I need some support, please, for a gravity assist analysis

[Dale]

No matter what, an interaction between two solid bodies can never result in the system gaining energy

The system doesn’t gain energy. The system doesn’t even gain kinetic energy. That is built into the elastic collision equations.

Kinetic energy does transfer from one object to the other.

Changing to a different frame of reference never has any effect whatsoever to the internal energy of any system.

Changing to a different frame of reference does change the kinetic energy.

Not exactly true.

100% exactly true. This is the principle of relativity. Are you denying the principle of relativity? It is a bedrock of physics.

Measuring the velocity of the planet, the probe sees it alternately slowing momentarily to a dead stop and then speeding up to a peak of 20 Km/s. The measurements are perfectly correct, but it does not mean the planet is somehow loosing energy and then gaining it back. It is never gaining or losing energy at all.

In the frame of the probe the planet is indeed gaining and losing KE. KE is $KE=\frac{1}{2}mv^2$. As $v^2$ changes so does KE.

In a gravity assist, the two smaller bodies ARE ineslatic in the FoR of the planetary barycenter

No. You did not provide a reference for this false claim. Again, treating a gravitational assist as an elastic collision is well established in the professional scientific literature. This claim is closed unless you provide specific peer reviewed literature references to the contrary

 

[jbriggs444]

Total kinetic energy depends on the frame of reference. That's for sure. Work however remains constant. Or at least that's how I recall it from the last time I had to derive it for a similar conversation regarding elastic collisions.

The work done by one object on another is not invariant. It depends on the choice of reference frame.

However, you are correct that the total of the work done by A on B plus the work done by B on A is an invariant. For an elastic collision, that total will be zero. This fact is irrelevant for the argument you proceed to make.

If two bodies interact gravitationally with each other, the orbits will be either elliptical or hyperbolic depending of the initial velocities of the bodies. We previously agreed the reference frame at the CoM between the two seems to be very useful so I will keep using that one during the discussion.

View attachment 329334

Before (black line) and after (green) flyby the kinetic energies of the bodies are the same. Do we agree on this?

The before and after kinetic energies of a given body are identical using the CoM frame. [Assuming some symmetry on where the two measurements are taken within the eccentric elliptical orbits shown in the illustration] Yes. we agree.

If they are the same, no work has been transferred.

Yes, we agree.

No matter the reference frame chosen, that will remain true.

No. That is not correct. The work done by one object on another is not an invariant.

 

[weirdoguy]

Work however remains constant.

It doesn't have to, since it's line integral of force it depends on the path which can be different in different frames, and force is invariant (if we regard inertial frames).

 

[PeroK]

C´mon, don't be harsh. I actually think we are making progress.

Again, I think it is more convenient to focus the conversation on WHAT's right instead of WHO's right.
It's a long thread already so I'll try an unofficial summary of it to help us get back on track. OP, correct me if this doesn't summarize the content discussed so far.

We're trying to figure out if it's possible to pass energy from one body to the other during a flyby. For example:
State 1: 5h before flyby.
State 2: Nearest point in the orbits.
State 3: 5h after flyby.

@LesRhorer claims that it is necessary to have a 3rd body if you want to have any energy transfer between the bodies. Otherwise, incoming and outgoing velocities will be the same. Velocities are dependent on the FoR chosen but the point is that there is no work or energy transfer between them which does not depend on the FoR. I do agree with this.
On the other hand, other people claim that no 3rd body is necessary to accomplish the extra kick.

Only one of those things (2 bodies NOT OK - 2 bodies OK) can be true so it's just a matter of time before we figure out which one it is.

I am no moderator or anything like that but I find the topic especially interesting and I wouldn't like the thread to derail into something nasty looking.

Just to put the record straight. The purpose of this forum is to promote mainstream science. Explicitly that means we must determine what is valid and what is bogus. It's not a debating chamber where every view has equal validity.

This thread is not a debate on what physics is valid. It's a (failed) attempt to correct the OPs basic misconceptions about kinematics. Which are deeply woven into the layers of flowery prose.

 

[Juanda]

So it seems Work / Energy transfer is also frame dependent. Let me check some calculations because, as you pointed out, my argument relied on that. If work is frame dependent, then I'm longer sure the 3rd body is necessary in order to be able to "steal" energy from one body and put it on the other.
I'll try solving an elastic collision on two different FoR (at whatever point and at the CoM) to better understand what's going on and that might give me some insight related to this orbital problem.

 

[jbriggs444]

For what it is worth, @Juanda, you are engaging as a thoughtful poster with whom it is possible to have a fruitful dialogue, despite any disagreements that may be present.

 

[PeroK]

So it seems Work / Energy transfer is also frame dependent. Let me check some calculations because, as you pointed out, my argument relied on that. If work is frame dependent, then I'm longer sure the 3rd body is necessary in order to be able to "steal" energy from one body and put it on the other.
I'll try solving an elastic collision on two different FoR (at whatever point and at the CoM) to better understand what's going on and that might give me some insight related to this orbital problem.

The classic example is an elastic collision between two balls of equal mass. In the rest frame of the first mass, the second mass loses all its KE. And vice versa. In COM frame, both balls rebound with equal and opposite velocities.

For the gravity assist, the local kinematics are largely independent of any other mass. However, when we switch to the rest frame of another mass, such as the Sun, we are looking for a collision that is favourable in terms of imparting KE to the space probe. That's the trick: to organise the collision so that the probe gains maximum KE relative to the Sun. The misconception is that the Sun's gravity is involved in the local kinematics. It is only involved to a marginal degree. This has been fully explained in posts by @A.T. and @Filip Larsen

 

[A.T.]

I'll try solving an elastic collision on two different FoR (at whatever point and at the CoM) to better understand what's going on and that might give me some insight related to this orbital problem.

Good idea. These are related concepts:

From: https://solarsystem.nasa.gov/basics/primer/

Here is another similar mechanism:

 

[LesRhorer]

I also think you can achieve hyperbolic trajectories with only two bodies if the incoming speeds are high enough.

Actually, for the slingshot effect, we stipulate it starts right at or rather near zero, an infinite distance away. Such an orbit is one right at escape velocity.Any faster and it is not quite a hyperbola, and the craft will never return. Any slower, and it isn't quite a hyperbola, either, but rather an extremely eccentric ellipse. It might take nearly an eternity, but barring any other influences it will eventually return. Such an orbit would be ideal for a slingshot maneuver, except of course the silly planet isn't staying still. It is whipping around the central star. What we need to do is at the point where the planet's gravitational field strength begins to exceed the star's, try as closely as possible to replicate one of the ideal orbits detailed above at that point. We also tray as best we can to select a perigee so that the magnitude of the incoming velocity is as close to the orbital speed of the planet. If we manage to get it just right, we can a much as double the speed of the spacecraft and send it in precisely the direction we want. To say it is a tricky maneuver is an incredible understatement.

However, before and after flyby conditions/states would be the same, right?

In the case of a two body system, yes absolutely. Adding a third sufficiently large body pretty much destroys the symmetry, to our great advantage.

So, in that case, you would not be really stealing energy from one body to pass it to the other in the way it was done during the Voyager missions to increase the speed of the probes or other similar missions.

There being no other force to change the motion of either body in the 2 body system, no.

In the case of a speed-up maneuver, which can only happen in a three body system, the planet will suffer a virtually infinitesimal reduction in orbital momentum about the Sun by tugging on the spacecraft to speed it up. Oddly enough, rather than slow the planet down, it actually speeds it up as well, but at at an infinitesimally lower orbit. In a braking maneuver, the craft slows down by pulling the planet along, rather than vice-versa. This induces the planet to climb into an infinitesimally higher orbit and slow down an immeasurably small amount.

Do you think the reasoning is correct?

It seems so. It all hinges on the fact there is only one force in a two body system, and that force is perfectly symmetrical with respect to both bodies. Adding a third body introduces a second force which destroys the symmetry. If the two bodies remain close together - i.e. an elliptical orbit around each other - then the force from the third body will never exceed that of the force between the two smaller bodies, and so all it does is perturb their orbit somewhat, rather than produce the very large acceleration we see with a slingshot maneuver.

In post #48 I claimed a similar thing to what I'm posting here although I was missing the word "hyperbolic" at that time.

Well, it is important. Fundamentally, in order to work as advertised, the spacecraft must be able to exceed escape velocity for the planet. The best way (the only way, really) to do that is for the spacecraft to approach the planet at something close to escape velocity - which to first approximation implies a hyperbolic trajectory.

 

[Dale]

Actually, for the slingshot effect, we stipulate it starts right at or rather near zero, an infinite distance away. Such an orbit is one right at escape velocity.

This is not correct. There is no requirement that the velocity be right at the escape velocity. In fact, it should be above it.

Any faster and it is not quite a hyperbola

That is also false. A hyperbolic orbit is always faster than escape validity. I don’t know where you are getting all of this incorrect information.

In the case of a two body system, yes absolutely.

Only in the CoM frame. A third body is not needed. By the principle of relativity we can use any inertial frame we like.

It all hinges on the fact there is only one force in a two body system, and that force is perfectly symmetrical with respect to both bodies. Adding a third body introduces a second force which destroys the symmetry.

This is not needed.

 

[A.T.]

Adding a third body introduces a second force which destroys the symmetry.

Not if the force from the third body is approximately uniform gravity, which accelerates the first two bodies nearly the same way.

What destroys the symmetry is switching from the CoM-frame of the the two bodies to the CoM-frame of all three bodies. But either frame is valid, and you can use both in the same same analysis if you transform the velocities correctly between them.

 

[LesRhorer]

The classic example is an elastic collision between two balls of equal mass. In the rest frame of the first mass, the second mass loses all its KE. And vice versa. In COM frame, both balls rebound with equal and opposite velocities.

Perfectly correct, of course. The point is the total kinetic energy of the system remains constant. If we fly a jet over the two balls, the relative energy of the system in the FoR of the jet is HUGE, but at the moment of the collision the energy of the two ball system WRT the jet does not change, even though the velocities of both balls do.

In a slightly more apt analogy for this case, instead of two balls of equal mass, we can take a freight train and bounce the ball off it. To a person on the train, the ball arrives and leaves at the same speed, just in opposite directions. If the ball's initial velocity is V, then the total acceleration is 2V. To a person at thetrain station, who sees the ball initially travelling at 1/2V, the ball will come back at 1-1/2 V. In that frame of reference, the total acceleration is 2V. To the jet flying overhead, the initial velocity of the ball might be, say, 100V. After the collision, depending upon the direction the jet is flying, the new velocity is either 98V or 102V, resulting in an overall acceleration of 2V. I trust everyone can see a very distinct pattern, here, The point is while velocites are always relative to the particular frame of reference, accelerations are not. We can fiddle with relative velocities all we want, but it does not change the amount f energy involved in some interaction. The changes in Voyager's velocites were not just a matter of changing reference frames. Their speed increased in every reference frame, including that of Jupiter and Saturn.

For the gravity assist, the local kinematics are largely independent of any other mass.

Well, yeas and no. Mostly yes. Jupiter and Saturn do have orbital velocities rather close to the incoming velocities of Voyager I and II. to that end, the velocities cannot be ignored, and they are 100% produced by the influence of the mass of the Sun. That said, over a relatively short time period we can take the velocity to be constant and the trajectory flat, rather than curved. During the time the craft is within a few planetary diameters, it is close enough for a first approximation. The salient point, however, is that even though the local field strength is much larger than the remote field strength, the sum total of all the contributions of the local gravitational filed is zero. Suddenly the very tiny, but still non-zero contribution of the second order field gets important to the overall result.

However, when we switch to the rest frame of another mass, such as the Sun, we are looking for a collision that is favourable in terms of imparting KE to the space probe. That's the trick: to organise the collision so that the probe gains maximum KE relative to the Sun.

Not just relative to the frame of reference of the Sun. For a speed increase maneuver, the change in velocity compared to that of an unaccelerated system is greater than the speed change relative to the Sun. The planet is accelerating away from its original locus after all. My point, however, is if the Sun has the mass of a pea, or is a few parsecs away, then no speed-up at all occurs. The Sun's presence and influence is absolutely required.

The misconception is that the Sun's gravity is involved in the local kinematics. It is only involved to a marginal degree. This has been fully explained in posts by @A.T. and @Filip Larsen

Again yes and no. At any point along the path of the spacecraft which can be deemed local to the planet, the Sun's contribution is indeed small compared to the planet's, at some points perhaps by many orders of magnitude. There is a catch, however. While the planet successfully and inexorably pulls on the craft to speed it up while inbound, it pulls just as inexorably on the craft slowing it down when outbound. As I showed above, for any span whose endpoints are equidistant on either side of perigee, the total contribution to the speed / energy is zero Throughout that same span, the sum of the Sun's differential contributions is not zero. This is why the amount of speed / energy gain is independent of the mass of the planet. It is not, however, independent of the mass of the Sun nor the distance from the Sun. Planets closer to the Sun can produce much higher gravity boosts than the very much larger gas giants.

It is also absolutely critical the planet is orbital. The entire effect is driven by the fact we are dealing with the angular momentum of the planetary system and the torque applied by the Sun.

(Note: the planet's mass and particularly density are not completely irrelevant. They do determine the escape velocity profiles and the altitude of perigee, both of which affect the efficiency of the transfer,)

 

[A.T.]

It is also absolutely critical the planet is orbital.

You are using a very narrow definition of "gravity assist", while most people here have a more general understanding of the concept.

 

[LesRhorer]

Not if the force from the third body is approximately uniform gravity, which accelerates the first two bodies nearly the same way.

False. This is not an effect of the tidal potential. it is an effect of the fact (and magnitude) the system has a angular momentum

What destroys the symmetry is switching from the CoM-frame of the the two bodies to the CoM-frame of all three

Again, that is false. The path is not symmetrical to the CoM of the two bodies. Inbound the speed is close to escape velocity of the planet. Outbound it can be close to twice the escape velocity of the planet, not to mention more than the escape velocity from the Sun. What is more, the trajectory can be twisted through a fairly large angle relative to the planet's orbit. What would ordinarily be a hyperbolic orbit around the planet gets flattened and turned into an immelman by the interaction with the Sun

bodies. But either frame is valid, and you can use both in the same same analysis if you transform the velocities correctly between them.

Of course, but that means converting from a non-inertial reference frame to an inertial one, and accounting not only for radial acceleration of the spacecraft y the planet and the Sun, but also the cross product between the spacecraft's velocity vector and the angular velocity of the system. This is also not symmetrical to either the CoM of the planet or the Sun.

Even if this were not correct, however, my main point still stands. It does not happen without the presence of the Sun,

 

[PeroK]

Perfectly correct, of course. The point is the total kinetic energy of the system remains constant. If we fly a jet over the two balls, the relative energy of the system in the FoR of the jet is HUGE, but at the moment of the collision the energy of the two ball system WRT the jet does not change, even though the velocities of both balls do.

That's energy conservation, which holds in each reference frame. That's not energy invariance. Note that below you use the invariance of acceleration (valid) and conclude results about energy invariance (which is not valid).

A ball accelerating by the invariant $1 m/s$ in some direction has a different change in KE in each reference frame. That change may be positive or negative and have any value.

This is a fundamental misunderstanding on your part of basic kinematics.

The point is while velocites are always relative to the particular frame of reference, accelerations are not. We can fiddle with relative velocities all we want, but it does not change the amount f energy involved in some interaction.

The above confuses acceleration with energy.

The changes in Voyager's velocites were not just a matter of changing reference frames. Their speed increased in every reference frame, including that of Jupiter and Saturn.

This is completely wrong. In one particular frame, the result of the gravity assist maneuver was to reduce Voyager's speed to zero. There is always a frame where the initial velocity is zero. And there is always a frame where the final velocity is zero.

The Sun's presence and influence is absolutely required.

Not for the local kinematics which provide the gravity assist. The gravity assist is to be measured in the Sun's rest frame, as the whole point is to help escape the solar system.

 

[PeroK]

PS that velocity and acceleration are vector qualities is something else you should note. Change in velocity (vector) is invariant (across all inertial reference frames), but change in speed (magnitude of velocity) is definitely not invariant.

PPS and KE, of course, is a function of speed, rather than velocity.

 

[Juanda]

So it seems Work / Energy transfer is also frame dependent. Let me check some calculations because, as you pointed out, my argument relied on that. If work is frame dependent, then I'm longer sure the 3rd body is necessary in order to be able to "steal" energy from one body and put it on the other.
I'll try solving an elastic collision on two different FoR (at whatever point and at the CoM) to better understand what's going on and that might give me some insight related to this orbital problem.

You are right. In an elastic collision, the energy transfer (work) between the bodies does depend on the speed of the reference frame. Therefore, the argument I proposed is not valid.
I can't still fully understand it. Something is not clicking in my head about the whole situation.
But the link provided by @A.T. definitely helped. Especially the picture with the train and the explanation in the link.

View attachment 329335
From: https://solarsystem.nasa.gov/basics/primer/

The third body (the sun) is not necessary to add any force to the other two bodies (Jupiter and the satellite). Its importance is just in giving us a reference frame that we could consider inertial since the CoM of the 3 bodies will be basically static and inside the sun. With respect to that reference frame, the satellite will see its speed increase after the maneuver.

Thank you all for your patience.

 

[LesRhorer]

That's energy conservation, which holds in each reference frame. That's not energy invariance.

I fully recognize the difference.

Note that below you use the invariance of acceleration (valid) and conclude results about energy invariance (which is not valid).

Not quite.I recognize they are two different things. They have to be, of course, since the kinetic energy is not proportional to the velocity.

A ball accelerating by the invariant $1 m/s$ in some direction has a different change in KE in each reference frame. That change may be positive or negative and have any value.

Of course. I never said differently. My point (and its is not the main one) is the only way to effect a change of energy in a gravitationally constrained system is to apply a force due to gravity, We can change the overall kinetic energy of the system to anything we want by changing the FoR but that does not enable us to claim we have extracted or added any energy to the system internally.

Suppose we have a vehicle in orbit around a free body in deep space with an inbound velocity of 3/4 escape velocity at some point. We can set a FoR so the initial velocity of the vehicle is zero in that frame of reference. When the vehicle swings round the body it will have a velocity in the external FoR of 1-1/2 times escape velocity of the body. This does not mean the vehicle will fly of into space just because it has a greater energy and momentum WRT the external FoR. He claims it will. It does not mean the body, by itself is producing a gravity assist of 1-1/2 times the escape velocity of the free body. He claims it does. He claims merely asserting the body "has a velocity of X" - which is of course utter nonsense - means the body will produce an increase of speed of X.

The above confuses acceleration with energy.

Not at all. For any mechanical system, the change in energy of a massive body is equal to the integral of the scalar product of the force vector and the differential of the position vector. The magnitude of said force vector is always proportional to the acceleration of the body in question,unless of course there is some other force being applied to the body in addition to the one in question. For a two body gravitational system, this inexorably ties the acceleration of both components to the increase in kinetic energy of the system internally. We can change the kinetic energy of the system or any part of it by merely changing the FoR, but that will never change the relative velocities of the two bodies WRT to each other.

The relationship does not apply in an inelastic system, of course.

This is completely wrong. In one particular frame, the result of the gravity assist maneuver was to reduce Voyager's speed to zero. There is always a frame where the initial velocity is zero. And there is always a frame where the final velocity is zero.

Of course. This is not relevant to any of my points. The fact Voyager's velocity in the first frame is zero does not mean Voyager stopped dead in its tracks relative to Jupiter, More importantly, it does not mean somehow Jupiter increased Voyager's speed by a factor of three, rather than two. The amount of energy ( a total of about 500 Gigajoules) is dependent upon the forces applied and the distance over which those forces were applied. Without ever leaving Low Earth Orbit, we could have easily come up wth a FoR in which Voyager's KE was 600 Gigajoules.This would not have magically caused Voyager to head out into deep space.

Not for the local kinematics which provide the gravity assist. The gravity assist is to be measured in the Sun's rest frame, as the whole point is to help escape the solar system.

Once again, yes of course. The point is it does not happen at all if there is no Sun (or other third body)

 

[Vanadium 50]

Does anyone need more of an example why "help me win an argument" is a bad idea?

 

[LesRhorer]

You are using a very narrow definition of "gravity assist", while most people here have a more general understanding of the concept.

Such as? The point of a gravity assist is to enable a spacecraft to achieve very high velocities without using much fuel. Attempting to do this in a 2 body system results in no increase in velocity at all.

 

[A.T.]

We can change the overall kinetic energy of the system to anything we want by changing the FoR but that does not enable us to claim we have extracted or added any energy to the system internally.

I think I get that point you are trying to make here:

- Given a single massive body, any energy gain by the probe is fully frame dependent.

- Only given a system of at least two massive bodies in relative motion one can extract some energy from that system in a frame invariant sense, by reducing the velocity difference between them.

Such as?

This concept is not restricted to bodies in orbit. You could also gain speed in a desired direction by interacting with a massive body moving independently through interstellar space.

 

[LesRhorer]

This is not correct. There is no requirement that the velocity be right at the escape velocity. In fact, it should be above it.

'Not much. The most efficient transfer occurs when the orbit is a hyperbola. Starting out any faster wastes fuel, although of course it may be necessary depending on the alignment of the planets. Nothing is perfect, after all

That is also false. A hyperbolic orbit is always faster than escape validity.

I think you mean "velocity"

The shape of an orbit which tends to zero at infinity is a hyperbola. A hyperbola is assymptotic to X = 0 and Y = 0 at Y = infinity and X = infinity, respectively. If the craft does not slow all the way to zero in the limit as its distance tends toward infinity, then its orbit is not properly speaking a hyperbola. Forgetting relativity, in the limit of infinite velocity, the orbit becomes a flat line.

Only in the CoM frame. A third body is not needed. By the principle of relativity we can use any inertial frame we like.

Doing so does not increase the velocity of V WRT P. It does not increase F as V approaches P and it does not decrease F as V passes perigee. It will not turn an elliptical orbit into a hyperbolic or trans-hyperbolic one. Only in a planetary system can asymmetrical orbits be produced. Just because there are an infinite number of frames in which the relative speed of the inbound path is lower than the relative speed of the outbound path in some FoR external to the barycenter of the system in no way means the large body has increased the KE of V.it only means there is no such things as an absolute inertial frame of reference, and that all linear motion is relative to any arbitrarily chosen FoR.

 

[LesRhorer]

There are a lot of systems where both momentum and energy conserved but it would be strange to call them all elastic collisions.

I agree, although it s really merely a semantic issue, and not terribly important as long as everyone in a discussion uses the same definitions. To be sure, if both energy and momentum are conserved, the interaction is elastic. I think most people would expect a collision to involve mechanical impact. I know for certain my insurance agent would not like saying a near miss is a collision.

 

[LesRhorer]

But my simulation in Universe Sandbox changed both the speed and direction... the asteroid gained nearly 6 km/s in speed.

In what direction? In order to know the answer one must know the velocity vector of the asteroid compared to the orbital velocity of the Earth. It looks to me like the simulation assumes the earth is not in orbit around the Sun. In this case, it is a simple 2 body problem, and the answer depends only upon the frame of reference. The Earth itself then imparts no net energy to the asteroid. At something like 16 Km/sec relative velocity, the asteroid should likely wind up in a reasonably stable orbit around Earth, unless of course that 10 Km/s initial velocity was something like heading straight toward the Earth. I presume not. The Earth, however, is in fact in orbit with an orbital velocity of nearly 30 Km/s.

If the path of the asteroid was substantially parallel to that motion, the asteroid would fly off into the inner solar system at up to nearly 20 Km/s (if I am adding correctly in my head). If the path of the asteroid was substantially anti-parallel to the Earth's path, then the asteroid would likely crash into the earth, having given up a large fraction of its momentum to the Earth. If the path is substantially perpendicular to the Earth's path, then the asteroid may not pick up or lose much speed at all, but rather will reflect either Northwards or Southwards out of the plane of the ecliptic. That is what being in orbit does for you.

Note in either of the first two cases, the asteroid will wind up going roughly in the opposite direction from which t approached. In the latter two cases, it will wind up traveling not quite 90 degrees to its original path. There is a totally radical difference between a flyby of a free body in deep space and a planet in orbit around a star. One is rather uninteresting, even if one fiddles with frames of reference. The other is perfectly astounding, whether taken from the FoR of the planet or of the star.

 

[Drakkith]

An orbital flyby of Mercury results in a huge increase in speed, (over 40 Km/s) despite the fact the planet is only about 5 times as massive as our moon. A flyby of Neptune only results in a fairly small overall acceleration (about 5 Km/s), despite it having more than 300 times the mass of Mercury. That really should tell one all one needs to know anout whether the Sun's influence in a maneuver like that performed by the Voyager spacecraft, Cassini, and New Horizons. The Messenger spacecraft used assists at Earth, Venus, and on three separate flybys of Mercury in braking maneuvers to slow itself down. These maneuvers all resulted in actual changes in speed and direction compared to the Sun. They are not an artifact of changing the reference frame.

It's not about the Sun's influence, it's about the speed of the objects relative to some reference frame. Mercury is moving at 40+ km/s relative to the Sun (or a reference frame 'pinned' to the Sun, or the barycenter, or whatever you want to say). The only reason the Sun is important here is because we are tying a reference frame to it and things in the solar system are moving with respect to it.

Furthermore, no interaction between two bodies is ever capable of achieving the aforementioned results. All two body interactions result in perfectly symmetrical trajectories. Thus, simple changes in the direction of a craft along the plane of its initial trajectory with no net increase in the energy of the craft with respect to the barycenter of the two body system qualifies.

My simulation disagrees with you.

@Drakkith do you agree with this? Maybe there is something wrong with the simulation? The results you provided no longer make sense to me. I assume it's being solved numerically. Maybe the acquaricy is being an issue.

You can find the various integrators that Universe Sandbox uses here: https://universesandbox.fandom.com/wiki/N-Body_Simulation#Models

In what direction?

I provided the details in my previous post, including the velocity vectors before and after the interaction relative to the coordinate system.

It looks to me like the simulation assumes the earth is not in orbit around the Sun.

That is correct.

In this case, it is a simple 2 body problem, and the answer depends only upon the frame of reference. The Earth itself then imparts no net energy to the asteroid.

Yes, reference frames matter. In the Earth's frame, or the asteroid's frame, the initial and final speeds are the same (but not the velocities). In another reference frame things are different and energy can be gained/lost by each body. As my simulation shows.

This reminds me of how the propulsive efficiency of a rocket engine depends on the reference frame.

 

[Filip Larsen]

The shape of an orbit which tends to zero at infinity is a hyperbola.

The (degenerate) case between an elliptic and hyperbolic trajectory is actually called a parabolic trajectory, that is, the two-body trajectory where the relative speed at infinity is zero. So I guess now that when you have said "hyperbolic" earlier you actually meant what is normally labelled parabolic, i.e. a trajectory with near zero hyperbolic excess speed? That would at least explain why those parts of your posts were so hard for me to decipher.

 

[Dale]

Such as? The point of a gravity assist is to enable a spacecraft to achieve very high velocities without using much fuel. Attempting to do this in a 2 body system results in no increase in velocity at all.

This is simply false. From the wikipedia article on Elastic collisions:
https://en.wikipedia.org/wiki/Elastic_collision#Two-dimensional_collision_with_two_moving_objects

$$v_x=\frac{\cos (\phi ) (u (m-M) \cos
(\theta -\phi )+2 M U \cos (\phi ))}{m+M}-u \sin
(\phi ) \sin (\theta -\phi )$$ $$v_y=\frac{\sin
(\phi ) (u (m-M) \cos (\theta -\phi )+2 M U \cos
(\phi ))}{m+M}+u \cos (\phi ) \sin (\theta -\phi
)$$ $$V_x=\frac{\cos (\phi ) (U (M-m) \cos (\phi
)+2 m u \cos (\theta -\phi ))}{m+M}+U \sin ^2(\phi
)$$ $$V_y=\frac{\sin (\phi ) (U (M-m) \cos (\phi
)+2 m u \cos (\theta -\phi ))}{m+M}-U \sin (\phi )
\cos (\phi )$$
Where I have cleaned up the notation a bit using capital letters for the large mass and lower case letters for the small mass, and I have chosen the $x$ axis to be the direction of the initial velocity ($U$) of the large mass.

You can confirm that both momentum and energy are conserved for this system.

Note that this is a 2-body collision. There is no third body. From this expression you can obtain the increase in velocity, which you falsely claim is zero, by directly evaluating $$\Delta v=\sqrt{v_x^2+v_y^2} - u =
\sqrt{\frac{m^2 u^2-2 m M u^2 \cos (2 \theta -2 \phi
)+2 M u U (m-M) \cos (\theta -2 \phi )+2 M u U \cos
(\theta ) (m-M)+M^2 u^2+2 M^2 U^2 \cos (2 \phi )+2
M^2 U^2}{(m+M)^2}}-u$$

We can further simplify this by doing a Taylor series expansion for small $m$ to obtain $$\Delta v \approx 2U-2(U-u)\frac{m}{M} $$

So, contrary to your statement, there can be a large $\Delta v$ for a 2 body elastic collision provided that $U$ is large.

The shape of an orbit which tends to zero at infinity is a hyperbola.

This is false, it is a parabola.

If the craft does not slow all the way to zero in the limit as its distance tends toward infinity, then its orbit is not properly speaking a hyperbola

This is also false. Hyperbolic trajectories are precisely the ones that do not slow all the way to zero in the limit as distance tends toward infinity.

See: https://en.wikipedia.org/wiki/Hyperbolic_trajectory "a body traveling along this trajectory will coast towards infinity, settling to a final excess velocity relative to the central body. ... gravitational slingshots, can be described within the planet's sphere of influence using hyperbolic trajectories."

Just because there are an infinite number of frames in which the relative speed of the inbound path is lower than the relative speed of the outbound path in some FoR external to the barycenter of the system in no way means the large body has increased the KE of V.

In all of those frames the large body has indeed increased the KE of the small one. You cannot increase the speed of a mass without increasing its KE.

there is no such things as an absolute inertial frame of reference, and that all linear motion is relative to any arbitrarily chosen FoR.

While this is true, it contradicts your previous statements. That you don't recognize that is unfortunate, but clearly not something you are interested in correcting.

At this point, this thread is done. Your initial question has been answered, we will not be providing you any material to support your argument as your argument is wrong on many, many points.