lambda = 476.1 \ nm = 476.1 *10^{-9} \ m](https://tex.z-dn.net/?f=%5Clambda%20%20%3D%20%20476.1%20%5C%20nm%20%20%3D%20%20476.1%20%2A10%5E%7B-9%7D%20%5C%20m)
The distance between the slit is ![d = 0.29 \ mm = 0.29 *10^{-3} \ m](https://tex.z-dn.net/?f=d%20%3D%20%200.29%20%5C%20%20mm%20%20%3D%20%200.29%20%2A10%5E%7B-3%7D%20%5C%20m)
The between the first and second dark fringes is ![y = 4.2 \ mm = 4.2 *10^{-3} \ m](https://tex.z-dn.net/?f=y%20%3D%20%204.2%20%5C%20mm%20%20%3D%20%204.2%20%2A10%5E%7B-3%7D%20%5C%20m)
Generally fringe width is mathematically represented as
![y = \frac{\lambda * D }{d}](https://tex.z-dn.net/?f=y%20%20%3D%20%20%5Cfrac%7B%5Clambda%20%2A%20D%20%7D%7Bd%7D)
Where D is the distance of the slit to the screen
Hence
![D = \frac{y * d}{\lambda }](https://tex.z-dn.net/?f=D%20%20%3D%20%20%5Cfrac%7By%20%2A%20%20d%7D%7B%5Clambda%20%7D)
substituting values
![D = \frac{ 4.2 *10^{-3} * 0.29 *10^{-3}}{ 476.1 *10^{-9} }](https://tex.z-dn.net/?f=D%20%20%3D%20%20%5Cfrac%7B%204.2%20%2A10%5E%7B-3%7D%20%2A%20%20%200.29%20%2A10%5E%7B-3%7D%7D%7B%20476.1%20%2A10%5E%7B-9%7D%20%7D)
![D = 2.6 \ m](https://tex.z-dn.net/?f=D%20%20%3D%20%202.6%20%5C%20m)