Answer:
W = 100000 J = 100 KJ
Explanation:
Here we will use the most basic and general formula of work, which is as follows:
![W = Fd](https://tex.z-dn.net/?f=W%20%3D%20Fd)
where,
W = Work Done = ?
F = Force Required = 200 N
d = Length of Track = 500 m
Therefore,
![W = (200\ N)(500\ m)\\](https://tex.z-dn.net/?f=W%20%3D%20%28200%5C%20N%29%28500%5C%20m%29%5C%5C)
<u>W = 100000 J = 100 KJ</u>
Kepler's third law is used to determine the relationship between the orbital period of a planet and the radius of the planet.
The distance of the earth from the sun is
.
<h3>
What is Kepler's third law?</h3>
Kepler's Third Law states that the square of the orbital period of a planet is directly proportional to the cube of the radius of their orbits. It means that the period for a planet to orbit the Sun increases rapidly with the radius of its orbit.
![T^2 \propto R^3](https://tex.z-dn.net/?f=T%5E2%20%5Cpropto%20R%5E3)
Given that Mars’s orbital period T is 687 days, and Mars’s distance from the Sun R is 2.279 × 10^11 m.
By using Kepler's third law, this can be written as,
![T^2 \propto R^3](https://tex.z-dn.net/?f=T%5E2%20%5Cpropto%20R%5E3)
![T^2 = kR^3](https://tex.z-dn.net/?f=T%5E2%20%3D%20kR%5E3)
Substituting the values, we get the value of constant k for mars.
![687^2 = k\times (2.279 \times 10^{11})^3](https://tex.z-dn.net/?f=687%5E2%20%3D%20k%5Ctimes%20%282.279%20%5Ctimes%2010%5E%7B11%7D%29%5E3)
![k = 3.92 \times 10^{-29}](https://tex.z-dn.net/?f=k%20%3D%203.92%20%5Ctimes%2010%5E%7B-29%7D)
The value of constant k is the same for Earth as well, also we know that the orbital period for Earth is 365 days. So the R is calculated as given below.
![365^3 = 3.92\times 10^{-29} R^3](https://tex.z-dn.net/?f=365%5E3%20%3D%203.92%5Ctimes%2010%5E%7B-29%7D%20R%5E3)
![R^3 = 3.39 \times 10^{33}](https://tex.z-dn.net/?f=R%5E3%20%3D%203.39%20%5Ctimes%2010%5E%7B33%7D)
![R= 1.50 \times 10^{11}\;\rm m](https://tex.z-dn.net/?f=R%3D%201.50%20%5Ctimes%2010%5E%7B11%7D%5C%3B%5Crm%20m)
Hence we can conclude that the distance of the earth from the sun is
.
To know more about Kepler's third law, follow the link given below.
brainly.com/question/7783290.
Answer:
The tension in the two ropes are;
T1 = 23.37N T2 = 35.47N
Explanation:
Given mass of the object to be 4.2kg, the weight acting on the bag will be W= mass × acceleration due to gravity
W = 4.2×10 = 42N
The tension acting on the bag plus the weight are three forces acting on the bag. We need to find tension in the two ropes that will keep the object in equilibrium.
Using triangular law of force and sine rule to get the tension we have;
If rope 1 is at 57.6° with respect to the vertical and rope 2 is at 33.8° with respect to the vertical, our sine rule formula will give;
T1/sin33.8° = T2/sin57.6° = 42/sin{180-(33.8°+57.6°)}
T1/sin33.8° = T2/sin57.6° = 42/sin88.6°
From the equality;
T1/sin33.8° = 42/sin88.6°
T1 = sin33.8°×42/sin88.6°
T1 = 23.37N
To get T2,
T2/sin57.6°= 42/sin88.6°
T2 = sin57.6°×42/sin88.6°
T2 = 35.47N
Note: Check attachment for diagram.
Distance ( say d ) is directly proportional to time ( say t ) .
mathematically ,
d = kt
where k is constant if proportionality .
Now differentiating the above equation with respect to time ,
we get ;
v = k
=> velocity is constant .
=> No acceleration .