Planetary Orbits - Elliptical or Wavelike?

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Discussion Overview

The discussion revolves around the nature of planetary orbits, specifically whether they can be described as elliptical or wavelike in different reference frames. Participants explore the implications of varying velocities and reference frames on the perceived motion of celestial bodies, including simulations and theoretical constructs.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant describes a simulation where orbits appear wavelike when the Sun reaches a relative speed of 70 km/s to a black hole, questioning if such descriptions are common in physics.
  • Another participant suggests that orbits can be described in any reference frame, but questions the necessity of complicating the description beyond elliptical orbits.
  • It is noted that orbits can appear spiral-like in frames moving linearly with respect to the barycenter, particularly when speeds exceed those of the innermost planets.
  • A participant introduces the idea that adding linear motion to circular motion can result in wiggly paths, referencing parametric equations.
  • Mercury's orbit is compared to a cycloid, with speculation about reference frames where this might be exact.
  • Some participants discuss the possibility of seeing the Earth at rest in certain frames, with one suggesting it could appear at rest for an entire year.
  • A thought experiment involving cameras and rigid rods is presented, questioning the nature of acceleration and motion in different frames.
  • Another participant emphasizes that it is trivial to choose a point of view where a moving object appears to come to rest, raising questions about the implications of such a perspective.
  • One participant notes that the discussion includes a reference to a PBS Space Time video, suggesting relevance to the topic.

Areas of Agreement / Disagreement

Participants express a range of views on the nature of orbits and reference frames, with no clear consensus on whether orbits can be universally described as wavelike or if elliptical descriptions are sufficient. The discussion remains unresolved with multiple competing perspectives.

Contextual Notes

The discussion includes assumptions about reference frames and the nature of motion, with some participants acknowledging limitations in their thought experiments, such as the non-existence of rigid rods.

Devin-M
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I was running a simulation in Universe Sandbox where I placed a 10 million solar mass black hole about 10 light years from the Solar System, initially stationary relative to the Sun. I noticed once the Sun had reached about 70km/s relative to the black hole, all the orbits became wavelike rather than elliptical. Are orbits ever studied or described in a reference frame where they are linear or wavelike rather than elliptical?

Here's a video:
 
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Devin-M said:
Are orbits every studied or described in a reference frame where they are linear or wavelike rather than elliptical?
I mean, you can? You are free to use any reference frame whatsoever.
I can't think of a reason to complicate the description like that, though. Normally you'd try to make things as simple as possible for yourself.

Devin-M said:
I noticed once the Sun had reached about 70km/s relative to the black hole, all the orbits became wavelike rather than elliptical.
They'll be spiral-like in any frame moving linearly w/r to the barycentre. If they look more wavy to you above certain speed is just due to exceeding the orbital speeds of even the innermost planets - the spirals get stretched enough that all the planets seem to always move more sideways in one direction, than up and down or backwards.
 
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The parametric equations of a circle are x = cosine and y = sine. Toss substantial linear or near-linear motion on top of that, perhaps from choice of reference frame, and of course you get wiggly lines.
 
Mercury’s path looks very similar to a cycloid. I wonder if there are some reference frames where it’s exact.
 
In any frame moving parallel to the plane of the orbit, with velocity w/r to the barycentre equal to its orbital velocity.

(with the caveat that it can be perfect only for exactly circular orbits)
 
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So from a certain frame you could see the Earth come to a rest once per year.
 
Well, from a certain frame you can see it at rest the entire year...
 
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Here's Earth on a 1AU Cycloid Orbit:
 
Suppose I have 2 de-rotated cameras attached by a rigid rod, one mounted at the center of the Earth, the other in deep space where the sun’s gravitational influence is negligible. The rod passes through and is fixed to the geographical north pole. Next I detach the deep space camera from the rod. If I understand correctly, neither camera will detect any acceleration, but one camera sees the Earth at rest year round and the other camera sees the Earth move along a cycloid path and come to a rest once per year on the anniversary of being detached. The only problem is rigid rods don’t exist.
 
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  • #10
Yes. At the risk of generalizing, it is universally and trivially possible to choose a point of view in 3D space wherein a given circularly- (or helically-)moving object is seen to come to rest at some point. Operative word: trivial. IOW, it doesn't imply any underlying principle, simply that which you choose to assign to your chosen POV.

An exercise for the reader: when we say "come to rest" do we mean actually come to rest in a 3-D coordinate system? Or simply appear to come to rest ... when viewed in the 2-D coordinate system of a screen render?

Devin-M said:
The only problem is rigid rods don’t exist.
Isn't this a thought experiment? You don't need a real rigid rod!
 
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  • #11
This was recently posted from PBS Space Time. 'Figured it's sort of relevant for this thread.

 
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