Derive the terrestrial equation of motion in the body-fixed frame

In summary, the conversation revolves around deriving the terrestrial equations of motion by using Newton's laws in a body-fixed frame with the origin at the surface of the earth. This involves assuming that the center of mass of the Earth moves at a constant velocity with respect to fixed stars and that the angular velocity of the Earth is also constant. The equations involve using the coordinates of a particle in both the inertial and body-fixed frame, with the origin of the body-fixed frame at a point with respect to the inertial frame. The starting point is \mathbf{F}=m\mathbf{A} in the inertial frame.
  • #1
richyw
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Homework Statement



Assume that the center of mass of the Earth moves with approximately constant velocity with respect to the fixed stars, and that [itex]\mathbf{\omega}[/itex], the angular velocity of the earth, is constant. Rederive the terrestrial equations of motion
[tex]\mathbf{F}'+m\mathbf{g}[/tex][tex]m\ddot{\mathbf{r}}-2m\mathbf{\omega}\times\dot{\mathbf{r}}[/tex]
By writing Newton's laws in a body-fixed frame with the origin at the surface of the earth.

Homework Equations



For a particle with coordinates [itex]\mathbf{r}_0[/itex] in the inertial frame and [itex]\mathbf{r}[/itex] in the body-fixed frame, where the origin of the body fixed frame is at the instantaneous point [itex]\mathbf{a}[/itex] with respect to the inertial frame.
[tex]\mathbf{r}_0 = \mathbf{a}+\mathbf{r}[/tex]

The Attempt at a Solution



I'm pretty confused on where to start here. I know that in the inertial frame [itex]\mathbf{F}=m\mathbf{A}[/itex]. Could anyone help get me started, or point me towards some literature on this?
 
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  • #2
wait I think I just arrived at the first equation.
 

1. What is the terrestrial equation of motion in the body-fixed frame?

The terrestrial equation of motion in the body-fixed frame is a mathematical expression that describes the motion of a body on the surface of the Earth, taking into account the rotation and curvature of the Earth. It is derived from Newton's second law of motion and is used to analyze the dynamics of objects in terrestrial environments.

2. How is the terrestrial equation of motion derived?

The terrestrial equation of motion is derived by considering the forces acting on a body, including gravitational, inertial, and surface forces, and using the principles of Newton's second law of motion. The resulting equation takes into account the Earth's rotation and curvature, and is expressed in terms of the body's position, velocity, and acceleration in the Earth's frame of reference.

3. What is the significance of using the body-fixed frame in the terrestrial equation of motion?

The body-fixed frame is a coordinate system that is fixed to a body and rotates with it, making it a useful frame of reference for studying the motion of that body. In the case of the terrestrial equation of motion, using the body-fixed frame allows for a more accurate analysis of the motion of objects on the Earth's surface, as it takes into account the Earth's rotation and curvature.

4. Can the terrestrial equation of motion be used to study the motion of objects in other environments?

Yes, the terrestrial equation of motion can be adapted to study the motion of objects in other environments, such as other planets or moons. However, it may need to be modified to account for the specific gravitational and surface forces present in those environments.

5. How is the terrestrial equation of motion used in practical applications?

The terrestrial equation of motion is used in a variety of practical applications, such as predicting the trajectory of projectiles, analyzing the flight of aircraft, and designing vehicles for optimal performance on the Earth's surface. It is also used in the fields of geodesy and geophysics to study the Earth's shape and rotation.

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