Calculate foci of planetary orbit given known parameters

In summary, the focal points can be calculated using the eccentricity and semi-major axis of the orbit, which can be determined from the total mechanical energy and angular momentum of the system.
  • #1
CarlosMarti12
8
0
Hello everyone. I am trying to calculate the focal points of the ellipse traced by a planet in orbit around a star, given the following known parameters:
  • [itex]M_{sun}[/itex] Mass of the sun
  • [itex]r_{planet}[/itex] Position vector of the planet from the sun
  • [itex]m_{planet}[/itex] Mass of the planet
  • [itex]v_{planet}[/itex] Velocity of the planet
  • [itex]G[/itex] Gravitational constant
  • [itex]F_{grav} = G\frac{Mm}{r^{2}}[/itex]

I would like to find (if possible) the orbital information of the planet (including eccentricity, focal points, and axes, if possible) based on these pieces of data. Is it possible to calculate the focal points of its orbit based on these parameters? If more parameters are necessary, I might be able to add them. Any help would be greatly appreciated! (The focal points of an ellipse are shown below.)

256px-Ellipse_with_focus.svg.png
 
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  • #2
Focal Points: (c, 0), (-c, 0)Where c is the distance between the two focal points.Yes, it is indeed possible to calculate the focal points of the ellipse given the above parameters. The eccentricity of an orbit can be calculated from the following equation:e = \sqrt{1 + \frac{2EL^{2}}{m_{planet}G M_{sun}}Where E is the total mechanical energy of the system and L is the angular momentum of the planet.Once the eccentricity is known, the focal points can be calculated using the following formula:c = a\sqrt{1 - e^{2}}Where a is the semi-major axis of the orbit.The semi-major axis is given by the equation:a = \frac{r_{planet}v^{2}}{G M_{sun}}Combining all these equations, we get:c = \frac{r_{planet}v^{2}}{G M_{sun}}\sqrt{1 - \left(1 + \frac{2EL^{2}}{m_{planet}G M_{sun}}\right)^{2}}Therefore, given the parameters specified in the question, it is possible to calculate the focal points of the ellipse traced by the planet in its orbit around the star.
 

1. What are the key parameters needed to calculate the foci of a planetary orbit?

The key parameters needed to calculate the foci of a planetary orbit are the semi-major axis, eccentricity, and the mass of the central body (usually a star). These parameters can be obtained from observations or measurements of the planet's orbit.

2. How do you calculate the foci of a planetary orbit?

The foci of a planetary orbit can be calculated using the following formula:
F = a * e
Where F is the distance from the center of the ellipse to the foci, a is the semi-major axis, and e is the eccentricity.

3. What is the significance of the foci in a planetary orbit?

The foci of a planetary orbit represent the two points in the orbit where the gravitational force from the central body is strongest. They are also important in determining the shape and orientation of the orbit.

4. Can the foci of a planetary orbit change over time?

Yes, the foci of a planetary orbit can change over time due to gravitational interactions with other objects in the solar system or external forces acting on the planet. However, these changes are usually very small and can only be observed over long periods of time.

5. How do the foci of a planetary orbit affect the planet's motion?

The foci of a planetary orbit play a crucial role in determining the planet's motion. The planet will always move in an elliptical path around the central body, with the foci as the two focal points. The distance between the foci also affects the speed of the planet, with the planet moving fastest when it is closest to the foci.

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