vishnu 73 said:
wait what is rigid body i mean is there a formal definition for a rigid body?
are you saying it does not have rotational KE because the sun and the Earth are not connected?
At root, the KE of a system is simply ∑½m
iv
i2, where the sum is taken over infinitesimal mass elements. Each such element is considered so small as to have no significant rotational KE.
But that is inconvenient when analysing systems of countless such elements. For a rigid body, i.e. one in which the pairwise distances between every pair of mass elements in it are conserved, we can represent the entire motion as the sum of a linear motion of its mass centre plus a rotational motion about some axis through that centre. For such a representation, it can be shown that ∑½m
iv
i2=½(∑m
i)v
com2+½I
xω
2, where ω is the rate of rotation and I
x is a constant describing the distribution of mass within the body about the given axis. Specifically, I
x=∑m
ix
i2, where x
i is the distance of element i from the axis.
In the case of a planet orbiting its star at distance r, not rotating on an axis of its own (i.e. one year=1 day, not gravitationally locked), each little mass element is describing a circle at the same rate and the same radius, just not all around the same centre. So if the linear speed of the planet is v then the KE of the planet is ∑½m
iv
com2=½Mv
com2.