Solving 1D First Order Equations for 3D Mass Positions and Velocities

Click For Summary
SUMMARY

This discussion focuses on deriving twelve one-dimensional first-order equations that describe the positions and velocities of two masses in three-dimensional space. The primary equation presented is r'' = -G m2 (r1 - r2)/|r1 - r2|^3, which is transformed into two first-order equations: a1' = a2 and a2' = -G m2 (a1 - r2)/|a1 - r2|^3. A suggestion is made to change coordinates to r_G and r, where r_G represents the center of mass, to facilitate the symbolic solution of these equations.

PREREQUISITES
  • Understanding of classical mechanics and gravitational forces
  • Familiarity with differential equations, particularly first-order equations
  • Knowledge of vector calculus in three dimensions
  • Experience with symbolic computation tools for solving equations
NEXT STEPS
  • Explore methods for solving first-order differential equations symbolically
  • Research the application of Newton's laws in three-dimensional motion
  • Learn about coordinate transformations in physics, specifically center of mass calculations
  • Investigate numerical methods for simulating gravitational interactions between masses
USEFUL FOR

Physics students, researchers in classical mechanics, and anyone involved in computational simulations of gravitational systems will benefit from this discussion.

Blanchdog
Messages
56
Reaction score
22
Homework Statement
Use the given equations to obtain the first order differential equations for the system of two gravitating bodies. Write them down on paper in terms of the individual components of the motion.
Relevant Equations
m1 r'' = -G m1 m2 (r1 - r2)/|r1 - r2|^3
m2 r'' = -G m1 m2 (r2 1 r1)/|r2 - r1|^3
Okay so I need to find 12 one dimensional first order equations that describe the position and velocity of both masses in 3 dimensions. The equations for the second body will be easy once I figure out how to do the first body, so I'll ignore that for now. For the first equation, I can rearrange it to become:

r'' = -G m2 (r1 - r2)/|r1 - r2|^3

And I can break that down into two first order equations

a1' = a2
a2' = -G m2 (a1 - r2)/|a1 - r2|^3

I'm just stuck on how I now break those up into x y and z and then solve them symbolically to be able to write them down.
 
  • Like
Likes Delta2
Physics news on Phys.org
Hi. You may find changing coordinates from ##r_1,r_2## to ##r_G,r## ,where ##r_G## is the coordinate of center of mass and ##\mathbf{r}=\mathbf{r_2-r_1}##, will be helpful.
\dot{x}_G=const.
\ddot{\mathbf{r}}=-G(m_1+m_2)\frac{\mathbf{r}}{r^3}
 
Last edited:

Similar threads

Replies
2
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K
Replies
3
Views
2K
Replies
7
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 12 ·
Replies
12
Views
2K
  • · Replies 97 ·
4
Replies
97
Views
16K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K