Answer:
The deviation of a mirror is equal to twice the angle of incidence.The total angle between the straight-line path and the reflected ray is twice the angle of incidence. This is called the deviation of the light and measures the angle at which the light has strayed from its initial straight-line path.
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Answer:
Coefficient of friction will be 0.587
Explanation:
We have given mass of the car m = 500 kg
Distance s = 18.25 m
Initial velocity of the car u = 14.5 m/sec
As the car finally stops so final velocity v = 0 m/sec
From second equation of motion
![v^2=u^2+2as](https://tex.z-dn.net/?f=v%5E2%3Du%5E2%2B2as)
![0^2=14.5^2+2\times a\times 18.25](https://tex.z-dn.net/?f=0%5E2%3D14.5%5E2%2B2%5Ctimes%20a%5Ctimes%2018.25)
![a=-5.76m/sec^2](https://tex.z-dn.net/?f=a%3D-5.76m%2Fsec%5E2)
We know that acceleration is given by
![a=\mu g](https://tex.z-dn.net/?f=a%3D%5Cmu%20g)
![5.76=\mu\times 9.81](https://tex.z-dn.net/?f=5.76%3D%5Cmu%5Ctimes%20%209.81)
![\mu =0.587](https://tex.z-dn.net/?f=%5Cmu%20%3D0.587)
So coefficient of friction will be 0.587
Answer:
1.4 billion light years away
Explanation:
v = Recessional velocity = 30000 km/s[/tex]
= Hubble constant = ![\frac{65}{3.2\times 10^6}\ ly](https://tex.z-dn.net/?f=%5Cfrac%7B65%7D%7B3.2%5Ctimes%2010%5E6%7D%5C%20ly)
D = Distance to the galaxy
According to Hubble's law
![v=H_0D\\\Rightarrow D=\frac{v}{H_0}\\\Rightarrow D=\frac{3\times 10^{4}}{65}\times 3.2\times 10^6\\\Rightarrow D=1476923076.92307\ ly\\\Rightarrow D=1.4\times 10^9\ ly](https://tex.z-dn.net/?f=v%3DH_0D%5C%5C%5CRightarrow%20D%3D%5Cfrac%7Bv%7D%7BH_0%7D%5C%5C%5CRightarrow%20D%3D%5Cfrac%7B3%5Ctimes%2010%5E%7B4%7D%7D%7B65%7D%5Ctimes%203.2%5Ctimes%2010%5E6%5C%5C%5CRightarrow%20D%3D1476923076.92307%5C%20ly%5C%5C%5CRightarrow%20D%3D1.4%5Ctimes%2010%5E9%5C%20ly)
The galaxy is 1.4 billion light years away
Answer:
<em>a) 3.56 x 10^22 N</em>
<em>b) 3.56 x 10^22 N</em>
<em></em>
Explanation:
Mass of the sun M = 2 x 10^30 kg
mass of the Earth m = 6 x 10^24 kg
Distance between the sun and the Earth R = 1.5 x 10^11 m
From Newton's law,
F = ![\frac{GMm}{R^2}](https://tex.z-dn.net/?f=%5Cfrac%7BGMm%7D%7BR%5E2%7D)
where F is the gravitational force between the sun and the Earth
G is the gravitational constant = 6.67 × 10^-11 m^3 kg^-1 s^-2
m is the mass of the Earth
M is the mass of the sun
R is the distance between the sun and the Earth.
Substituting values, we have
F =
= <em>3.56 x 10^22 N</em>
<em></em>
A) The force exerted by the sun on the Earth is equal to the force exerted by the Earth on the Sun also, and the force is equal to <em>3.56 x 10^22 N</em>
b) The force exerted by the Earth on the Sun = <em>3.56 x 10^22 N</em>