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The Pioneer Anomaly
mike
post Nov 9 2005, 09:42 PM
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That's what a theory is.
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elakdawalla
post Nov 10 2005, 01:29 AM
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QUOTE (deglr6328 @ Oct 3 2005, 02:53 AM)
sooooo did the planetary soc. get the data or what...? They haven't updated on us the status of thier original $250K begathon since like March.
*

smile.gif We've been a little preoccupied!

There are updates on our website here, including reports from a staff member who we sent to the conference in Switzerland:
http://www.planetary.org/programs/projects...ly/updates.html
And "begathon"...I like it...captures the tone of those four-page letters nicely...

--Emily


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Guest_Myran_*
post Nov 10 2005, 05:21 AM
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Guests






QUOTE
Richard Trigaux said: I wonder if we could do any theory of any kind, adjust parametres and obtain a fit with anything.

But if the fit goes for not only Pioneer data, but all similar data, it is more intersting. Not an evidence of any given theory, but a last of a common mechanism.


Yes, why I was somewhat vary of the idea of a "fifth force" suggested here.
I like things bare bones simple, and so a strong supporter that Occam sharpen his blade.
So when MOND theory originally for explaining the rotation of galaxies also turned out to fit for the much closer Pioneer I happily accepted the notion that there might be something more that makes this idea deserves attention.
(Note: I originally read about the theory in Scientific American, and got interested in it.)
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lyford
post Nov 10 2005, 06:41 AM
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Call me old fashioned, but I am a bit wary of jettisoning the "old physics" when the effects are at what I understand to be the threshold of detection, and we really don't know what the environment the little guys are swimming in right now is like - we may need to look for a new theory of interstellar wind before altering the laws of motion.

Still it is fun to think about - and it IS possible I suppose -

This page from the Planetary Society puts it well:
QUOTE
The simple engineering explanation cannot yet be ruled out, but enough work has been done in trying all the different possibilities that even Occam's Razor allows us to cut a little way into the idea of a new physics.


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ljk4-1
post Nov 10 2005, 02:33 PM
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QUOTE (elakdawalla @ Nov 9 2005, 08:29 PM)
smile.gif We've been a little preoccupied!

There are updates on our website here, including reports from a staff member who we sent to the conference in Switzerland:
http://www.planetary.org/programs/projects...ly/updates.html
And "begathon"...I like it...captures the tone of those four-page letters nicely...

--Emily
*


Dear Emily,

Speaking of TPS-funded projects, what has happened with Project BETA? Was the Harvard dish ever repaired? If not, is there an alternate plan to keep BETA running? Or is everything focused on Optical SETI now? And what has happened with that project lately?

Thank you.


--------------------
"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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The Messenger
post Nov 10 2005, 04:44 PM
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QUOTE (lyford @ Nov 9 2005, 11:41 PM)
Call me old fashioned, but I am a bit wary of jettisoning the "old physics" when the effects are at what I understand to be the threshold of detection, and we really don't know what the environment the little guys are swimming in right now is like - we may need to look for a new theory of interstellar wind before altering the laws of motion. 

Still it is fun to think about - and it IS possible I suppose -

Pioneer 10 & 11 are not the only odd-ball observations, and I am not talking about rocks that look like a pock-marked Elvis.

Pioneer 6 charted heavy Doppler residuals, and a linear component (similar to the term used in this paper) had to be added to the solar wind to plot both Galileo and Ulysses during interplanetary transitions. There is a possibility that when all the dots are connected, something fundamental will jump out of the wood work.
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elakdawalla
post Nov 10 2005, 04:46 PM
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QUOTE (ljk4-1 @ Nov 10 2005, 07:33 AM)
Dear Emily, Speaking of TPS-funded projects, what has happened with Project BETA?  Was the Harvard dish ever repaired?  If not, is there an alternate plan to keep BETA running?  Or is everything focused on Optical SETI now?  And what has happened with that project lately? Thank you.
*

That's a good question, and I don't know the answer, and the SETI areas of our website have suffered a bit through the redesign process. We should have answers for you there and we don't. I'll try to follow up. Amir Alexander here at the Society is the one who does SETI, I'll see if he can answer your question.

--Emily


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lyford
post Nov 10 2005, 10:06 PM
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QUOTE (The Messenger @ Nov 10 2005, 08:44 AM)
Pioneer 10 & 11 are not the only odd-ball observations.... (edit) ....There is a possibility that when all the dots are connected, something fundamental will jump out of the wood work.
*

True, but we have too few dots right now, and this is another great reason to have more outer solar system missions!

Though, infuriatingly, we will have to wait quite a long time for a return on investment, even for the New Horizons data.

I don't mean to imply that only odd balls that make odd ball observations, and I realize an anomaly to be explained can be a doorway to new understanding - Black Body Radiation anyone?

I find it fascinating nonetheless that the universe is understandable at all, and if you think about it, Science has only had a few centuries to explore the entire span of space time from our little home here. I am sure there are plenty of surprises in store. tongue.gif


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"Zis is not nuts, zis is super-nuts!" Mathematician Richard Courant on viewing an Orion test
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ljk4-1
post Dec 20 2005, 04:05 PM
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Astrophysics, abstract
astro-ph/0505310

From: Michael A. Ivanov [view email]

Date (v1): Sat, 14 May 2005 19:34:27 GMT (122kb)
Date (revised v2): Mon, 19 Dec 2005 16:23:51 GMT (124kb)

Low-energy quantum gravity leads to another picture of the universe

Authors: Michael A. Ivanov

Comments: 13 pages, 4 figures, LaTeX. Contribution to the 1st Crisis in
Cosmology Conference (CCC-1), Moncao, Portugal, 23-25 June 2005. A computational error amd some misprints are corrected in this version

If gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false: a full magnitude of cosmological redshift would be caused by interactions of photons with gravitons. Non-forehead collisions with gravitons will lead to a very specific additional relaxation of any photonic flux that gives a possibility of another interpretation of supernovae 1a data - without any kinematics. These facts may implicate a necessity to change the standard cosmological paradigm. Some features of a new paradigm are discussed. In a frame of this model, every observer has two different cosmological horizons. One of them is defined by maximum existing temperatures of remote sources - by big enough distances, all of them will be masked with the CMB radiation. Another, and much smaller, one depends on their maximum luminosity - the luminosity distance increases with a redshift much quickly than the geometrical one.

If the considered quantum mechanism of classical gravity is realized in the nature, then an existence of black holes contradicts to the equivalence principle. In this approach, the two fundamental constants - Hubble's and Newton's ones - should be connected between themselves. The theoretical value of the Hubble constant is computed. Also, every massive body would be decelerated due to collisions with gravitons that may be connected with the Pioneer 10 anomaly.

http://arXiv.org/abs/astro-ph/0505310


--------------------
"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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ljk4-1
post Jan 3 2006, 02:31 AM
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General Relativity and Quantum Cosmology, abstract
gr-qc/0512121

From: Slava G. Turyshev [view email]

Date: Wed, 21 Dec 2005 21:49:36 GMT (882kb)

The Study of the Pioneer Anomaly: New Data and Objectives for New Investigation

Authors: Slava G. Turyshev, Viktor T. Toth, Larry R. Kellogg, Eunice. L. Lau, Kyong J. Lee

Comments: 42 pages, 40 figures, 3 tables

Radiometric tracking data from Pioneer 10 and 11 spacecraft has consistently indicated the presence of a small, anomalous, Doppler frequency drift, uniformly changing with a rate of ~6 x 10^{-9} Hz/s; the drift can be interpreted as a constant sunward acceleration of each particular spacecraft of a_P = (8.74 \pm 1.33) x 10^{-10} m/s^2. This signal is known as the Pioneer anomaly; the nature of this anomaly remains unexplained. We discuss the efforts to retrieve the entire data sets of the Pioneer 10/11 radiometric Doppler data. We also report on the recently recovered telemetry files that may be used to reconstruct the engineering history of both spacecraft using original project documentation and newly developed software tools. We discuss possible ways to further investigate the discovered effect using these telemetry files in conjunction with the analysis of the much extended Doppler data. We present the main objectives of new upcoming study of the Pioneer anomaly, namely i) analysis of the early data that could yield the direction of the anomaly, ii) analysis of planetary encounters, that should tell more about the onset of the anomaly, iii) analysis of the entire dataset, to better determine the anomaly's temporal behavior, iv) comparative analysis of individual anomalous accelerations for the two Pioneers, v) the detailed study of on-board systematics, and vi) development of a thermal-electric-dynamical model using on-board telemetry. The outlined strategy may allow for a higher accuracy solution for a_P and, possibly, will lead to an unambiguous determination of the origin of the Pioneer anomaly.

http://arxiv.org/abs/gr-qc/0512121


--------------------
"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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tfisher
post Jan 3 2006, 07:10 AM
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I just read through the last paper linked. They've done quite well at recovering a complete data set, including telemetry data like temperature and voltage readouts useful for reconstructing thermal contributions to the Pioneers' accelerations. Another cool tidbit: there is one last opportunity to attempt to contact Pioneer 10, coming up in this February/March. (They think that, just barely maybe there is enough power still now in the old RTGs...) The round-trip light-time is 25 hours, so the contact would proceed by sending out a signal from Goldstone, waiting a day while the earth spins around once and the radio waves make their merry way, and listening for a response again at Goldstone. Somehow that image amuses me :^)
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ljk4-1
post Jan 4 2006, 06:18 PM
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Paper: astro-ph/0504367

Date (v1): Sun, 17 Apr 2005 17:04:48 GMT (32kb)
Date (revised v2): Sat, 1 Oct 2005 13:46:27 GMT (43kb)
Date (revised v3): Mon, 2 Jan 2006 16:12:03 GMT (36kb)

replaced with revised version Mon, 2 Jan 2006 16:12:03 GMT (36kb)

Title: Can Minor Planets be Used to Assess Gravity in the Outer Solar System?

Authors: Gary L. Page, David S. Dixon, John F. Wallin

Comments: Accepted for publication in The Astrophysical Journal

The twin Pioneer spacecraft have been tracked for over thirty years as they headed out of the solar system. After passing 20 AU from the Sun, both exhibited a systematic error in their trajectories that can be interpreted as a constant acceleration towards the Sun. This Pioneer Effect is most likely explained by spacecraft systematics, but there have been no convincing arguments that that is the case.

The alternative is that the Pioneer Effect represents a real phenomenon and perhaps new physics. What is lacking is a means of measuring the effect, its variation, its potential anisotropies, and its region of influence.

We show that minor planets provide an observational vehicle for investigating the gravitational field in the outer solar system, and that a sustained observation campaign against properly chosen minor planets could confirm or refute the existence of the Pioneer Effect.

Additionally, even if the Pioneer Effect does not represent a new physical phenomenon, minor planets can be used to probe the gravitational field in the outer Solar System and since there are very few intermediate range tests of gravity at the multiple AU distance scale, this is a worthwhile endeavor in its own right.

\\ ( http://arXiv.org/abs/astro-ph/0504367 , 36kb)


--------------------
"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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tasp
post Jan 5 2006, 04:14 AM
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I bet it is not as simple as this, but I will post an idea and watch it be shredded . . .

blink.gif

Any possibility either Voyager craft could be spun at a few revs per hour, with the thrusters turned off, and keep the dish pointed at earth for maybe a year or two?

My thought is if we could get a confirmation of the Pioneer anomaly with a Voyager craft it might help JPL design a more capable or sophisticated 'Pioneer Anomally Probe' someday.

With the 'nodding' motion compensation used at Triton, I am cautiously optimistic that there might still be a new trick for our favorite 'old dog' to learn.

Having a spin stabilised period of flight for a Voyager might yield enough high quality tracking data at what would have to be an attractive price compared to launching another probe designed for the task.

Besides, I'm getting old and would like this mystery cleared up while I am still around . . .
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mchan
post Jan 5 2006, 06:06 AM
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QUOTE (tasp @ Jan 4 2006, 08:14 PM)
Any possibility either Voyager craft could be spun at a few revs per hour, with the thrusters turned off, and keep the dish pointed at earth for maybe a year or two?
*


One problem is that something that was not designed to be spin stabilized (like Voyager) would very likely not spin very well. E.g. the spin axis would move around. In the case of Voyager, a stable spin axis (is such exists) may not align with the axis if the high gain antenna.
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ugordan
post Jan 5 2006, 08:52 AM
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QUOTE (mchan @ Jan 5 2006, 07:06 AM)
One problem is that something that was not designed to be spin stabilized (like Voyager) would very likely not spin very well.  E.g. the spin axis would move around.  In the case of Voyager, a stable spin axis (is such exists) may not align with the axis if the high gain antenna.
*

Wasn't the spacecraft-solid rocket stack spin stabilized for the duration of the rocket's burn during Jupiter injection or was it also in 3-axis stabilization mode? I would have figured delivery errors would be minimized by spinning up first.

Another possible problem with spin-stabilizing is the star sensor, would it be able to cope with starfield smearing during rotation?


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