Acceleration of gravity in space.

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Discussion Overview

The discussion revolves around the calculation of the velocity of two objects in space as they are pulled together by gravity. Participants explore the implications of gravitational forces, conservation of energy, and the application of Newton's laws in a scenario where two objects collide rather than orbit.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant inquires about a formula to determine the velocity of two objects as they are pulled together by gravity, assuming no other forces act on them.
  • Another participant suggests using conservation of energy, stating that the sum of kinetic energy (KE) and potential energy (PE) is constant, and that knowing the initial PE can help find the KE and speeds.
  • A participant seeks clarification on how to determine the velocity of the objects at any point along their paths, given they start from rest and are of equal mass.
  • One response indicates that the velocity can be derived from the difference in PE at different distances between the objects, using kinetic energy formulas.
  • Another participant proposes using gravitational formulas and Newton's second law to find acceleration, expressing uncertainty about the necessity of this approach.
  • A later reply elaborates on the gravitational force between the two bodies and sets up differential equations to find the speed and location of each body over time.

Areas of Agreement / Disagreement

Participants express various methods for calculating velocity and acceleration, but there is no consensus on a single approach or formula. Multiple competing views on how to tackle the problem remain evident throughout the discussion.

Contextual Notes

Participants reference the need for the distance between the two bodies to be much greater than their dimensions, and the discussion includes assumptions about initial conditions and the nature of the forces involved.

loafula
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I was wondering if someone could answer a question for me. If you had two objects in space X distance from each other, is there a formula to determine what their velocity would be at the point where gravity finally pulls them together? Let's assume that the objects smack into each other instead of orbiting each other, and that there are no other forces acting on the objects.
 
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Hi loafula! :wink:

Yes, it's conservation of energy

KE + PE is constant, so if you know the original PE ( the potential energy ), you can find the KE, and therefore the speeds. :smile:
 
Thanks Tim!
I understand that KE would equal the PE from the objects initially moving apart, but is there a way to determine velocity two objects would have at any given point along their paths toward each other? Assume the two objects are of equal mass, and have an initial velocity of zero.
 
Equal mass or not, it'll always be minus the PE of their relative position. :wink:
 
loafula said:
Thanks Tim!
I understand that KE would equal the PE from the objects initially moving apart, but is there a way to determine velocity two objects would have at any given point along their paths toward each other? Assume the two objects are of equal mass, and have an initial velocity of zero.

Find the PE of the objects at their initial distance.
Find the PE of the objects for the distance between them at the given point.
Take the difference.
Use this answer and the formula for kinetic energy to find what velocity either mass has at that point.
 
cant you just find the acceleration with the gravity's formula and Newton's second law's formula? (if I am worng, please don't kill me). wouldn't be any point to it though after what you guys said.
 
fawk3s said:
cant you just find the acceleration with the gravity's formula and Newton's second law's formula? (if I am worng, please don't kill me). wouldn't be any point to it though after what you guys said.

I am understanding that we need only consider the forces between the 2 bodies.

We have
[tex]F_{12} = F_{21}= F = G \frac {m_1 m_2} d[/tex]

Where d is the distance between the 2 bodies.
We also need for d to be much greater then any dimension of either of the bodies.

For the acceleration of body 1 we have:
[tex]a_1 = \frac F {m_1}[/tex]

For body 2
[tex]a_2 = \frac F {m_2}[/tex]

Now set up a coordinate system with the Origin at the Center of Mass of the 2 bodies.

You now have 2 differential equations from which you can find the speed and location of either body and any time.
 

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