Solar System Motions: Exploring Change in Angular Velocity

In summary, the conversation discusses the solar system's change in angular velocity relative to the guide star and the potential causes for this change. There is mention of a geodetic precession caused by the solar system's motion around the galaxy, but this is deemed to be negligible. The conversation also mentions a potential binary companion or other factor causing a greater change in angular velocity, and evidence for this is discussed. However, it is noted that this motion has been excluded in the past and is a well-known effect in astronomy. The conversation also mentions the solar apex and its movement, which is believed to be a separate motion from the solar system's orbit around the galaxy
  • #1
maurol2
23
0
This thread has been split off from the [thread=104694]Gravity Probe B[/thread] thread. Some posts here are duplicated in the above thread to keep a sense of continuity -- cristo

Garth said:
The "solar system’s change in angular velocity relative to the guide star" will be caused by its motion around the galaxy, I have dealt with the motion of the galaxy itself above (it is negligible).

Orbiting the galaxy would cause a geodetic precession of

[tex](\frac{M_G}{M_E})^\frac{3}{2}(\frac{R_E}{R_G})^\frac{5}{2} \times 8 \text{arcsecs/yr }[/tex]

(See MTW 'Gravitation' page 1119 eq 40.35)

i.e. about 10-8 arcsecs per year.

I think this can also be safely ignored!

Garth

Yes, but aren't you being dogmatic? Polestar101 is suggesting that the solar system is not orbiting the galaxy (at least, not only) but a binary companion(or something else, I would say). In that case the change in angular velocities(and in so called geodetic precession) will be greater than the one caused by the orbit around the galaxy.

There's some evidence for this. See the "http://en.wikipedia.org/wiki/Solar_apex" " entry on Wikipedia.

I've also found out a paper from circa 1880,
"On the Movement of the Solar System in Space, deduced from the Proper Motions of 1167 Stars"
Here's a link to http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1863MNRAS..23..166D&link_type=GIF" where you can find the abstract.
That paper is clearly pointing to a movement that is NOT the movement around the galaxy, but a movement with a far greater amount of change.

Please note also that the literature tends to differentiate between the movement of the Local Standard of Rest (LSR), which is the assumed movement around the galaxy, of the solar system and its local surroundings, and the proper movement of the solar system towards the solar apex.

I don't understand why these movements of the Solar system towards the so called solar apex, which are being studied since at least the nineteen century, are unknown or are not taken into account. Why these issues were forgotten or ignored in the course of time? Maybe because there's no known mechanism to explain them?

Regards,
Mauro
 
Last edited by a moderator:
Astronomy news on Phys.org
  • #2


maurol2 said:
Yes, but aren't you being dogmatic? Polestar101 is suggesting that the solar system is not orbiting the galaxy (at least, not only) but a binary companion(or something else, I would say). In that case the change in angular velocities(and in so called geodetic precession) will be greater than the one caused by the orbit around the galaxy.

Hi Mauro

Garth is correct based on the prevailing assumptions – but you are correct that if those assumptions are not accurate then the angular velocity of the solar system could be much higher. This was the gist of a poster/paper on “Earth Orientation” that I presented in the Geodesy group at the recent AGU conference in SF.

We measure changes in Earth orientation to VLBI reference points far outside the solar system yet we do not account for any motion of the solar system frame relative to those reference points. In fact because we allocate all changes in Earth orientation to local dynamics (traditional lunisolar inputs) we effectively constrain solar system motion to zero. So the big question is how much angular velocity is contained within the total annual precession observable of about 50.3” p/y.

The best way to solve this problem in my opinion is to try to measure how much the Earth actually precesses relative to objects within the moving frame of the solar system (i.e. EO changes relative to the moon, the sun, Venus, etc.) then compare these amounts to the EO measurements taken relative to VLBI reference points outside the moving frame.

The result we find is nutation and Chandler wobble and other short period effects are locally measurable and therefore appear to be directly traceable to local dynamics, whereas precession is nowhere to be found when measuring relative to local objects. In other words, we only see precession when measuring relative to objects outside the moving solar system indicating that what we call precession is largely just the angular velocity of the solar system relative to reference points outside the moving frame.

Incidentally, thanks for the old article on solar system motion. There have been a few other similar articles over the years, and even the IAU in 2006 said the current precession nutation model was “inconsistent with dynamical theory” (IAU P03). Alas, until we start traveling out of the solar system I doubt anyone will seriously question assumptions about its motion.
 
  • #3


maurol2 said:
Yes, but aren't you being dogmatic? Polestar101 is suggesting that the solar system is not orbiting the galaxy (at least, not only) but a binary companion(or something else, I would say). In that case the change in angular velocities(and in so called geodetic precession) will be greater than the one caused by the orbit around the galaxy.

Yes, and what he doesn't get (and which I don't have the patience to explain to him) is that all of the motions that he thinks he will see are ones that have long ago been excluded. Since you seem to be rational, I'll explain to you why his ideas (and I don't know of a nice way of saying this) are totally nutty.

One problem is that the Earth's wobble is such a well known and obvious effect that astronomers correct all of their measurements for it, and he is looking in journals and not seeing precession because when numbers are quoted precession is removed. It's something that they teach you to do in freshman astronomy classes. Polestar doesn't under very, very basic astronomy. I don't have the patience to teach him, and he doesn't seem to be interested in learning.

Now if you have any questions I'd be glad to answer.

There's some evidence for this. See the "http://en.wikipedia.org/wiki/Solar_apex" " entry on Wikipedia.

That paper is clearly pointing to a movement that is NOT the movement around the galaxy, but a movement with a far greater amount of change.

This is well known motion. Basically if you look at the stars, you get an effect that looks a lot like what the stars look like when Han Solo goes into warp drive. This is largely irrelevant for the purposes of the gravity experiment, because the sun to the first approximation is moving in a straight line through the stars. The only effect would be if the movement of the sun is curved, and that's a small effect.

I don't understand why these movements of the Solar system towards the so called solar apex, which are being studied since at least the nineteen century, are unknown or are not taken into account.

They don't matter for the purposes of this experiment, because as long as the sun is moving in a straight line, it's not accelerating and if it's not accelerating then they don't effect any experiments designed to measure acceleration.

One way of thinking about it is to imagine Captain Kirk on the Starship Enterprise. When the Enterprise is going through the star field, you see star move past, but Kirk isn't getting bumped around. It's only when the Enterprise makes a sharp left turn that Kirk gets thrown around the bridge of the Enterprise. Now imagine a spinning gyroscope on the bridge, and you'll see why the local movement of the sun doesn't matter.

Why these issues were forgotten or ignored in the course of time? Maybe because there's no known mechanism to explain them?

All of these mechanism are not forgotten and they are well known, and people do take them into account.
 
Last edited by a moderator:
  • #4


Also there are very strong limits on the existence of any extra solar star based on

1) celestial mechanics. Anything that could simulate axis precession would wreck havoc on solar system planetary motion

2) comets. Something with a 26,000 year orbit would be in the Oort and Kupier belts and we'd see comets raining down from that area

3) stellar evolution. Any star that is within a 26,000 year orbit is going to be seen.

This is just a totally nutty idea. There's a whole literature that places on the extra-solar system objects which are possible. Planet X and Nemesis. It's just one step above flat earth.

One problem is that most of the people on this thread are GR experts, and if you want to rule out the existence of a binary companion to the Sun, the strongest tests are not GR effects.
 
Last edited:
  • #5


twofish-quant said:
Now if you have any questions I'd be glad to answer.

They don't matter for the purposes of this experiment, because as long as the sun is moving in a straight line, it's not accelerating and if it's not accelerating then they don't effect any experiments designed to measure acceleration.

Just for clarity: the Sun is not moving in a straight line. It is moving in what we consider to be, in the relative short term, equivalent to a straight line.

All of these mechanism are not forgotten and they are well known, and people do take them into account.

So, can I ask you what is the presumed cause of these movements?
And what's the known rate of curvature and/or acceleration of the movement towards the solar apex?
Or, in other words, assuming this movement is elliptical, o equivalent to an elliptical movement, what is its period in years?

Thanks,
Mauro
 
  • #6


twofish-quant said:
Also there are very strong limits on the existence of any extra solar star based on

1) celestial mechanics. Anything that could simulate axis precession would wreck havoc on solar system planetary motion
This a strong objection, and it's the main reason I disagree with Polestar101. If the solar system is moving in a curved path, that movement will produce parallax effects, not precession. The only way for them to produce precession, would be if the actually known physical laws are not valid for these movements.

2) comets. Something with a 26,000 year orbit would be in the Oort and Kupier belts and we'd see comets raining down from that area
This is not a so strong objection, as there have been comets raining down in the past. We can be now in a relatively quiet part of the orbit. Also, the orbit's period can be bigger than 26000 years.
3) stellar evolution. Any star that is within a 26,000 year orbit is going to be seen.
Again, that is not a so strong objection. The sun can be in orbit with an invisible companion. Indeed, so called "dark matter" points in that direction.

This is just a totally nutty idea. There's a whole literature that places on the extra-solar system objects which are possible. Planet X and Nemesis. It's just one step above flat earth.
Let's say that for Polestar101 ideas to be valid, our actual understanding about how the physical universe works would have to be radically changed, or extended.

One problem is that most of the people on this thread are GR experts, and if you want to rule out the existence of a binary companion to the Sun, the strongest tests are not GR effects.

I know. I'm not interested in ruling out a binary companion (nor in the tests of GR in itself), but in precisely understanding the solar system movement in space, its causes, and its effects. Maybe GP-B results can be of any help in that regard. That's the reason I'm posting.

Mauro
 
  • #7


maurol2 said:
So, can I ask you what is the presumed cause of these movements?

One of the things that Newton figured out is that if something moves in a straight line, there isn't a need to explain why it's moving in a straight line. You only need an explanation if something is curving or accelerating.

What's happening is that the stars in our region in space are moving in an orbit around the center of the milky way whose period is 220 million years. The sun has a random motion relative to its neighbors.
 
  • #8


This probably should be carved off into another topic.

maurol2 said:
This a strong objection, and it's the main reason I disagree with Polestar101. If the solar system is moving in a curved path, that movement will produce parallax effects, not precession.

There are also tidal effects. If there was a gravitational object on one side of the solar system, you'd see stronger gravity on one end of the solar system than on other. There are limits to the size of "planet X" objects around the solar system, and a solar binary companion is exclude.

This is not a so strong objection, as there have been comets raining down in the past. We can be now in a relatively quiet part of the orbit. Also, the orbit's period can be bigger than 26000 years.

It's not so much the number, but the distribution of comets. If you have a gravitation object on one side of the solar system that would disrupt comets on that side more than the other, so we should see more comets coming in from one side of the solar system than the other.

Also the orbital period can be more than 26000 years which is the problem. Anything with an orbit of say 50,000 years is likely to interact with an object that has an orbit of 26,000 years.

The sun can be in orbit with an invisible companion. Indeed, so called "dark matter" points in that direction.

Even if the hidden companion was a black hole, you'd see it bend/block the stars behind it. The thing about a hidden companion is that you'd be able to quickly figure out the direction from observations, and even if it was a black hole, you'd see it bending the stars behind it.

Let's say that for Polestar101 ideas to be valid, our actual understanding about how the physical universe works would have to be radically changed, or extended.

No, that's not true. Science is a game in which people through up objections, people counter objections and so forth. The thing is that if you make any theory complicated enough you can explain anything, but if you can explain anything, you explain nothing.

I know. I'm not interested in ruling out a binary companion (nor in the tests of GR in itself), but in precisely understanding the solar system movement in space, its causes, and its effects. Maybe GP-B results can be of any help in that regard. That's the reason I'm posting.

One problem is that sometimes people with crackpot ideas get a false sense of how strong their ideas are by talking to scientists. Scientists tend to be super expert about one thing, but outside of the one thing, they just have average knowledge. So what happens is that if you have a nutty theory you can often get some scientist not to react at how nutty the idea really is, if the thing that kills the theory falls outside their area of expertise.

GP-B may not exclude the possibility of a solar companion, but it also doesn't tell us anything about the dinosaurs or how to make good tasting pizza. What really *kills* the idea of a solar companion are planetary motions.
 
  • #9


twofish-quant said:
One of the things that Newton figured out is that if something moves in a straight line, there isn't a need to explain why it's moving in a straight line. You only need an explanation if something is curving or accelerating.

What's happening is that the stars in our region in space are moving in an orbit around the center of the milky way whose period is 220 million years. The sun has a random motion relative to its neighbors.

So, this movement of the sun is not rectilinear and uniform. As something cannot be "random" and rectilinear and uniform at the same time.
Are the movements of the solar system towards the solar apex actually clearly understood and explained as caused by the gravity of the surrounding stelar environment? Can you point to papers or articles about this? Particularly: is the actual rate of change of this movement known?

Thanks,
Mauro
 
  • #10


Garth said:
If other effects such as poholde and perturbing forces are eliminated then gyros 'point in a constant direction' in space. Garth

You can't simply eliminate polhode and other perturbing forces to save the experiment without first being able to exactly quantify these effects. And to try and measure them by eliminating anything that does not get to the GR goal is circular reasoning and bad science.
 
  • #11


twofish-quant said:
... the Earth's wobble is such a well known and obvious effect that astronomers correct all of their measurements for it...

And this is the root of the problem. The earth’s wobble is indeed well known, measured and corrected for – so most scientists ‘assume’ that its theoretical cause (primarily lunisolar forces acting on the oblate earth) is a proven theory. Unfortunately, belief in a theory without questioning can have devastating results. In this case that unfounded belief wasted over $800 million of taxpayer money on an ill conceived gravity experiment and earned GP-B the well publicized grade of 'F' from the NASA review board. The GP-B guys failed to consider unknown solar system motion relative to the guide star. Rather than question if conventional theories are correct they prefer to use polhode and other unquantifiable effects to fix their results.

twofish-quant said:
It's something that they teach you to do in freshman astronomy classes

Good thing education doesn’t stop there. A deeper study of precession theory will show that Newton’s original equations didn’t work (and only temporarily came close after d”Alembert made assumptions about a non-rigid earth). Noticing the model’s inability to predict changes in the rate of precession over the last century scientists have repeatedly added and modified inputs resulting in the supposed final PN model in the year 2000 (2000A has almost 1400 terms and few realize it is forced to fit the observable). Alas, this problem has not escaped the IAU who in 2006 passed a resolution to say the precession nutation model “is not consistent with dynamical theory”. Read: it’s broken.

twofish-quant said:
They don't matter for the purposes of this experiment, because as long as the sun is moving in a straight line, it's not accelerating and if it's not accelerating then they don't effect any experiments designed to measure acceleration.

Assuming the sun has no acceleration compounds the mistake and obfuscates the solution. Direct observations show the sun moves across the background stars at the rate of about 50” p/y. But convention assumes it doesn’t really do this because it assumes we are observing from a wobbling earth. And this is based on the assumption that lunisolar theory is correct so we deny the observation and constrain solar system motion to zero – and thereby conclude there can’t be any acceleration. Too many assumptions make for bad science. At the very least we should admit we don’t know where the sun is going and ask if there is any other way to explain its motion.

If the apparent motion of the stars moving across the sky at the rate of 30 degrees per month has been found to be due to an orbit (the earth’s orbit around the sun) it should not be inconceivable that the apparent motion of the stars moving across the sky at the rate of 30 degrees per 2000 years (a.k.a. the precession observable) might also be due to orbital dynamics (the orbit of the solar system around another mass). This is a simple concept but unfortunately when the cause of the later observable was hypothesized no one knew the solar system moved – and no one has bothered to rethink the problem (question Newton!?) since that time.

At BRI we’ve built a model to predict the changing rate of precession by applying Kepler’s laws to orbit parameters (24,000 year periodicity, apoapsis in 500AD) given by the Indian astronomer Sri Yukteswar in 1894, which he used to explain the precession observable. We then compared that model to the precession model given by the best astronomer of the same era, Simon Newcomb, and ran the two models from 1900 to 2000 then compared these to the actual precession rate reported in the Astronomical Almanac. The result is the Yukteswar orbit based model predicted changes in the rate of the precession observable 41 times more accurately than Newcomb’s lunisolar based model over the last 100 years. If predictability is the hallmark of science then the local dynamics model should be replaced with an angular velocity model as the later has proven a far more accurate way to predict changes in the so called precession rate over time.


twofish-quant said:
Since you seem to be rational, I'll explain to you why his ideas (and I don't know of a nice way of saying this) are totally nutty.

Yes, it may be “nutty” to question conventional theory but it is even nuttier to blindly support a flawed theory. Let rational science and predictability, not convention, determine which theory is correct. It boggles the imagination that convention measures changes in the earth’s orientation to VLBI reference points far outside the moving frame of the solar system without accounting for any motion of that frame relative to those reference points. Does the Earth not move with the solar system? Now that’s “nutty”!

Polestar
 
  • #12


twofish-quant said:
Also there are very strong limits on the existence of any extra solar star based on

1) celestial mechanics. Anything that could simulate axis precession would wreck havoc on solar system planetary motion

No exo-solar object “stimulates axis precession” because there is no classical precession to produce. The observable of the stars moving across the sky at the rate of 30 degrees per 2000 years is simply the observable of a solar system in motion, just as the observable of the stars crossing the sky at the rate of 30 degrees per month is caused by the orbital motion of the Earth around the sun. The moon causes nutation and the tides – the precession observable has been misdiagnosed.

twofish-quant said:
2) comets. Something with a 26,000 year orbit would be in the Oort and Kupier belts and we'd see comets raining down from that area

Scientists such as Whitmire and Matesse have suggested that long cycle comet activity is due to a companion but several scenarios suggest the object could be much much farther away (depending on the speed of the solar system). Remember we are not talking about a planet that revolves around the sun, we are talking about our sun (and entire solar system) revolving around a common center of mass with a very distant mass. As long as the distance between our furthest planet and the companion is at least 5x the distance of our furthest planet from our sun the perturbations on the planetary system would hardly be noticeable.

twofish-quant said:
3) stellar evolution. Any star that is within a 26,000 year orbit is going to be seen.

It could well be that we do see it but don’t recognize it but it could also be a brown dwarf, red dwarf towards the galactic center, or even a black hole. If astrophysicist Reg Cahill is correct the solar system is moving a lot faster than anyone believes – this opens up a lot of possibilities.

twofish-quant said:
This is just a totally nutty idea.

Sitting on a mud ball hurtling through space – dark matter - communicating with electrons now – its all nutty, no question about it!

twofish-quant said:
One problem is that most of the people on this thread are GR experts, and if you want to rule out the existence of a binary companion to the Sun, the strongest tests are not GR effects.

You are right. It is just that GP-B was a great experiment to detect motion of the solar system. Unfortunately, the team did not account for a moving reference frame relative to the guide star (far beyond their expectations) so they ended up with all sorts of "noise" they could not understand. They tried to save the experiment by calling it polhode - effects impossible to predict - but thankfully the NASA review board recognized the charade. By the way, I have no problem with the GR effects - but I am more interested in the "noise". : )

Polestar
 
  • #13


maurol2 said:
... Imagine for a moment that there actually are unknown effects, whose causes are being mistaken in the GP-B experiment.

This is not really a useful direction. It's a truism that there may always be unexpected effects that we don't know and what we think we know is wrong.

The point is that the actual measurements have a level of uncertainty which limits the accuracy at which they can test the GR effects. To the extent that they can test any of the ideas we are considering, they confirm GR -- though not to the accuracy that was initially hoped.

There is no consistent detectable signal in the numbers found that might correspond to unknown effects. There may be unknown effects, of course -- this is true for any experiment. But the numbers say they unknowns -- such as alleged unusual or unexpected motions of the solar system -- are too small to be tested by this experiment.

The notion that they are just being ignored or assumed away is flatly false.

Cheers -- sylas
 
  • #14


Polestar101 said:
You can't simply eliminate polhode and other perturbing forces to save the experiment without first being able to exactly quantify these effects. And to try and measure them by eliminating anything that does not get to the GR goal is circular reasoning and bad science.

This doesn't make any sense at all. They DO quantify the podhole effect. It was quantified and understood and taken into account from the start. There is an additional effect which was stronger than anticipated; from a tiny residual change on the gyroscopes, which gives an additional effect on the motions. There is no doubt at all that this effect exists. Most of the work of the extended data analysis phase HAS been to quantify this effect -- and not by assumption. When quantified, it can be extracted to reveal any underlying signal.

This is an extra factor influencing the gyroscopes which was larger than anticipated, and has been at the root of the limited accuracy to which results could be given.

The description by Polestar101 is very misleading. It's not bad science at all -- it is precisely what science should do to test GR as well as they can without making assumptions. They quantify all influences and obtain the residual signal, which stands then as a test of the predictions from the frame-dragging effect. There is no assumption of GR involved in that process. Without the proper quantification of the electromagnetic forces, the accuracy of the test is very weak. With proper quantification, the test will improve, though it is unlikely to get to the level of 1% which had originally been hoped.

There's a nice summary of the issues in The Gravity Probe B Bailout, IEEE Spectrum, Oct 2008. This report is describing how the team was able to secure additional funding; and their own project page gives more on the existing funding. (Gravity Probe B -- current status -- updated November 12, 2009. The work is ongoing, and primarily this is focused upon quantifying the effects of the electromagnetic influences, so that they can be properly take into account -- without just making assumption -- and so improving the accuracy of the true independent test of GR.
 
  • #15


Can someone please start another thread...

First of all, do you accept Newtonian physics as a reasonable approximation for solar system dynamics. If you don't then we really have no basis for discussion since if you make up your own physics, you can get any answer you want.

Polestar101 said:
No exo-solar object “stimulates axis precession” because there is no classical precession to produce.

I'm not talking about that. I'm talking about predictions about the location of the planets (i.e. were is Mars)? If you have a exo-solar object and you aren't totally rewriting the laws of gravity then this exo-solar object will influence the locations of the planets in a big way. Now if you are rewriting the laws of gravity than all bets are off.

Remember we are not talking about a planet that revolves around the sun, we are talking about our sun (and entire solar system) revolving around a common center of mass with a very distant mass. As long as the distance between our furthest planet and the companion is at least 5x the distance of our furthest planet from our sun the perturbations on the planetary system would hardly be noticeable.

Except that it's not. You have long period comets which are going to interact with this hypothetical star. There was some discussion a few years back about whether a companion star to the sun causing mass extinctions. The consensus now is that this isn't happening, but you are talking about a far more massive companion which would have much larger effects.

It could well be that we do see it but don’t recognize it but it could also be a brown dwarf, red dwarf towards the galactic center, or even a black hole. If astrophysicist Reg Cahill is correct the solar system is moving a lot faster than anyone believes – this opens up a lot of possibilities.

So tell us what to look for and where to see it. It's OK to list the possibilities and then eliminate them.

You are right. It is just that GP-B was a great experiment to detect motion of the solar system.

Personally I don't think it is, since GP-B was trying to eliminate that as an effect.

Unfortunately, the team did not account for a moving reference frame relative to the guide star (far beyond their expectations) so they ended up with all sorts of "noise" they could not understand.

That's precisely what makes it a terrible experiment to look for what you are looking for. The first reaction of any physicist to any small effect is that it's noise, and the reason physicists have that reaction is that most of the time, it is. If you want to convince people that your theory is right, you have to come up with an experiment that has such a *HUGE* effect that you can't argue that it's noise. That's the job of a theorist. If the different is a few arcminutes, this is going to convince anyone. You have to come up with an experiment that is off by tens of degrees.

It occurs to me that the motion of Pluto is going to be a lot better experiment than anything that you can come up with in GP-B.

By the way, I have no problem with the GR effects - but I am more interested in the "noise". : )

I think GP-B is just the totally wrong experiment for you to focus your attention on, since they are trying to eliminate the effects you are looking for. The experiments are really sensitive and if there are any unexplained results they are small enough that people are going to conclude that it's just noise. You are wasting your time on GP-B, and you should be looking at something else.

Something that you should do (and I'm putting the work on you because you are the theorist) is to calculate the effect of your companion star on Pluto and compare that with the effects on Jupiter. If it's small, then try something else. You aren't going to convince anyone of anything by looking at small effects, you have to have a whopping big effect that no one can possibly explain by tweaking the variables.
 
  • #16


maurol2 said:
That's what Polestar101 is saying, if I understood correctly. And I think that that's a possibility that clearly deserves a closer scrutiny.

Perhaps but not by GP-B.

Those are the known, small effects, predicted by GR. Imagine for a moment that there actually are unknown effects, whose causes are being mistaken in the GP-B experiment.

If the effects are small enough, then you'll never see them with GP-B. It's quite possible that there is some unknown effect that is being dismissed as noise by GP-B, and in fact I think it's quite likely that there is some unknown effect somewhere that is effecting GP-B. But the way that physicists do experiments, if it's not something that you are expecting then you aren't going to see it. The trouble is that it's hard to see something that you aren't looking for.

This happens all the time in science. People come up with a new idea and then they go back to old data and find that it was staring them at the face all the time. But to come up with the new idea usually involves a "smoking gun."

That's where theorists come in, and the job of a theorist is to come up with ideas for experiments which have effects that are far, far, far too large to be dismissed as noise. The reason don't think that Polestar101 is that he isn't accepting the fact that you are just never going to convince people that GP-B results are due to some companion star, and not looking for the smoking gun elsewhere. I'm trying to be helpful and I've come up with about three suggestions for what to look for.
 
  • #17
maurol2 said:
So, this movement of the sun is not rectilinear and uniform. As something cannot be "random" and rectilinear and uniform at the same time.

Yes it can be.

Are the movements of the solar system towards the solar apex actually clearly understood and explained as caused by the gravity of the surrounding stelar environment?

It's not caused by the gravity of the surrounding stellar environment. The idea in both Newtonian and GR is that if something moves in a straight line, then there is nothing to explain. Gravity causes things to curve.

Can you point to papers or articles about this?

Probably not since in the framework of physics that most people use, there's nothing to explain.
 
  • #18
First, thanks for your answers, twofish-quant.
twofish-quant said:
Yes it can be.

I see. The official position on this is that the sun is moving on a straight line towards a random point.

It's not caused by the gravity of the surrounding stellar environment. The idea in both Newtonian and GR is that if something moves in a straight line, then there is nothing to explain. Gravity causes things to curve.
I know that, twofish-quant. The question would then be: how do scientists know that the Sun is moving in a straight line towards the solar apex?
Better yet: what amount of curvature would be acceptable given the actual knowledge of solar system motion? that is, assuming that a gently curved motion is assimilable to a straight line, for relatively short intervals of the curve, how gentle that curve must be?

Probably not since in the framework of physics that most people use, there's nothing to explain.

Well, it could be interesting to compare the results of Dunkin's 1880 paper on solar system motion, with a recent similar study of solar system motion. In more than a century a noticeable difference could show up, even if the statistical nature of the process will tend to obscure it.

Mauro
 
  • #19
I see. The official position on this is that the sun is moving on a straight line towards a random point.

The official position is that all of the stars in this area are moving around the center of the galaxy. Now if you look at the sun's position relative to these stars, you'll see an extra "random" motion. There would be something weird if the sun's motions were different than the other stars in the region but they aren't.

The question would then be: how do scientists know that the Sun is moving in a straight line towards the solar apex?

I think the correct statement would be that the observations are consistent with the sun moving in a straight line toward the solar apex. The data is really noisy, so if there was some curvature I don't think you'd see it from stellar proper motion observations.

Better yet: what amount of curvature would be acceptable given the actual knowledge of solar system motion? that is, assuming that a gently curved motion is assimilable to a straight line, for relatively short intervals of the curve, how gentle that curve must be?

That's a great question. I don't think you can get this information from stellar evolution velocities measurements since you just have a snapshot of proper motions. One obvious constraint is planetary motions. Anything that causes the solar system to curve is going to create a "centrigual force" on the planets, which would change their orbits.

Something else that you can see are doppler shift changes to distant quasars. Changes in the CMB.

I'm not sure what the limits would be off hand, but they would be interesting to calculate. My gut feeling is that the limits would be on the order of meters per second.

Well, it could be interesting to compare the results of Dunkin's 1880 paper on solar system motion, with a recent similar study of solar system motion. In more than a century a noticeable difference could show up, even if the statistical nature of the process will tend to obscure it.

It would be, but comparing these sorts of datasets turns out to be hard because they are often noisy.
 
  • #20
twofish-quant said:
That's a great question. I don't think you can get this information from stellar evolution velocities measurements since you just have a snapshot of proper motions.
Thanks.

One obvious constraint is planetary motions. Anything that causes the solar system to curve is going to create a "centrigual force" on the planets, which would change their orbits.
Indeed.
The orbits of the planets seem to be changing. There's an unexplained lengthening of Sun-Earth distance, by example, which is measured with great precision using laser or radar ranging. I'll post the article or paper when I find it.
A lengthening of Sun-Earth distance over the semi major axis would be consistent with an acceleration of the Sun in the direction of the (northern) winter solstice, if I'm not mistaken.
It could be interesting to compare Sun-Earth distance changes over the semi-major axis vs. changes in distance at the equinoxes, i.e. to try to determine changes in the eccentricity of Earth's orbit.
Also, if the Sun is accelerating "laterally", the Sun-Earth distance at one of the equinoxes will tend to be smaller than at the other equinox, and the side of the smaller distance will be in the direction of the acceleration. And the amount will tell us something about the magnitude of the acceleration.
Comparative orbital dynamics! It seems that's all we need to know how and how much our direction in space is changing.

I'm not sure what the limits would be off hand, but they would be interesting to calculate. My gut feeling is that the limits would be on the order of meters per second.
Could be. Could be more. Could be changing.
My own estimate is that the limits would be on the order of some hundreds of meter per second maximum, because the estimations and measurements of velocity towards the solar apex(if they are correct, of course) are in the order of tens of kilometers per second. An amount two orders of magnitude smaller sounds like something that could be overlooked, specially if the data is noisy.

Regards,
Mauro
 
  • #21
maurol2 said:
The orbits of the planets seem to be changing. There's an unexplained lengthening of Sun-Earth distance, by example, which is measured with great precision using laser or radar ranging. I'll post the article or paper when I find it.

Yes. The trouble is that there may be a thousand different things that could cause this, and you need some particular reason to believe that a curvature in the sun's motion is causing that as opposed to interaction with dark matter particles or mismeasurements in the mass of Jupiter. Something that I found interesting is that radiation pressure turns out to be able to change the motion of asteroids.

One problem I have with polestar is that he keeps picking small anomalies and not realizing that any of his ideas would result in much, much larger differences that those anomalies.

A lengthening of Sun-Earth distance over the semi major axis would be consistent with an acceleration of the Sun in the direction of the (northern) winter solstice, if I'm not mistaken.

And it's also consistent with a thousand other things. What you really need to get a smoking gun is to start with the assumption of acceleration, figure out all of the consequences, and then come up with some sort of obvious smoking gun. Just to give you one, if the you have an unexplained motion of the earth, and an unexplained motion of Mars and they are in the same direction that means something very different than if they aren't.

You can also work it the other way. Given what we know about the solar system, what is the maximum amount of acceleration that is possible? It's not zero.

My own estimate is that the limits would be on the order of some hundreds of meter per second maximum, because the estimations and measurements of velocity towards the solar apex(if they are correct, of course) are in the order of tens of kilometers per second. An amount two orders of magnitude smaller sounds like something that could be overlooked, specially if the data is noisy.

There is a dimensional problem here. Acceleration is in distance per second per second.

My suspicion is that the limits from the proper motion data are much worse than that since the data is so noisy. Something to point out is that one set of solar apex measures provide no obvious limits on the acceleration of the solar system, since you are just taking one snapshot. You need measurements over time, and I suspect even those are going to be extremely noisy. Also solar apex measures tell you nothing at all, if all the stars in the local region are getting accelerated in the same way as the sun.

Also this is all an interesting game, because you are always thinking of ways of getting tighter measurement.
 
  • #22
twofish-quant said:
There is a dimensional problem here. Acceleration is in distance per second per second.
You're right. I was thinking about changes in velocity during an interval of some years between observations or estimations, I suppose.

Some interesting related papers:
http://arxiv.org/abs/0907.2469"
http://arxiv.org/abs/gr-qc/0604052"
http://arxiv.org/abs/0904.1562"
http://arxiv.org/abs/0907.4514"

What would be interesting to do is to analyze the changes of the Sun-Earth distances at different points of the Earth orbit. That is, instead of working on trying to explain the general secular increase of the Astronomical Unit, to try to detect if there are specific sectors of the Earth orbit at which the distances are increasing / diminishing.
That could be a way to see if the changes are due to an acceleration of the Sun, or to other factors. Of course this is not so easy to calculate, because the effects of the different planets, particularly Jupiter, would have to be carefully taken into account, these planets are also moving, the sun-earth barycenter is changing, etc.
But this looks more promising than to try to compare historical statistical analysis of stelar proper motions.

Regards,
Mauro
 
Last edited by a moderator:
  • #23
Curiously in looking at the references in one of the papers I found this

http://adsabs.harvard.edu/abs/2005AJ...130.1939Z

It uses millisecond pulsars to establish an acceleration limit of a/c~a few×10-19 s-1 which ends up being 3 x 10^-10 m/s/s

One thing that I find pretty amazing is that we seem to know length of the astronomical unit to with 3 *meters*, and the increase in the AU is 15 *cm* per year. This makes it really difficult to figure out whether the increase is higher in one part of the Earth's orbit than another, since I don't you have the data to that resolution.
 
Last edited:
  • #24
twofish-quant said:
Curiously in looking at the references in one of the papers I found this

http://adsabs.harvard.edu/abs/2005AJ...130.1939Z

It uses millisecond pulsars to establish an acceleration limit of a/c~a few×10-19 s-1 which ends up being 3 x 10^-10 m/s/s

One thing that I find pretty amazing is that we seem to know length of the astronomical unit to with 3 *meters*, and the increase in the AU is 15 *cm* per year. This makes it really difficult to figure out whether the increase is higher in one part of the Earth's orbit than another, since I don't you have the data to that resolution.

I've found the original paper on the secular increase of the AU:
http://iau-comm4.jpl.nasa.gov/GAKVAB.pdf

They are using comparations of radiometric distances to Mars stationed spacecraft .
That's why the precision is better than that of the AU itself.

I suppose this rules out my idea of studying distance asimetries on different sectors of Earth's orbit, unless a reliable method to measure distance to the Sun(distance measurement to a Sun's close orbiting spacecraft ?) is established.
 
Last edited by a moderator:
  • #25
maurol2 said:
I suppose this rules out my idea of studying distance asimetries on different sectors of Earth's orbit, unless a reliable method to measure distance to the Sun(distance measurement to a Sun's close orbiting spacecraft ?) is established.

That's where the fun part of physics comes in. You often want to do something and you find out that for various reasons you can do it in the obvious ways, so you spend the next several months/years trying to figure out how to do it in a non-obvious way. You might want dig some more about exactly how the measurements are done.

Trying to figure out what correlates with the increase in the AU is interesting because it may turn out that when you look at the data, it doesn't correlate with the location of the Earth at all but with the location of Mars. Something else that occurs to me (and I'm thinking out loud) it might be a good idea to compare observations that involve spacecraft and those that involve things that are planted on the ground.

One other thing that I'd find interesting is to try to see if there are any systematic differences between US, Russian, and European spacecraft , since it occurs to me that all of the anomalies seem to be associated with US spacecraft , and it would make me more confident that it's not equipment if you are able to repeat the results with Russian spacecraft using Russian equipment.
 
  • #26
The Moon orbit is turning more eccentric:
"Williams J.G., Boggs, D.H., 2008, paper presented at 16th International Workshop on Laser Ranging 13-17 October 2008 - Poznań , Poland"

This is consistent with an acceleration of the Earth. Which is in turn consistent with an acceleration of the Sun.
These accelerations would also be consistent with an increase of the AU, so the increase of the eccentricity of the Moon and the increase of the AU could have origin in the same phenomena: the Sun's acceleration.

It could be interesting to calculate the Sun's acceleration in the direction of Sun's actual motion towards the solar apex, taking as a basis the Moon's change of eccentricity.
 
  • #27
maurol2 said:
This is consistent with an acceleration of the Earth. Which is in turn consistent with an acceleration of the Sun.

Show me the numbers. I'm not convinced :-) :-)

One of the papers on planet X that you cited goes through the calculations that you need to make in order to figure out the effect of accelerations on orbits.

These accelerations would also be consistent with an increase of the AU, so the increase of the eccentricity of the Moon and the increase of the AU could have origin in the same phenomena: the Sun's acceleration.

To make a case like that you have to present actual numbers, and demonstrate if there is X amount of acceleration of the sun you end up with X increase in eccentricity of the moon and Z increase in Earth's orbit. You then also can try to figure out that it results in effect A, which no one has looked for. Also you have to figure out how to explain the millisecond pulsars.

Now it would take about six months to work through all of the numbers, but if you do it and it ends up that all of them fit, then that's worth a paper. My guess is that once you work through the numbers, you'll find that an acceleration that causes the moon's eccentricity to behave in one way will cause the AU to behave in another. If that starts to happen, then you have to figure out how to turn lemons into lemonade.

The problem is that without doing actual calculations then anything is possible. That's why numbers are important in this game.

There are some practical reasons for getting this all right. Figuring out whether or not an asteroid is going to hit the Earth and where exactly it's going to hit requires extremely high precision orbital predictions. If you figure out that an asteroid is going to hit the earth, then the next thing to do is to figure out what direction to "nudge" it so that it gets out of the way.

It could be interesting to calculate the Sun's acceleration in the direction of Sun's actual motion towards the solar apex, taking as a basis the Moon's change of eccentricity.

I think there is enough information in the papers that you've cited to do that calculation, although doing it and getting it write is going to be *HARD*.

Also you need to read up more on the limits of acceleration of the solar system. If the *only* thing that puts limits on the solar system acceleration is miliisecond pulsars, then this would be easy to "break." On the other hand, I suspect that if you do a literature search you'll find a dozen other tests that create limits. Even if you don't find anything, you'll have to think of some on your own.
 
  • #28
Here's more data on lunar ranging

http://dda.harvard.edu/brouwer_award/BrouwerAward_2006_Williams.pdf

Something to point out is that we are talking about a really, really tiny effect (a few mm per year), and looking at the models, there are so many things that could cause the anomaly. It would be interesting to look through everything and make a list of everything that could cause the issue.
 
Last edited by a moderator:
  • #29
Also there is an effect called the "pigeon poop effect." When Penzias and Wilson first discovered the CMB radiation, their first guess was that they were looking at an equipment malfunction so they went in and among other things cleaned the telescope of pigeon poop. The reason for this is that if you start by claiming that your results may be the result of pigeon poop and then over time it becomes obvious that you really did discover something big, you look like a genius. Conversely, if you start by claiming that you discovered something big, but then it turns out that you didn't, you look foolish.

Something that you have to realize is that observations are hard to do and so is theory. One reason that it's a good idea to go through and try to calculate the effect of accelerations on planetary motions is that you'll find that it's hard to do, and you'll be spending at least a week going through all your calculations to make sure that you didn't mis-add two numbers.

Also observations are also prone to silly errors and mistakes. We are talking about incredibly small differences (a few mm/year) and it's quite possible that it will turn out to be something silly, like some technician on the floor below readjusting their equipment so things move a few mm/year or the size of the building changing in response to the air conditioning system.
 
  • #30
twofish-quant said:
Also there is an effect called the "pigeon poop effect." When Penzias and Wilson first discovered the CMB radiation, their first guess was that they were looking at an equipment malfunction so they went in and among other things cleaned the telescope of pigeon poop. The reason for this is that if you start by claiming that your results may be the result of pigeon poop and then over time it becomes obvious that you really did discover something big, you look like a genius. Conversely, if you start by claiming that you discovered something big, but then it turns out that you didn't, you look foolish.
You're right, of course. The short answer is: I couldn't care less :-)
The long answer is, that I'm not going to do all the calculations, because I don't have the time. I'm just pondering and throwing ideas here, because it looks like a good place to do it(mainly thanks to you, I must say), and the exchange seems useful.
Maybe some other guy at a later time would read this, and could be interested in doing all the number crunching.

Well, let's move on. Here's a related thing I want to mention:
In our recent talk regarding planet X (a talk that was expurgated and where posts were deleted, so I must repeat it here) I mentioned "dark matter" as a possible cause of the Sun's movement, and you said that a black hole would also be noticed, due to gravitational lensing and other effects.
I want to stress that when I mentioned "dark matter", I was talking about an actually unknown or undiscovered aspect of the way gravity(or another force, btw) works, not about a dark companion/black hole. That is, I understand "dark matter" as a way to say that we don't know what gravity is, and even how gravity works at long scales.
Related to that, I want to mention also: If the Sun is rotating around the galaxy at 220 km/s, and the distance to the center of the Milky Way is ~ 26000 light years, and assuming we're orbiting the galaxy in a circle(which sounds like a good approximation) the Sun must be subjected to a centripetal acceleration ac = v^2/r ~= 2 x 10^-10 m/s^2 (btw, this value is less, but close, to the limit based on millisecond pulsars)
Is this centripetal acceleration actually observed?
It could be interesting to analize this centripetal acceleration and its potential relation with the movement towards the Solar Apex, i.e. the movement towards the solar apex as a consequence of a wobbling or oscillation around the main direction of rotation. Picture the Sun and the solar system in a kind of circular(spiral, really) stream (the milky way arm in which are located), oscillating back and forth and up and down while they travel around the center of the galaxy. This would clearly talk about the galaxy as some kind of "sinking hole", and of gravity as a fluid. Maybe the gravity we know, that is, the gravity we tend to associate with matter, is only a part of the total phenomena, and there's another aspect of gravity that is not associated with matter(what we call "dark marker"), and which only manifests itself as a flow affecting the matter we can observe.

Regards,
Mauro
 
  • #31
maurol2 said:
Maybe some other guy at a later time would read this, and could be interested in doing all the number crunching.

My guess is that lots of people have already crunched the numbers, and they haven't found anything. If you crunch the numbers and you find something then you publish, but if you do it and you end up with nothing then you have nothing to publish.

I want to stress that when I mentioned "dark matter", I was talking about an actually unknown or undiscovered aspect of the way gravity(or another force, btw) works, not about a dark companion/black hole. That is, I understand "dark matter" as a way to say that we don't know what gravity is, and even how gravity works at long scales.

At large scales. People who do modified gravity theory put into their models the idea that at solar system scales, nothing the propose makes a difference. That's the idea behind f(R) and MOND models. All of them are set up so that at solar system scales, there is nothing weird, because if there were something really weird we would have noticed it. Yes there is an anomaly of a few mm each year, but there is no anomaly that is a few cm per year, and that puts huge limits on what you can get away with.

About centripetal acceleration. It looks like from the numbers that if we are just a bit more accurate about our measurements then we should be able to see some effects from galactic rotation. Also, if you

It could be interesting to analize this centripetal acceleration and its potential relation with the movement towards the Solar Apex, i.e. the movement towards the solar apex as a consequence of a wobbling or oscillation around the main direction of rotation. Picture the Sun and the solar system in a kind of circular(spiral, really) stream (the milky way arm in which are located), oscillating back and forth and up and down while they travel around the center of the galaxy.

This is likely to be what's going on. One thing that would be interesting to look at is to look at models of the suns motion through the spiral galaxy. and see what accelerations there are.

This would clearly talk about the galaxy as some kind of "sinking hole", and of gravity as a fluid. Maybe the gravity we know, that is, the gravity we tend to associate with matter, is only a part of the total phenomena, and there's another aspect of gravity that is not associated with matter(what we call "dark marker"), and which only manifests itself as a flow affecting the matter we can observe.

One thing that about dark matter is that there are a lot of different types of dark matter. Most of the ordinary matter in the universe is dark, and that would certainly have some effect on galactic motion.
 
  • #32
twofish-quant said:
My guess is that lots of people have already crunched the numbers, and they haven't found anything. If you crunch the numbers and you find something then you publish, but if you do it and you end up with nothing then you have nothing to publish.
Hi twofish-quant.
I'm not so sure about that. These anomalies are relatively recent.
And Iorio in fact did discovered something related to the retrograde perihelion of Saturn. Namely, that it could be explained by a mass outside the solar system, and (perhaps more importantly) if the mass is in the direction of the galactic center, their results are also consistent with MOND.

At large scales. People who do modified gravity theory put into their models the idea that at solar system scales, nothing the propose makes a difference. That's the idea behind f(R) and MOND models. All of them are set up so that at solar system scales, there is nothing weird, because if there were something really weird we would have noticed it. Yes there is an anomaly of a few mm each year, but there is no anomaly that is a few cm per year, and that puts huge limits on what you can get away with.
Again, Iorio apparently explained the anomalous motion of the perihelion of Saturn. This is a tiny effect(and is even yet to be confirmed) and the math is hard, but anyways, the effort loks very worthwhile.

One thing that about dark matter is that there are a lot of different types of dark matter. Most of the ordinary matter in the universe is dark, and that would certainly have some effect on galactic motion.

Dark matter could be not ordinary matter, but something else that we're only expecting to be ordinary matter, due to conceptual constraints.
In my opinion, it's necessary to disassociate gravity from ordinary matter(at least as an avenue for research), to (perhaps) be able to understand what's really going on.
Accumulation and acceleration of matter would then be a consequence of gravity, but gravity would not be a consequence of matter(which is also a logical dead-end, btw).
That is: accumulation/acceleration of matter is a manifestation of gravity, but there could be "gravity"(or something that behaves like gravity) without matter as a cause.
We tend to associate gravity with matter only because we're used to see gravity where there is matter, but, as you said before: most of the "matter" of the universe would not be ordinary matter. This is (at least potentially) equivalent as saying that there exists gravity without a material cause.
 
  • #33
twofish-quant said:
All of them are set up so that at solar system scales, there is nothing weird, because if there were something really weird we would have noticed it. Yes there is an anomaly of a few mm each year, but there is no anomaly that is a few cm per year, and that puts huge limits on what you can get away with.
You forgot the observed secular increase of the AU, inferred to be about 15 cm/yr.

But in general, your line of reasoning is not valid. That is, taking the mainstream model and trying to restrict
alternatives solely from the fact that the remaining anomalies are small, is not a useful exercise. There are
two main reasons for this. First, almost all observational results in astrophysics are indirect, i.e., the raw
data are analysed with some (mainstream) theoretical assumptions assumed to be valid. The numbers
thus obtained and cited as observational facts, are not completely general results, but inferred and theory-
dependent results. That is, change the theory and the numbers may change. This effect must be evaluated
from case to case - no general statements of how any alternative theory affects the results can be made.
Second, mainstream theory includes free parameters, some of which may absorb large effects predicted
from alternative theories. Unfortunately, it's a problem that free parameters may sometimes be treated as
independent facts, blocking the possibility that free parameters can be disposed of and replaced with
something else in an alternative theory.

The bottom line is that a little learning is indeed dangerous. That is, one should certainly study the
mainstream models thoroughly, so that one knows what theoretical assumptions are made when
analysing the data - just to get an idea of how general the results are. But one should also study alternative
models where crucial mainstream assumptions do not hold. Only by doing this can one really get an
impression of the size of effects one may get away with and still being consistent with observations.
If you do this, I believe that you would be surprised.
 
Last edited:

1. What is angular velocity?

Angular velocity is a measure of how fast an object is rotating or moving in a circular motion. It is measured in radians per second (rad/s) or degrees per second (deg/s).

2. How does the Earth's rotation affect the length of a day?

The Earth's rotation on its axis is what causes day and night. However, due to the gravitational pull of the Moon and other celestial bodies, the Earth's rotation is gradually slowing down. This means that days are getting longer by about 1.7 milliseconds per century.

3. What is precession and how does it affect the Earth's axis?

Precession is the gradual change in the direction of the Earth's axis of rotation. This is caused by the gravitational pull of the Sun and Moon on the Earth's equatorial bulge. As a result, the Earth's axis traces out a cone shape, completing a full cycle every 26,000 years.

4. What is the difference between a solar day and a sidereal day?

A solar day is the time it takes for the Sun to return to the same position in the sky, which is about 24 hours. A sidereal day is the time it takes for the Earth to make one full rotation on its axis, which is about 23 hours and 56 minutes. This difference is due to the Earth's orbit around the Sun.

5. How do the motions of the planets affect their orbital periods?

The orbital period of a planet is determined by its distance from the Sun and its orbital speed, which is affected by the gravitational pull of the Sun and other planets. The closer a planet is to the Sun, the faster it orbits and the shorter its orbital period. The farther away a planet is, the slower it orbits and the longer its orbital period.

Similar threads

  • Astronomy and Astrophysics
Replies
4
Views
2K
  • Sci-Fi Writing and World Building
Replies
21
Views
1K
Replies
5
Views
222
  • Astronomy and Astrophysics
Replies
1
Views
2K
  • Engineering and Comp Sci Homework Help
Replies
3
Views
1K
  • Astronomy and Astrophysics
Replies
2
Views
3K
  • Astronomy and Astrophysics
Replies
8
Views
3K
  • Astronomy and Astrophysics
Replies
12
Views
3K
  • Astronomy and Astrophysics
2
Replies
43
Views
58K
  • Sci-Fi Writing and World Building
Replies
10
Views
2K
Back
Top