The spherical symmetry of massive bodies

In summary, when studying the motion of a two-body system with only gravitational forces, the presence of non-spherical symmetry in one or both of the bodies can complicate the process. While a "brute force" numerical integration method can be used, it may not be feasible in all situations. Approximations and assumptions may be made for smaller, artificial satellite bodies, but for more precise astronomical calculations, the non-symmetry of bodies must be taken into account.
  • #1
rob60
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Homework Statement



Consider the study of the motion of a two bodies system interacting with only gravitational forces.
If the two bodies (or even one of them) has not spherical symmetry, how will you proceed? Indeed the Earth and the moon does not have spherical symmetry mass distributions but normally we consider them as..
thank you



Homework Equations





The Attempt at a Solution



 
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  • #2
If one of the masses is spherical, you can easily find its gravitational field. Then you place the non-spherical mass in that field and do a numerical integration to find the net force on it. If the first mass is not spherical, then you first need to do a numerical integration to find its gravitational field.

This "brute force" method will work with any mass and requires no approximations or assumptions. It basically calculates the net force between the two masses by adding over all possible pairs dm1 and dm2.
 
  • #3
Thank you, I've understand.
It is true that if the body is small enough it can be considered set in a field of parallel forces (with obvious and simple results) but this is an approximation that works fine, i think, for artificial satellites and for the bodies on a 'human scale'.
In astronomical calculations on the motions of planets and satellites, however, I wonder how it is take in account the 'non-symmetry' of bodies.
Do you know any reference?
 

Related to The spherical symmetry of massive bodies

1. What is spherical symmetry?

Spherical symmetry is a concept in physics and mathematics that describes objects or systems that are symmetrical in all directions around a central point, resulting in a spherical shape.

2. How does spherical symmetry apply to massive bodies?

Spherical symmetry is commonly observed in massive bodies, such as planets, stars, and galaxies. This is because their large size and gravitational forces cause them to collapse into a nearly spherical shape due to the equal distribution of mass in all directions.

3. What are the implications of spherical symmetry in astrophysics?

The spherical symmetry of massive bodies allows for simplified mathematical models and calculations in astrophysics. It also helps us understand the behavior and properties of these bodies, such as their gravitational pull and orbital motion.

4. Are there any exceptions to spherical symmetry in massive bodies?

While most massive bodies exhibit spherical symmetry, there are some exceptions. For example, binary star systems may have an elliptical or irregular shape due to their mutual gravitational forces. Additionally, the rotation of a massive body can also cause it to deviate from perfect spherical symmetry.

5. How do scientists study and measure spherical symmetry in massive bodies?

Scientists use various methods, such as observations from telescopes and satellites, to study and measure the spherical symmetry of massive bodies. They also use mathematical models and simulations to understand the effects of spherical symmetry on the behavior of these bodies.

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