Gravitational Warping by Non-Spherical Celestial Bodies

In summary, if there were very massive celestial bodies which were not spherical, the geodesical paths around them would not be elliptical and the orbits would be affected by the stress-energy tensor. This means that objects would follow non-elliptical paths and the gravitational warping would be mainly Newtonian rather than relativistic.
  • #1
Gerinski
323
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Purely theoretically, if there were very massive celestial bodies which were not spherical, how would their gravitational warping be? Which shapes would the geodesical paths around them have? Would they still be elliptical orbits or would they have sudden changes of direction?
Say for example, a huge massive cube, or huge a pyramid, a rod or a giant horseshoe? If a freefalling object would approach those and fall into orbit, which kind of path would it follow?
 
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  • #2
In the examples you're describing, the main effect would be Newtonian, not relativistic. The orbits would of course not be elliptical. A less extreme example is that part of the perihelion precession of Mercury is due to the sun's oblateness.

Relativistically, the gravitational field is produced not just by the mass but by the stress-energy tensor, so it also depends on things like the pressure and shear stresses.
 

FAQ: Gravitational Warping by Non-Spherical Celestial Bodies

What is gravitational warping by non-spherical celestial bodies?

Gravitational warping is the phenomenon where the gravitational pull of a non-spherical celestial body, such as a planet or star, causes a distortion in the surrounding space-time. This distortion can affect the trajectory of objects passing by the celestial body.

How does the shape of a celestial body affect its gravitational warping?

The shape of a celestial body plays a significant role in its gravitational warping. The more asymmetrical or non-spherical a body is, the greater its warping effect on space-time will be. This is because the distribution of mass in a non-spherical body is uneven, resulting in varying gravitational forces.

Can gravitational warping by non-spherical celestial bodies be observed?

Yes, gravitational warping has been observed and measured in various astrophysical phenomena, such as the bending of light from distant stars and the orbital paths of planets around a non-spherical star. These observations provide evidence for the existence of gravitational warping by non-spherical celestial bodies.

Are there any practical applications of studying gravitational warping by non-spherical celestial bodies?

Studying gravitational warping by non-spherical celestial bodies can help us understand the dynamics of the universe and how it evolves over time. It also has practical applications in space travel and navigation, as knowing the warping effects of large celestial bodies can help us plan more efficient trajectories.

Can the warping effects of non-spherical celestial bodies be used to create artificial gravity?

While the warping effects of non-spherical celestial bodies can create a gravitational pull, it is not strong enough to create artificial gravity. The gravity created by non-spherical celestial bodies is still significantly weaker than the force of gravity on Earth, making it impractical for creating artificial gravity for space stations or spacecraft.

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