Answer:
not moving
static actually means lacking in movement or action❤
From the equestion:
I=V÷R
I=20÷100
I=0.2A
<u>Answer:</u>
<em>The required radius of its motion is
.</em>
<u>Explanation:</u>
The formula for calculating the required radius of its motion is given by

Where <em>m= mass </em>
<em>V= moving velocity
</em>
<em>F=frictional force
</em>
<em>r = radius of its motion
</em>
Then the required radius of its motion is given by

<u>Given that
</u>
<em>mas =0.0818 kg
</em>
<em>Frictional force= 0.108 N
</em>
<em>Moving with Velocity of = 0.333 m/s
</em>
<em>radius of its motion =
</em>
<em>Hence the required radius of its motion is r =
</em>
T² caries directly as R³ .
This is Kepler's 3rd law of planetary motion .
Answer:
p = -q
he distance is equal to the current distance, so the distance does not change
Explanation:
For this exercise we can solve it using the equation of the constructor
1 / f = 1 / p + 1 / q
where f is the focal length, p the distance to the object and q the distance to the image
For a flat surface the radius is at infinity, therefore 1 / f = 0, which implies
1 / p = - 1 / q
p = -q
Therefore the distance is equal to the current distance, so the distance does not change