Emanresu said:
Thank you for your answer. I accept what you say as a fact. So my confusion is to do with why a constant rate of fuel consumption does not produce a constant force. Can you explain this please ?
E.
Suppose an object is gaining kinetic energy from 0 joules... at a rate of P joules per second where P is a constant... ie:
Energy = Pt
(1/2)mv^2 = Pt
now take the derivative of both sides:
mv*dv/dt = P
mv*a = P
ma = P/v
ie: Force = P/v. as the velocity of the object increases... the force driving it foward gets smaller and smaller...
But what did I use above... that kinetic energy = (1/2)mv^2. But why is kinetic energy this way... as (1/2)mv^2?
I think we need to demonstrate why (1/2)mv^2 is useful... and why energy, kinetic energy and work ideas are useful...
The answer to all this comes from the fact that all the fundamental forces are "conservative"... ie: \int Fdx depends only on the final position and initial position... and not the path in between... or anything else for that matter...
Let's take the gravitational force as an example... for simplicity I'm going to say that the force is mg... take an object moving under the influence of a gravitaitonal force and nothing else... so we haven't defined energy yet... we're just working with forces and kinematics...
taking up as positive... down as negative... as an object goes from h1 to h2... \int Fdx is -mg(h2-h1).
see that the result of this integral depends only on h2 and h1... not on the time it takes the object to get from h1 to h2... not on the path between h1 and h2...
now we also know that (1/2)mvf^2 - (1/2)mvi^2 = \int Fdx
so: (1/2)mvf^2 - (1/2)mvi^2 = -mg(h2-h1).
so this is a critical point... the change in velocity is the result of a change in position... or rather, given the initial position and initial velocity... we can calculate the velocity of the object at any time, knowing its position at that time. notice... time is not anywhere here...
we also see that
(1/2)mvf^2 +mg(h2) = (1/2)mvi^2 + mg(h1)
so (1/2)mv^2 + mgh is a conserved quantity! we can find the velocity at any height that this object is at given the initial (1/2)mv^2 + mgh value.
So now, it makes sense to define these terms to make use of that the fact that this quantity is conserved... Kinetic energy as (1/2)mv^2... gravitational potential energy as mgh... total energy as (1/2)mv^2 + mgh.
so:
1) \int Fdx is a useful integral in nature... because the fundamental forces are conservative and this result depends on only initial and final positions... and it gives us a relationship between the initial and final velocities of an object under the influence of this force.
2) Since \int Fdx = (1/2)mvf^2 - (1/2)mvi^2... and since \int Fdx = U(final position) - U(initial position) for some function U... we get conservation of (1/2)mv^2 + U.
3) For the above 2 reasons, it is useful to define a quantity called kinetic energy as (1/2)mv^2... and a quantity U as gravitational potential energy (for our case above)... and the conserved quantity "energy" as the sum of these 2 (or in general sum of kinetic energy and all potential energies)... Also, as a result of defining kinetic energy in this way \int Fdx is hence a change in kinetic energy.
Now, above I was just talking about 1 object just experiencing a gravitational force... but the thing is all the fundamental forces are conservative... the integral of Fdx for any of them depends only on final position and initial position. we can get potential energies for each fundamental force.
Hope this gives some idea of why we define KE the way we do... and why energy is defined the way it is...