Calculating Height of a Free-Falling Body Over Time

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Discussion Overview

The discussion centers on the calculation of the height of a free-falling body over time, particularly in scenarios where gravitational acceleration (g) is changing. Participants explore the mathematical complexities involved, including differential equations and conservation of energy, while also referencing related concepts such as elliptical orbits.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants inquire about the formula for height as a function of time when g is changing, suggesting a need for advanced mathematical tools like differential equations.
  • Others express their current limitations in mathematical knowledge, indicating they are still in high school and seeking simpler explanations.
  • One participant mentions that calculating velocity is straightforward, but they find the original question about height more complex.
  • There is a discussion about the relationship between elliptical orbits and free fall, with some participants suggesting that conservation of energy principles can be applied.
  • Some participants challenge the applicability of certain formulas, noting that the formula h = (1/2)gt² is only valid when g is constant, which contradicts the original question's premise.
  • There is a mention of iterative methods as a potential approach to solving the problem of height as a function of time, emphasizing the complexity of the situation.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the formula for height as a function of time in the context of changing g. Multiple competing views remain regarding the applicability of various formulas and the methods for solving the problem.

Contextual Notes

Limitations include the assumption that g may vary with height, which complicates the direct application of simpler formulas. The discussion also highlights the challenge of deriving time from distance in free fall scenarios, particularly when considering elliptical orbits.

ddddd28
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Considering a body falls a free fall and g is changing, what is the formula of the height as a function of time?
 
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ddddd28 said:
Considering a body falls a free fall and g is changing, what is the formula of the height as a function of time?
How much maths do you know? Differential equations?
 
Unfortunately not yet, I am still in high school. Can you show me the formula and explain it briefly?
 
It is too advanced for me.
 
ddddd28 said:
It is too advanced for me.

Getting a formula for the height (or speed) of a falling object as a function of time is mathematically very difficult (as you can see).

You can, however, calculate the speed of the object at each height using conservation of energy. Do you know about potential and kinetic energy under gravity?
 
yes of course, calculating the velocity is not a problem at all.
 
ddddd28 said:
yes of course, calculating the velocity is not a problem at all.

If you are looking for an interesting problem, you might like to try this. If a planet is in an elliptical orbit round the sun and you know its nearest point (perigee) ##r_1## and its furthest point (apogee) ##r_2##, can you calculate its speed at either of these points in terms of ##G##, ##M## - the mass of the sun - and ##r_1## and ##r_2##?
 
As far as I understand, at the points of perigee and apogee there is no radialic speed, so, it is calculated using the circular motion, isn't it?
If your problem involves elliptical motion knowledge, as you can guess, I will not be able to solve it.
The original question was asked because of pure curiosity. Is there any ellegent proof for that? and can you express the equation by only the distance between the objects, not the surface level?
 
  • #10
ddddd28 said:
As far as I understand, at the points of perigee and apogee there is no radialic speed, so, it is calculated using the circular motion, isn't it?
If your problem involves elliptical motion knowledge, as you can guess, I will not be able to solve it.

Yes, that there is no radial component of the velocity is key. You don't need to know anything else about elliptical orbits. You need conservation of energy and one other thing. Can you work out what that other thing is? It's another conservation law.

ddddd28 said:
The original question was asked because of pure curiosity. Is there any ellegent proof for that? and can you express the equation by only the distance between the objects, not the surface level?

You mean you think my solution in the above thread is not elegant enough? :frown: Some problems admit solutions in terms of energy conservation but don't give up exact solutions in terms of time easily or, sometimes, not at all.

Those equations in the above post are all based on distance between the centres of mass. The surface level ##R## simply represents the point at which the free fall abrupty comes to an end!
 
  • #11
  • #12
is it √GM/r ?
 
  • #13
ddddd28 said:
is it √GM/r ?

That's for a circular orbit, yes.
 
  • #14
I thought you were first considering a scenario of a free falling object?
 
  • #15
ddddd28 said:
Considering a body falls a free fall and g is changing, what is the formula of the height as a function of time?
Others may correct me if I am wrong, but I don't think there is a direct solution for finding distance as a function of time in this situation. You can find the time to fall a given distance by single equation, but not the other way around. You get the same problem with elliptical orbits. You can directly solve for the time it takes to travel from one point of an orbit to another, but you can't do so going the other way (except for when the two points are the periapis and apoapis.)
This doesn't mean that you can't solve the problem, but it generally involves a process of "narrowing down" to the answer rather than a direct solution.( one solution method involves iteration, where you plug a number into a equation, take the answer and plug it back into the equation and then repeat. ( how many times you repeat will determine the accuracy of your final answer.)
 
  • #16
FritoTaco said:
I thought you were first considering a scenario of a free falling object?
Yes, but a planet in an elliptical orbit is a free falling object.
FritoTaco said:
I was in high school last year, I only have half of my notes. Is this the formula? Unless your high school is more advanced, I don't remember using perigee and apogee.

h=12gt2​
h=\dfrac{1}{2}gt^{2}
This formula only is accurate for situations where g does not change with height. The original question dealt with the situation where it does, and this is something that must be accounted for with elliptical orbits.
 
  • #17
Janus said:
Yes, but a planet in an elliptical orbit is a free falling object.

This formula only is accurate for situations where g does not change with height. The original question dealt with the situation where it does, and this is something that must be accounted for with elliptical orbits.

Oh, I could only assume we used the same formula, I don't remember too much, but thanks for that.
 

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