Coriolis effect and relativity

In summary, the Special Principle of Relativity states that all physical laws are in agreement among inertial frames, but this does not apply when one observer is experiencing an acceleration. Rotating frames are not inertial, so it is possible to tell if you are rotating by observing the coriolis effect. This shows that the principle does not apply to rotation, as it involves changing velocity and is considered an acceleration.
  • #1
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With my fairly sketchy knowledge of relativity, one of the basic assumptions is that you can't tell who's point of view is right, with regards to how thing are moving. But, in the case of rotation, isn't it possible to tell if you are rotating by observing the coriolis effect?
For instance, when a rocket is launched, it seems to curve as we rotate away from it, but it wouldn't do this if we were not rotating. Surely this shows that we are rotating.
Does the 'not knowing who is moving' rule apply to rotation, or does this somehow not violate it? Thanks.
 
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  • #2
As you have hopefully guessed already, the existence of the coriolis force isn't proof that the Special Principle of Relativity is wrong. When one follows a curve, you are experiencing a force - and an acceleration:

[tex]a=\frac{v^2}{r}[/tex].

The special principle of relativity states that all physical laws are in agreement amoungst all intertial frames, so does not apply when one observer is experiencing an acceleration.

Have a look at:

http://en.wikipedia.org/wiki/Inertial_frame
 
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  • #3
is that you can't tell who's point of view is right, with regards to how thing are moving.

In the case on inertial observers, everyone is right and you can choose a frame to suit your convenience. But rotating frames are not inertial. So if you were spinning on a roundabout, you could tell you are rotating from the forces you feel and measure. Other observers would also agree that you are rotating.

simultaneous with the above - fasterthanjoao you can correct your tex by changing the [ \ tex ] to [ / tex ]
 
  • #4
Rotation, even at constant speed, involves changing velocity and is an acceleration so not inertial.
 
  • #5
Alright, thanks a lot.
 

Related to Coriolis effect and relativity

What is the Coriolis effect?

The Coriolis effect is a phenomenon in which an object moving in a straight line appears to curve due to the rotation of the Earth. It is caused by the conservation of angular momentum, which states that an object will maintain its direction and speed unless acted upon by an external force.

How does the Coriolis effect affect weather patterns?

The Coriolis effect plays a significant role in the formation of weather patterns. In the Northern Hemisphere, winds and ocean currents are deflected to the right due to the Earth's rotation, while in the Southern Hemisphere, they are deflected to the left. This creates large-scale circulation patterns that influence global weather systems.

What is the difference between Coriolis effect and centrifugal force?

Coriolis effect and centrifugal force are often confused, but they are two distinct phenomena. The Coriolis effect is the apparent deflection of objects due to the Earth's rotation, while centrifugal force is the outward force experienced by objects due to their circular motion. Centrifugal force is a result of inertia, while the Coriolis effect is a result of the conservation of angular momentum.

How does Einstein's theory of relativity relate to the Coriolis effect?

Einstein's theory of relativity states that the laws of physics are the same for all observers, regardless of their relative motion. This means that the Coriolis effect will be observed by all observers, regardless of their position or motion on the Earth. Additionally, relativity helps to explain the small discrepancies in the Coriolis effect between different latitudes due to the Earth's oblateness.

Can the Coriolis effect be observed on other planets?

Yes, the Coriolis effect can be observed on any rotating object, not just the Earth. It has been observed on other planets, such as Mars, and even on larger scales, such as in the rotation of galaxies. However, the strength of the effect will vary depending on the size and rotation rate of the object.

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