Astronomy: Orbit Terminology

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SUMMARY

The discussion clarifies the terminology used to describe orbital directions, specifically distinguishing between prograde, retrograde, and posigrade motions relative to the body being orbited. Prograde and retrograde describe orbits based on the rotation direction of the central body, but these terms become ambiguous for non-rotating bodies like tidally locked moons. The term "posigrade" is introduced as a precise descriptor for a spacecraft's heading aligned with the orbital velocity vector, while "retrograde" refers to the opposite direction. Additional terminology such as R-bar, V-bar, and H-bar vectors are used for relative approach and departure maneuvers in close-proximity orbital operations, such as docking with the ISS. The discussion also highlights practical delta-v constraints that influence the feasibility of leaving orbit in prograde versus retrograde directions.

PREREQUISITES

  • Orbital Mechanics: Prograde and Retrograde Orbit Definitions
  • Celestial Body Rotation and Tidal Locking Concepts
  • Spacecraft Maneuvering: Hohmann Transfers and Delta-V Budgeting
  • Relative Orbital Coordinate Systems: R-bar, V-bar, H-bar Vectors

NEXT STEPS

  • Study Posigrade and Retrograde Burn Maneuvers in Orbital Transfers
  • Explore R-bar, V-bar, and H-bar Coordinate Systems for Rendezvous Operations
  • Analyze Delta-V Requirements for Orbit Escape in Prograde vs Retrograde Directions
  • Investigate Orbital Inclination Effects on Prograde and Retrograde Orbit Classification

USEFUL FOR

Space mission planners, aerospace engineers, orbital mechanics students, and spacecraft operators engaged in trajectory design, orbital rendezvous, and mission planning involving complex orbital maneuvers and escape trajectories.

  • #31
The trouble is if you look at the earth from above the north pole then counterclockwise, from above the south pole clockwise. Same with the solar system.
 
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  • #32
Hornbein said:
The trouble is if you look at the earth from above the north pole then counterclockwise, from above the south pole clockwise. Same with the solar system.
Yet, the right-hand rule provides an unambiguous direction towards the rotational north pole. This isn't as much of a problem as you make it out to be.
 
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  • #33
Bandersnatch said:
Yet, the right-hand rule provides an unambiguous direction towards the rotational north pole. This isn't as much of a problem as you make it out to be.
But then all heavenly bodies rotate counterclockwise. Is that useful?
 
  • #34
Hornbein said:
But then all heavenly bodies rotate counterclockwise. Is that useful?
Why wouldn't it be? The direction of the pseudovector in whatever reference frame we pick provides all the information about the direction of the rotation, and one is still free to describe rotation of bodies in relative terms using words like clockwise/anticlockwise.

The point is to remove ambiguity from statements like 'Venus rotates clockwise when viewed from the North pole of the invariable plane of the solar system'.

And in any case, if it's good enough for the IAU, it's maybe good enough for us.
 
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  • #35
Bandersnatch said:
The point is to remove ambiguity from statements like 'Venus rotates clockwise when viewed from the North pole of the invariable plane of the solar system'.
All you can do is compare the rotational or orbital planes of two heavenly bodies and conclude that their rotational direction is either the same or differs. In the case of Uranus this does not work, as the planes are perpendicular.
 
  • #36
Hornbein said:
All you can do is compare the rotational or orbital planes of two heavenly bodies and conclude that their rotational direction is either the same or differs.
I'm not sure why you're framing this as an objection. Yes, that's what you do, and that's what makes it unambiguous.
Wasn't the perceived ambiguity in picking the reference 'north' direction from which to judge the rotation the point you initially took issue with? We may be talking at cross purposes here.

As for Uranus. It's plane of rotation is not exactly perpendicular to the invariant plane, or any other obvious reference frame you may pick, be it solar equatorial plane, or the ecliptic. The few degrees of deviation from perpendicularity lets you say that when its rotation vector points below the plane, i.e. towards the southern hemisphere of the reference - that's clockwise rotation. Above that plane - anticlockwise.
 
  • #37
Pixelworks said:
how is the prograde or retrograde direction determined if the body in question is not rotating?
IMO this thread has taken us down a rabbit hole. The apparent magic of the retrograde orbit of Mars was a huge stumbling block for the Geocentric Universe model. Several hundred years ago, the Heliocentric model solved the 'anomaly. The term "retrograde" its really pretty irrelevant now. because celestial objects go as you'd expect and they are (afaik) consistent.
It does have a place when discussing some situations, though. When placing a craft in lunar orbit, it is less costly in energy if you choose a 'figure of eight' with retrograde lunar path because the net orbital energy change is a lot less than if you went for a prograde lunar orbit. You would need a huge retro thrust to get the ship to slow down enough to be captured into a lunar orbit of the same sense as its orbit round the Earth (which is there all the time when hooked on to the Moon).
1776783255376.webp
 
  • #38
Pixelworks said:
how is the prograde or retrograde direction determined if the body in question is not rotating?
IMO this thread has taken us down a rabbit hole. The apparent magic of the retrograde orbit of Mars was a huge stumbling block for the Geocentric Universe model. Several hundred years ago, the Heliocentric model solved the 'anomaly. The term "retrograde" its really pretty irrelevant now.
It does have a place when discussing some situations, though. When placing a craft in lunar orbit, it is less costly in energy if you choose a 'figure of eight' path because the net orbital energy change is a lot less. You would need a huge retro thrust to get the ship to slow down enough to be captured into a lunar orbit of the same sense as its orbit round the Earth (which is there all the time when hooked on to the Moon).
View attachment 371084
 
  • #39
sophiecentaur said:
The apparent magic of the retrograde orbit of Mars was...
You're thinking of 'apparent retrograde motion', on the celestial sphere. Where this thread talks about retrograde, it's in the context of directions of orbits. A different thing.
 
  • #40
Bandersnatch said:
You're thinking of 'apparent retrograde motion', on the celestial sphere. Where this thread talks about retrograde, it's in the context of directions of orbits. A different thing.
I take your point but why would there her any significance in this? In an early solar system there would have been a mix of small objects with an assortment of angular momenta; only a small majority being one way. Collisions and partial captures would end up producing a mature solar system with most large objects with prograde orbits.

The same set of interactions would produce a disc shaped system with an angular momentum vector more or less the same a that of the original cloud.
 
  • #41
sophiecentaur said:
I take your point but why would there her any significance in this?
I suppose the significance could manifest when you're in a spaceship and Houston tells you to rotate the craft for a retrograde burn. It might be nice to know what they're talking about.
And in any case, it's the context the OP asked about.
 
  • #42
Bandersnatch said:
rotate the craft for a retrograde burn.
Maybe but most navigation instructions tend to be numerical - eg Heading and thrust. "Rotating the craft " would not be sufficient and they have to get it right. But I have never driven one of those things so don't listen to me.
Edit: Then again; if you were in a polar orbit, which would ground control tell you to do? It's like the old problem when people insist on using acceleration and deceleration when the variable acceleration would have a sign. It's hard to do calculations with signless variables.
 
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