What Is the Gravitational Quadrupole Moment of a Homogeneous Ellipsoid?

In summary, the surface of a homogeneous body with mass m is described by the ellipsoid (x/a)^2 + (y/b)^2 + (z/c)^2 = 1 with a, b, c > 0. To find the gravitational quadrupole moment dyadic of this body, one can use the equation Q = ∫ρ(r)(3r.r-r^2.1) dr, where 1 is the unit dyadic. However, this formula does not provide any hints on how to apply it. Alternatively, one can use Legendre polynomials to solve the problem and expand the answer into a 3 x 3 matrix. The integral can be evaluated using ellipsoidal coordinates, even though it
  • #1
Osman123
2
0

Homework Statement



The surface of a homogeneous body of mass m is the ellipsoid
(x/a)^2 + (y/b)^2 + (z/c)^2 = 1 with a,b,c>0.

What is the gravitational quadrupole moment dyadic of this body?


Homework Equations



This is my first confusion: what is the right equation?

In my Clssical Mechanics lect notes, it says

Q = ∫[itex]\rho[/itex](r)(3r.r-r^2.1) dr

where 1 is the unit dyadic. But there is no hint on how to apply this formula!

The Attempt at a Solution



Since I am concurrently doing EM, I remember using Legendre polynomials to solve both electric/magnetic quadrupole expansion-type question. So the question is, is it a must to use that weird integral in 2. above or can the answer be obtained using Legendre polynomials and somehow expanded into a 3 * 3 matrix?

Thank you very much in advance!

P.S. also I usually solve my doubts by browsing online, but on gravitational quadrupole moment I can't find any links at all that show how to do the integration. What should I search under? GR? Or something else. Thanks once again.
 
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  • #2
You don't need GR or anything the like. All you need is to calculate that integral over the volume of the ellipsoid. As the ellipsoid is homogenous the mass density is just a constant.
So calculate that integral over an ellipsoid which is an exercise of vector analysis. I would suggest switching to ellipsoidal coordinates. It's pretty ugly...
 

FAQ: What Is the Gravitational Quadrupole Moment of a Homogeneous Ellipsoid?

What is the gravitational quadrupole moment?

The gravitational quadrupole moment is a measure of the distribution of mass in a system that produces a gravitational field. It is a mathematical quantity that describes the shape and orientation of the mass distribution, and is related to the strength of the gravitational field.

How is the gravitational quadrupole moment different from the monopole and dipole moments?

The gravitational monopole moment represents the total mass of a system, while the dipole moment represents the asymmetry in the mass distribution. The quadrupole moment is a more complex measure of the distribution of mass, taking into account the shape and orientation of the mass distribution, and is important for understanding the strength and direction of gravitational forces.

How is the gravitational quadrupole moment calculated?

The gravitational quadrupole moment can be calculated using integrals of the mass distribution over space. It is expressed as a tensor, which is a mathematical object that describes the magnitude and direction of a physical quantity. The specific formula for calculating the quadrupole moment depends on the shape and orientation of the mass distribution.

What is the significance of the gravitational quadrupole moment?

The gravitational quadrupole moment is important for understanding the gravitational interactions between massive objects, such as planets, stars, and galaxies. It can also provide insights into the internal structure and dynamics of these objects. In astrophysics, the quadrupole moment is used to study phenomena like gravitational waves and the rotation of celestial bodies.

How is the gravitational quadrupole moment related to general relativity?

In the theory of general relativity, the gravitational quadrupole moment is one of the multipole moments that can be used to describe the curvature of space-time caused by a massive object. It is a key factor in the equations of general relativity and is used to explain various phenomena, such as the bending of light by massive objects and the precession of orbits.

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