Orbital Mechanics: Find Eqns of Motion w/ Initial Conditions

In summary, the conversation discusses the difficulty in calculating the position of an orbiting body and asks if there is a way to find the equations of motion for a satellite's orbit using only initial tangential velocity, distance from the central mass, and satellite mass. It is referred to as the two-body problem and a possible solution is proposed using a word document that takes into account the masses and distance between the bodies.
  • #1
Timothy S
49
0
Hello,

After searching on the internet, I have come to the conclusion that there is no completely general way to calculate the position of an orbiting body. My question is whether there is a way to find the equations of motion with respect to time of a satellite orbit given only the initial tangential velocity, distance from the central mass, and mass of the satellite. If there is, I would appreciate a derivation of the equation.

Thank you.
 
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  • #3
you are looking for paticular object?
 
  • #4
If you ignore the mass of the satellite, its easy, its rotation rate = v / r (radians per second)

If you had the mass of the orbited body:
Using the attached word document, given both masses, and the centre to centre distance, you can derive what you need, if not you may get some mileage from it anyway.
 

Attachments

  • 2 body data sheet.docx
    83 KB · Views: 148

1. What is orbital mechanics?

Orbital mechanics is a branch of classical mechanics that deals with the motion of objects in outer space, particularly how objects move and interact in orbit around a larger celestial body such as a planet.

2. What are the equations of motion used in orbital mechanics?

The most commonly used equations of motion in orbital mechanics are the Newton's second law of motion, Kepler's laws of planetary motion, and the gravitational force equation. These equations can be used to calculate the position, velocity, and acceleration of an object in orbit.

3. What are initial conditions in orbital mechanics?

Initial conditions refer to the initial position and velocity of an object in orbit at a given point in time. These values are essential in calculating the future motion of the object using the equations of motion.

4. How do you find the equations of motion with initial conditions in orbital mechanics?

To find the equations of motion with initial conditions, you will need to use the initial position and velocity values to solve for the constants in the equations of motion. Once the constants are determined, you can use the equations to calculate the position, velocity, and acceleration of the object at any point in time.

5. What is the importance of understanding orbital mechanics?

Understanding orbital mechanics is crucial in space exploration and satellite technology. It allows us to predict and control the motion of objects in orbit, which is essential in launching and maneuvering satellites, spacecraft, and other objects in space. Understanding orbital mechanics also helps us study and understand the motion of celestial bodies in our solar system and beyond.

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