Do Large Objects Fall at the Same Rate as Smaller Ones Due to Earth's Gravity?

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Discussion Overview

The discussion revolves around the question of whether large objects fall at the same rate as smaller ones due to Earth's gravity. Participants explore the implications of gravitational equations, the effects of mass on acceleration, and the nuances of gravitational interactions between objects of varying sizes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions the standard teaching that all objects fall at the same speed, particularly when considering larger masses and the gravitational equation.
  • Another participant notes that while the Earth does experience a force due to the falling object, its acceleration is negligible for small masses like a tennis ball.
  • Some participants clarify that the simpler form of the gravitational equation is typically applied to objects whose mass is insignificant compared to Earth's mass.
  • It is mentioned that the gravitational equation holds for all masses, but the distance from the center of the Earth must be accurately considered to yield the standard acceleration value of 9.81 m/s².
  • A participant raises a scenario involving lifting a weight and questions whether the Earth moves at all in response, leading to a discussion about the relative motion of the Earth and the object being lifted.
  • Another participant suggests that if a large object, like Mars, were to approach Earth, it would experience the same gravitational acceleration as smaller objects, with the difference in impact time potentially influenced by the Earth's own acceleration.
  • Confounding factors such as tidal effects and Roche limits are mentioned as complicating the scenario of large objects falling towards Earth.
  • It is noted that a large object's gravitational pull would contribute to the overall gravitational interaction in a system involving both the Earth and the large object.

Areas of Agreement / Disagreement

Participants express a range of views on the effects of mass and distance on gravitational acceleration, with no consensus reached on the implications of large objects falling towards Earth compared to smaller ones. The discussion remains unresolved regarding the specific conditions under which different masses affect gravitational interactions.

Contextual Notes

Participants highlight the importance of considering the distance from the center of the Earth in gravitational calculations, as well as the complexities introduced by large masses and their gravitational effects.

Ghost803
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We keep getting drilled with the info in class that all objects would fall to the Earth at the same speed. And it does not make sense to me

So the equation is (Ge * m1 * m2)/r2 = F

And F = m1 * a. There fore m1 * a = (Ge* m1*m2)/r2

This can be simplified and the m1 eliminated by dividing it from both sides, so that a = Ge *m2(mass of earth)/r2.

So my question is, how does this work with masses larger than the earth? Because according to this equation the only thing determining acceleration is the mass of the Earth and the distance and the the Gravitational Constante Ge.

Do you just use the mass of the larger object to calculate acceleration and disregard the smaller object's mass?
 
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Because you also have a force on the Earth, the Earth is accelerating up to meet the falling object but normally the effect for a tennis ball is rather small so you can ignore it.

For two stars/planets falling into each other you have to take it into account.
 
i.e the simpler form of the equation is only used for objects whose mass when compared to Earth's is insignificant.
 
DaveC426913 said:
i.e the simpler form of the equation is only used for objects whose mass when compared to Earth's is insignificant.

Not quite.

Note that there are no approximations made in deriving the equation in the OP. It holds for all masses, but there is one key restriction built into it. You must use your distance from the center of the earth, that is the r in the denominator. If you use the radius of the Earth you get the common value of 9.81 m/s2. So this value is only meaningful at or near the Earth's surface.
 
OK. here's one for you...

I''m sitting here on my chair veiwing PF.
I now raise with one hand a 1/lb weight 2-feet above me.

The Earth does not move 2-feet backwards, of course, BUT, does it move at all?
 
pallidin said:
OK. here's one for you...

I''m sitting here on my chair veiwing PF.
I now raise with one hand a 1/lb weight 2-feet above me.

The Earth does not move 2-feet backwards, of course, BUT, does it move at all?

Yes. It moves an amount equivalent to the Earth's mass divided your arm's mass times two feet.
 
Integral said:
Not quite.

Note that there are no approximations made in deriving the equation in the OP. It holds for all masses, but there is one key restriction built into it. You must use your distance from the center of the earth, that is the r in the denominator. If you use the radius of the Earth you get the common value of 9.81 m/s2. So this value is only meaningful at or near the Earth's surface.
Right. Forgot about the distance thing.
 
Aah, I think I understand it now. I forgot to take into account the acceleration of the earth.

Which would be F= m2 * a.

m2 *a = (Ge *m1 *m2)/ r2

cancel out the m2s and you get a = Ge *m1/r2

So now my question is..


Does this mean that if any object how ever large were to come close to the earth, that it would have the same acceleration as us. And that any difference in speed for the two colliding, would solely be caused by the Earth also accelerating at a great speed, which it usually does not because our masses are soo insignificant?
 
Ghost803 said:
Does this mean that if any object how ever large were to come close to the earth, that it would have the same acceleration as us. And that any difference in speed for the two colliding, would solely be caused by the Earth also accelerating at a great speed, which it usually does not because our masses are soo insignificant?

What?
 
  • #10
I meant. Say an object like Mars or something were to come close to the Earth's surface. Would it accelerate towards earth, at 9.8m/s2, just like objects on Earth with really small mass?

And would any difference in time it would take for impact by the large object, compared to how long an small object, like us would take to hit the Earth be caused by the Earth also accelerating. Which the Earth would not usually do if small objects fall down, because their mass is so small compared to the mass of the earth.
 
  • #11
Ghost803 said:
I meant. Say an object like Mars or something were to come close to the Earth's surface. Would it accelerate towards earth, at 9.8m/s2, just like objects on Earth with really small mass?
Wellll... the part of Mars that is near Earth would feel the tug of 9.8m/s^2, yes. That there are a lot of confounding factors - mostly to do with tides (differences in pull at different points) and Roche limits - that make the question mostly academic.

Ghost803 said:
And would any difference in time it would take for impact by the large object, compared to how long an small object, like us would take to hit the Earth be caused by the Earth also accelerating. Which the Earth would not usually do if small objects fall down, because their mass is so small compared to the mass of the earth.

Yes, a large object would contribute its gravitational pull to the equation. (Note that you're now talking about a system whose mass is Earth PLUS Mars, so it makes sense that the attraction is stronger).
 

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