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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
It has not escaped my attention that one cannot revise the distance to
SgrA* without revising the Cepheid scale and with it the value of Hubble's constant, and I have been revising the numerical parameters describing the teleconnection cosmology. There is some reason to think the "best" standard distance for SgrA* may be nearer to 7.5kpc, rather than 8kpc - not least imv that I think this is the distance at which SgrA* must be if it stationary at the galactic barycentre as I would expect of such a massive object, rather than bouncing up and down through the galactic plane. At this distance the solar velocity would be 227km/s, rather than 242km/s. There is a certain flexibility in fitting the rotation curve, but I find I get a reasonable fit based on the teleconnection with a distance of 6kpc. At this distance the true solar velocity would be 181km/s, and the illusory part of Doppler velocity would ~55km/s, making an apparent solar velocity of ~235km/s, consistent with observations based on Doppler. If one revises down the Cepheid scale proportionately, by 20%, then one needs to revise up Hubble's constant by 25%. The current popular value of 71 then becomes 88. This ties in with two other predictions of the teleconnection, that the Pioneer acceleration is Hc, and the characteristic MOND acceleration is Hc/8. The measured Pioneer drift is 2.92+-0.44 x 10^-18 s/s^2, while the value corresponding to H0=71 is 2.33 x 10^-18/s, marginally consistent, but not close. After revising H0 upward by 25% one finds 2.91 x 10^-18 /s, extremely close to the Pioneer value (I didn't understand the error bounds quoted by JPL; as I recall their measurements appeared much more accurate). One also finds the precise value of the measured characteristic MOND acceleration, H0c/8 = 1 x 10^-8 cm/s^2. It is also necessary to revise the age of the universe. Using H0=88, together with Omega=1.9, which I had from supernova fits to a no Lambda model, I get from Ned Wright's calculator an age of 12.85 Gyr, just under the age I get for a standard Lambda model with Omega = 3, i.e. 13.3 Gyr. That's a little short on the age of the oldest stars in the Milky way, 13.4+-0.8, but within bounds and none of these figures can be all that precise. What is probably more important is that the predicted age now agrees well with the age necessary to the observed proton- neutron ratio which is quite tightly constrained by the rate of expansion during big bang nucleosynthesis. I haven't worked out the effect on the Great Attractor, but one estimates that we are not moving quite so fast toward M31 and that the Great Attractor will be not quite so great after making all corrections. If it wasn't all so darn complicated, what I would really like to do is work out the effect on WMAP and see if I could account for the alignments in the data. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
On 22 Mar, 11:40, Oh No wrote:
If one revises down the Cepheid scale proportionately, by 20%, then one needs to revise up Hubble's constant by 25%. The current popular value of 71 then becomes 88. This ties in with two other predictions of the teleconnection, that the Pioneer acceleration is Hc, ... I thought when we last discussed the Pioneer anomaly you finally agreed that the classical prediction was A_p = 2 H v where v is the speed of the craft? You said your theory then gave a value half of the classical version. The prediction is about 3 orders less than is measured which is comparable to v/c hence Anderson et al note the similarity of Ap to Hc but only as a coincidence. George |
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{!!! SPAM ???} The distance to Sgr A*, Hubble's Constant, and Pioneer drift
Thus spake "
On 22 Mar, 11:40, Oh No wrote: If one revises down the Cepheid scale proportionately, by 20%, then one needs to revise up Hubble's constant by 25%. The current popular value of 71 then becomes 88. This ties in with two other predictions of the teleconnection, that the Pioneer acceleration is Hc, ... I thought when we last discussed the Pioneer anomaly you finally agreed that the classical prediction was A_p = 2 H v where v is the speed of the craft? You said your theory then gave a value half of the classical version. No, I recognised that I had been in error when I had previously said that I calculated half of the classical version, and that I needed to revise my argument. The correct argument turned out to be much simpler. I can't remember if I posted it here. I had overlooked it because of a trivial mistake in signs, a particular bugbear of mine. When the classical momentum of pioneer is parallel displaced to an observer on earth it obeys p_observed/a(t1)^2 = p_actual/a^2(t0) Where t0 is the time when lock is lost. Then p_observed = (1 + H0*(t1 - t0)) p_actual So what is measured is a frequency drift toward the blue. My confusion arose because the sign is opposite to the cosmological redshift which applies to photon momentum between emission and reception, but which is negligible here. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
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{!!! SPAM ???} {!!! SPAM ???} The distance to Sgr A*, Hubble's Constant, and Pioneer drift
On 22 Mar, 13:59, Oh No wrote:
Thus spake " On 22 Mar, 11:40, Oh No wrote: If one revises down the Cepheid scale proportionately, by 20%, then one needs to revise up Hubble's constant by 25%. The current popular value of 71 then becomes 88. This ties in with two other predictions of the teleconnection, that the Pioneer acceleration is Hc, ... I thought when we last discussed the Pioneer anomaly you finally agreed that the classical prediction was A_p = 2 H v where v is the speed of the craft? You said your theory then gave a value half of the classical version. No, I recognised that I had been in error when I had previously said that I calculated half of the classical version, and that I needed to revise my argument. The correct argument turned out to be much simpler. I can't remember if I posted it here. I had overlooked it because of a trivial mistake in signs, a particular bugbear of mine. When the classical momentum of pioneer is parallel displaced to an observer on earth it obeys p_observed/a(t1)^2 = p_actual/a^2(t0) Where t0 is the time when lock is lost. Then p_observed = (1 + H0*(t1 - t0)) p_actual So what is measured is a frequency drift toward the blue. My confusion arose because the sign is opposite to the cosmological redshift which applies to photon momentum between emission and reception, but which is negligible here. What is t1? Lock times are tricky because cycle slips could occur but contacts usually lasted around 4 hours from memory. If the above equation relates to a single contact, how do you translate that for the fit over many years? George |
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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
Thus spake "
On 22 Mar, 13:59, Oh No wrote: Thus spake " On 22 Mar, 11:40, Oh No wrote: If one revises down the Cepheid scale proportionately, by 20%, then one needs to revise up Hubble's constant by 25%. The current popular value of 71 then becomes 88. This ties in with two other predictions of the teleconnection, that the Pioneer acceleration is Hc, ... I thought when we last discussed the Pioneer anomaly you finally agreed that the classical prediction was A_p = 2 H v where v is the speed of the craft? You said your theory then gave a value half of the classical version. No, I recognised that I had been in error when I had previously said that I calculated half of the classical version, and that I needed to revise my argument. The correct argument turned out to be much simpler. I can't remember if I posted it here. I had overlooked it because of a trivial mistake in signs, a particular bugbear of mine. When the classical momentum of pioneer is parallel displaced to an observer on earth it obeys p_observed/a(t1)^2 = p_actual/a^2(t0) Where t0 is the time when lock is lost. Then p_observed = (1 + H0*(t1 - t0)) p_actual So what is measured is a frequency drift toward the blue. My confusion arose because the sign is opposite to the cosmological redshift which applies to photon momentum between emission and reception, but which is negligible here. What is t1? Lock times are tricky because cycle slips could occur but contacts usually lasted around 4 hours from memory. t1 is the time when a signal is observed on Earth. If the above equation relates to a single contact, how do you translate that for the fit over many years? Sorry, I was ambiguous. I was referring to the loss of radar lock. While radar lock is maintained the matter on Pioneer has particular defined classical relationship with matter on earth. Once it is lost, that relationship is lost too. Nothing changes with respect to the physics obeyed by Pioneer, but the relationship between reference frames defined at Pioneer and at Earth is altered. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
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{!!! SPAM ???} The distance to Sgr A*, Hubble's Constant, and Pioneer drift
"Oh No" wrote in message
... Thus spake " On 22 Mar, 13:59, Oh No wrote: ..... No, I recognised that I had been in error when I had previously said that I calculated half of the classical version, and that I needed to revise my argument. The correct argument turned out to be much simpler. I can't remember if I posted it here. I had overlooked it because of a trivial mistake in signs, a particular bugbear of mine. When the classical momentum of pioneer is parallel displaced to an observer on earth it obeys Fair enough but what follows still doesn't derive the anomaly in the form A_p. p_observed/a(t1)^2 = p_actual/a^2(t0) Where t0 is the time when lock is lost. Then p_observed = (1 + H0*(t1 - t0)) p_actual So what is measured is a frequency drift toward the blue. My confusion arose because the sign is opposite to the cosmological redshift which applies to photon momentum between emission and reception, but which is negligible here. What is t1? Lock times are tricky because cycle slips could occur but contacts usually lasted around 4 hours from memory. t1 is the time when a signal is observed on Earth. If the above equation relates to a single contact, how do you translate that for the fit over many years? Sorry, I was ambiguous. I was referring to the loss of radar lock. While radar lock is maintained the matter on Pioneer has particular defined classical relationship with matter on earth. Once it is lost, that relationship is lost too. Nothing changes with respect to the physics obeyed by Pioneer, but the relationship between reference frames defined at Pioneer and at Earth is altered. So what does that mean? Perhaps you are saying that during any one contact there would be no apparent anomaly (though of course it is too small to check) and that the 'acceleration' is in the form of discrete steps in apparent velocity that occur between the end of one contact and the beginning of the next. If that is the case, the apparent speed error must be frozen into the system at the signal acquisition time and hence independent of the duration of the contact. To look like a constant acceleration, the error must also be proportional to the time since the start of the mission and independent of the time since the last contact. Your equations only contain lock times, not the time since the mission start. You say above that you cannot remember if you posted it and certainly I have never seen any derivation at all that explained your claim. Can you start with a clear set of definitions and show the derivation fully through to getting A_p = H_0 * c ? From what I have seen so far, you aren't going to be able to do that because nothing in any of your equations relates to the mission time but you hev never posted the whole thing, just unconnected snippets. George |
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{!!! SPAM ???} The distance to Sgr A*, Hubble's Constant, and Pioneer drift
Thus spake George Dishman
"Oh No" wrote in message ... Sorry, I was ambiguous. I was referring to the loss of radar lock. While radar lock is maintained the matter on Pioneer has particular defined classical relationship with matter on earth. Once it is lost, that relationship is lost too. Nothing changes with respect to the physics obeyed by Pioneer, but the relationship between reference frames defined at Pioneer and at Earth is altered. So what does that mean? Perhaps you are saying that during any one contact there would be no apparent anomaly (though of course it is too small to check) and that the 'acceleration' is in the form of discrete steps in apparent velocity that occur between the end of one contact and the beginning of the next. No, I don't think so. If that is the case, the apparent speed error must be frozen into the system at the signal acquisition time and hence independent of the duration of the contact. To look like a constant acceleration, the error must also be proportional to the time since the start of the mission and independent of the time since the last contact. Your equations only contain lock times, not the time since the mission start. It must be linear with the time since start of mission, not proportional to it. I have it as proportional to the time since loss of radar lock. Can you start with a clear set of definitions and show the derivation fully through to getting A_p = H_0 * c ? From what I have seen so far, you aren't going to be able to do that because nothing in any of your equations relates to the mission time but you hev never posted the whole thing, just unconnected snippets. I'll work on something. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
Oh No wrote:
There is some reason to think the "best" standard distance for SgrA* may be nearer to 7.5kpc, rather than 8kpc ..... I get a reasonable fit based on the teleconnection with a distance of 6kpc. If you decrease the GC distance by 20%, you decrease the globular cluster distances by the same factor. That decreases the stellar luminosity at the main sequence turnoff by 40%, mass at the turnoff by about 12%, and increases the stellar age by something like 25% or 3 Gyr. That seems uncomfortable. I'm still unclear on what your predictions say about radial velocities. If there's a cluster of stars at the GC that has a true average radial velocity of zero and radial velocity dispersion of 100 km/s, what values will be measured by standard Doppler techniques at Earth? |
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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
Thus spake Steve Willner
Oh No wrote: There is some reason to think the "best" standard distance for SgrA* may be nearer to 7.5kpc, rather than 8kpc .... I get a reasonable fit based on the teleconnection with a distance of 6kpc. If you decrease the GC distance by 20%, you decrease the globular cluster distances by the same factor. That decreases the stellar luminosity at the main sequence turnoff by 40%, mass at the turnoff by about 12%, and increases the stellar age by something like 25% or 3 Gyr. That seems uncomfortable. Interesting. I have other reasons for thinking my original estimate may be a little much. There is quite a lot of balancing to be done, but some flexibility because error margins are not that tight. I'm still unclear on what your predictions say about radial velocities. If there's a cluster of stars at the GC that has a true average radial velocity of zero and radial velocity dispersion of 100 km/s, what values will be measured by standard Doppler techniques at Earth? It's not a simple relationship, but the illusory component of radial velocity decreases toward the galactic centre. Unfortunately, I don't have a precise general solution, and toward the centre it will depend on mass distribution. ATM I am still working with estimates. At our distance the illusory component is about 25% of the true distance. As the sun is moving toward the galactic centre at about 10km/s, I believe that will contribute about 2.5km/s, which will be an offset for the average velocity of the cluster. For the velocity dispersion, I think there will be at most 10% illusory component. I have started to look at globular clusters, and there is an interesting trend in the rotational velocities which appears to confirm this. The apparent average rotational velocity goes from about 50km/s retrograde for clusters far from the galactic centre to about 100km/s prograde near the galactic centre. Very preliminary calculations - don't put too much on them just yet. Regards -- Charles Francis moderator sci.physics.foundations. substitute charles for NotI to email |
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The distance to Sgr A*, Hubble's Constant, and Pioneer drift
If there's a cluster of stars at the GC that has a true
average radial velocity of zero and radial velocity dispersion of 100 km/s, what values will be measured by standard Doppler techniques at Earth? Oh No wrote: It's not a simple relationship, but the illusory component of radial velocity decreases toward the galactic centre. Unfortunately, I don't have a precise general solution, and toward the centre it will depend on mass distribution. ATM I am still working with estimates. At our distance the illusory component is about 25% of the true distance. As the sun is moving toward the galactic centre at about 10km/s, I believe that will contribute about 2.5km/s, which will be an offset for the average velocity of the cluster. For the velocity dispersion, I think there will be at most 10% illusory component. It won't have escaped you that I was describing the maser technique for determining Galactic center distance. If you want the distance to be smaller, the observed radial velocity _dispersion_ has to be _larger_ than the true radial velocity dispersion. The magnitude of the radial velocity itself is irrelevant for the distance determination. |
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