Flatland said:
But mass will only resist acceleration if there is inertia. During free-fall there is no inertia.
Not really. You seem to be identifying inertia with the sensation you feel when standing on the ground of the Earth: the Earth pulls you towards its centre of mass, you are pressed against the ground and the ground reacts with a normal force of equal magnitude and opposite direction and you seem to resist that, in a sort of loop, which leads to a quite stable equilibrium (net force = 0). Instead, when in free-fall, like when you go down in a rapidly falling elevator or down a hill in a roller coaster (that is to say, when there is no opposition of the counter-force of the mass you are attracted to), you don’t have the sensations mentioned at the beginning. But that doesn’t mean that either the weight or the inertia is missing in free-fall:
- First, you are not weightless. It’s only that the weight is not apparent in that way, it’s not detectable through that particular method. But it’s there because you are accelerating towards the Earth. And to the extent that the body we consider is big enough, it becomes apparent due to the non-homogeneity across distance of the gravitational field: particles closer to the Earth are attracted more than those farther away. That’s why you have tides (tidal effects, in general).
- Second, if there is weight, there is inertia. Otherwise, you would accelerate at a much higher rate.
In the standard explanation, the justification goes as follows:
The force of gravity is:
F = \frac{{GM_g m_g }}{{R^2 }}
Your acceleration is:
<br />
\begin{gathered}<br />
F = m_i a_m = \frac{{GM_g m_g }}<br />
{{R^2 }} \to \hfill \\<br />
a_m = \frac{{\frac{{GM_g m_g }}<br />
{{R^2 }}}}<br />
{{m_i }} = \frac{{m_g }}<br />
{{m_i }}\frac{{GM_g }}<br />
{{R^2 }} = \frac{{GM_g }}<br />
{{R^2 }} \hfill \\ <br />
\end{gathered} <br />
As you can see, in the standard explanation, your gravitational mass is balanced out by your inertial mass and so you are attracted to the Earth at a rate only related to the (gravitational) mass of the Earth.
What we are saying here (not objected so far) is that the explanation should be slightly different, for example as follows:
<br />
\begin{gathered}<br />
F = m_i \frac{{M_i }}<br />
{{(m_i + M_i )}}\frac{G}<br />
{{R^2 }}(m_g + M_g ) \to \hfill \\<br />
a_m = \frac{F}<br />
{{m_i }} = \frac{{m_i \frac{{M_i }}<br />
{{(m_i + M_i )}}\frac{G}<br />
{{R^2 }}}}<br />
{{m_i }} = \frac{{GM_i }}<br />
{{R^2 }}\frac{{(m_g + M_g )}}<br />
{{(m_i + M_i )}} \hfill \\ <br />
\end{gathered} <br />
The difference is that here your inertial mass is canceled out by your inertial mass. So that’s unavoidable. And then there is the possibility that the sum of the two intervening gravitational masses is canceled out by the sum of the two inertial masses… or not, if they were not really equivalent. The advantage of this formulation is that it opens the latter possibility without threatening Newton’s Third Law or conservation principles. Additionally, it’s not some ad hoc invention, but it links coherently with the logic of the whole system. In the last posts we were simply considering the possibility of replacing the idea of gravitational mass with a sort of “coefficient of gravitational charge” specific to each material, in the understanding of course that this is just an intellectual exercise, since no experiments have ever detected a difference between inertial and gravitational masses.
Maybe you are pointing at Einstein’s idea that free-fall motion is (not exclusive of but) equivalent to inertial motion, in a sufficiently small region of space and time (hence no tidal effects) and so you can apply the same laws of physics in both types of frames. That’s another issue. Maybe connected to this, but we were having a purely Newtonian discussion.
cragar said:
there are physicists now that are trying to prove that more massive objects fall fasters because the gravitational attraction between the Earth and the object would be greater.
Can you be more specific? The fact that, given two mutually attracting masses M and m1, if you replace m1 with a more massive m2, the meeting time is reduced… is not discussed here. That’s a non-controversial phenomenon. In that case, the relative acceleration (wrt M, for example) increases. It only happens that the centre of mass of the system slides a little towards m2. Due to this, the individual accelerations (wrt this centre of mass) turn out to be the same, no matter whether the falling object is m1 or m2. That’s mainstream physics, although Turtle and I were arguing that it’s better seen, more didactically shown with the longer formulation of Newton’s Law of Gravitation written above.