00:01
Hello students, let us look on this question.
00:02
So, in this question we have given the sun in the mid, we have given this is sun and this is the distance that is given to us is r a and this is the r p, okay.
00:14
This is a p g and p g distances both are given to us and this is the any orbital particle moving with the speed of v a and here moving with the speed of v p, this is v p, okay.
00:28
And we have given some values here.
00:30
First of all we have given distance r p, r p equal to 1 .47 into 10 raise to the power 7 kilometer.
00:39
Then we have given the r a equal to 1 .52 into 10 raise to the power 7 kilometer.
00:45
Then we have given the speed of the point a that is equal to 29 .29 into 10 raise to the power 3 meter per second.
00:53
Then the mass of the e is equal to simply given to us 5 .922 into 10 raise to the power 24 kg.
01:03
And finally, we have given the mass of the s is equal to 1 .989 into 10 raise to the power 30 kg.
01:10
These are the values that is given to us.
01:12
And we know in the circular orbit is we can set all the points.
01:16
If i am talking about the first of all the angular momentum, if i am talking about the angular momentum that is angular momentum and second thing is total energy, total energy.
01:32
So, we can say both are conserved in this circular motion, both are conserved...