Satellite Motion conceptual problem

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Discussion Overview

The discussion revolves around the conceptual understanding of satellite motion, particularly the conditions required for an object to achieve stable orbit around the Earth. Participants explore the implications of gravitational curvature and the limitations of using flat Earth approximations in orbital mechanics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant expresses confusion about the falling distance of an object in motion relative to the curvature of the Earth, questioning the application of flat Earth calculations to a spherical Earth.
  • Another participant suggests that the assumption of a constant gravitational field is incorrect for larger distances and proposes a better approach involving centripetal acceleration.
  • A different viewpoint emphasizes that the parabolic motion can be considered for short distances but warns against applying it to orbital mechanics without accounting for the Earth's curvature.
  • Some participants discuss the need for a formula to calculate the normal distance from a tangent line to a circle, indicating a shift towards more technical mathematical considerations.
  • There are references to specific formulas for calculating distances related to circular motion, with some participants noting simplifications and corrections to earlier statements.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the appropriateness of using flat Earth approximations for understanding satellite motion. Multiple competing views remain regarding the correct approach to orbital mechanics and the implications of gravitational curvature.

Contextual Notes

Limitations include the dependence on assumptions about gravitational uniformity and the applicability of parabolic motion to orbital dynamics. The discussion highlights unresolved mathematical steps and the complexity of accurately modeling satellite motion.

godingly
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Hey Dear forum,
I know I'm wrong, but I don't know why:

Since the Earth's descends 5 meters for every 8km, a horizontal speed of 8km/sec will put an object to rotate around the Earth (neglecting air resistance). I.e. in one second it will fall 5m below it's initial height, but so will the earth. But by the simple formula S = V_{o}t + \frac{at^{2}}{2} by the 2^{nd} second it suppose to descend 20 meters from its original height - but the Earth would only curve by 10 (5*2)! Which means during the 1st and 2nd second it will crash into Earth!

What is my mistake?
 
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Your mistake is in your assumption that the field of gravity has a constant direction while the object travels. That is approximately correct for short distances, but you are trying to use the approximation for larger distances.

A better approach is through asking the following question: what velocity must an object have to rotate circularly with radius equal to that of the Earth and centripetal acceleration equal to the acceleration of gravity at the surface of the Earth.
 
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godingly said:
...but the Earth would only curve by 10 (5*2)!

What is my mistake?

That. Relative to your starting position, the Earth curves approximately 5 * 22 m in 16 km. Draw a diagram of the arc of a circle and a line tangent to it.

Or, as Volo said, if you want to consider each interval separately, you have to remember that "downwards" always points towards the center of the earth, so it is in a different direction in the two intervals.
 
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godingly said:
Hey Dear forum,
I know I'm wrong, but I don't know why:

Since the Earth's descends 5 meters for every 8km, a horizontal speed of 8km/sec will put an object to rotate around the Earth (neglecting air resistance). I.e. in one second it will fall 5m below it's initial height, but so will the earth. But by the simple formula S = V_{o}t + \frac{at^{2}}{2} by the 2^{nd} second it suppose to descend 20 meters from its original height - but the Earth would only curve by 10 (5*2)! Which means during the 1st and 2nd second it will crash into Earth!

What is my mistake?

You appear to be trying to impose 'flat Earth' calculations on a spherical earth, here. The parabola equation only works properly for a uniform g field over a horizontal surface. I could take you a little way over the horizon before it fails but it definitely isn't the way to approach Orbital mechanics.

To work out that, you need to look into the force need to produce circular motion. That force is a 'central attractor' and is provided by gravity, which follows the inverse square law. The 'book work' that shows you what's what can be found in many places. To maintain a particular altitude of orbit, you need to be traveling at a certain speed, which will require a particular centripetal force (equal to the g force at that height).
The guys on Hyperphysics are pretty good as a source of this sort of basic theory.
 
The parabola is fine to consider the first few seconds - the important point is the quadratic deviation from a flat surface. 5m in 8km imply 20m in 16km, not 10.
 
mfb said:
The parabola is fine to consider the first few seconds - the important point is the quadratic deviation from a flat surface. 5m in 8km imply 20m in 16km, not 10.

Maybe but when the title of the thread includes the word 'satellite', a flat Earth / parabolic approximation is hardly the right thing.
The introductory animation, showing a gun firing a shell horizontally with progressively higher and higher velocity until an orbit is achieved, is fine but not if anyone wants to assume parabolic motion.

With or without an arithmetical mistake, the quantitative approach is a bit too flawed to make it worth while, imo. Arm waving about it is fine.
 
Thank you all for the answers! For mfb and alephzero - is there a formula to calculate the perpendicular (normal) distance from a point on a tangent line to the circle? When I say normal, I mean 90 degrees at the tangent line, not at the circle.
 
That Hyperphysics link?
 
The formula is $$ h = r \left(\sqrt {1 + \tan^2 \frac s r} - 1\right), $$ where ##r## is the radius, and ##s## is the arc distance.
 
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Or $$h = r\left(\frac{1}{\cos{\dfrac s r}} - 1\right)$$ which is fewer buttons to push on most calculators.

Note, in this and Volo's formula, the trig functions use radians not degrees.

Or if ##s## is small relative to ##r##, approximately $$\frac{s^2}{2r}$$
 
  • #11
AlephZero said:
$$h = r\left(\frac{1}{\cos{\dfrac s r}} - 1\right)$$

I missed an obvious simplification, dammit!
 
  • #12
godingly said:
Thank you all for the answers! For mfb and alephzero - is there a formula to calculate the perpendicular (normal) distance from a point on a tangent line to the circle? When I say normal, I mean 90 degrees at the tangent line, not at the circle.

The shape of the curve that's followed is an ellipse - just as with all orbits. The ellipse will pass through the Earth if the velocity isn't right. Needless to say, if you take off from a point on the Earth's surface (the highest mountain you could find), the 'successful' orbit (neglecting gravity), will actually be a circle (special case of an ellipse) and will take the shell round and it will hit you in the back of the head after about 90 minutes.
 

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