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| Tags: but, dilation, recession, redshift, speed, time |
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#11
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"Roland PJ" wrote in message ups.com... On Jun 24, 10:33 am, wrote: On Jun 24, 12:01 am, Roland PJ wrote: Red-shiftof distant objects could be due to ... 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. How does your theory explains the fact that thered-shiftis larger for galaxies that are farther away? Should you assume that far galaxies are more massive? It depends what you've used to determine that the galaxies are further away. Have you used brightness? If so, then you haven't eliminated the possibility that both the dimness _and_ the red-shift are due to the galaxy being not necessarily further away, but either denser (more tightly packed with stars), or more massive. And note that using brightness seems to be the first rung in the standard 'distance ladder' of cosmological measurement. Roland Certain types of star are known to have a certain brightness.... http://hubblesite.org/newscenter/arc.../49/astrofile/ "Two well-defined primary distance indicators, or "standard candles," are the Cepheids and fainter RR Lyrae stars. They have a regular variation in brightness, and the period of this pulsation is closely linked to the star's intrinsic brightness. So, if the pulsation period of a star is known, its true brightness can be deduced. The distance to the star can then be calculated by comparing its true brightness with its apparent brightness." |
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#12
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"Roland PJ" wrote in message oups.com... What I'm asking is why the history of cosmological distance measurement (the 'distance ladder') seems to ignore it completely, and focus only on recession speed. That can't be right, can it? Focus is not only on recession speed.. http://hubblesite.org/newscenter/arc.../49/astrofile/ "Two well-defined primary distance indicators, or "standard candles," are the Cepheids and fainter RR Lyrae stars. They have a regular variation in brightness, and the period of this pulsation is closely linked to the star's intrinsic brightness. So, if the pulsation period of a star is known, its true brightness can be deduced. The distance to the star can then be calculated by comparing its true brightness with its apparent brightness." |
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#13
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On Jun 24, 1:20 pm, "CWatters"
wrote: "Roland PJ" wrote in message ups.com... On Jun 24, 10:33 am, wrote: On Jun 24, 12:01 am, Roland PJ wrote: Red-shiftof distant objects could be due to ... 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. How does your theory explains the fact that thered-shiftis larger for galaxies that are farther away? Should you assume that far galaxies are more massive? It depends what you've used to determine that the galaxies are further away. Have you used brightness? If so, then you haven't eliminated the possibility that both the dimness _and_ the red-shift are due to the galaxy being not necessarily further away, but either denser (more tightly packed with stars), or more massive. And note that using brightness seems to be the first rung in the standard 'distance ladder' of cosmological measurement. Roland Certain types of star are known to have a certain brightness.... http://hubblesite.org/newscenter/arc.../49/astrofile/ "Two well-defined primary distance indicators, or "standard candles," are the Cepheids and fainter RR Lyrae stars. They have a regular variation in brightness, and the period of this pulsation is closely linked to the star's intrinsic brightness. So, if the pulsation period of a star is known, its true brightness can be deduced. The distance to the star can then be calculated by comparing its true brightness with its apparent brightness." That may be true for observers at the same GR time-dilation as the Cepheid stars, but if a Cepheid is close to a large and/or dense mass, then we, on earth, will observe the period to be longer, and the brightness to be less, both to tue GR time-dilation. Unfortunately for this 'standard candle', these errors don't cancel out, but rather compound each other. A Cepheid with a longer observed period is deemed to be intrinsically brighter, and when we observe it to be dimmer than it is (due to GR time-dilation), we will interpret the longer period and lower brightness as indicating the star is significantly further than it really is. In the limit case of a Cepheid orbiting a near-black-hole, this error compounds essentially towards infinity. Of course, we don't observer the near-black-hole cos it's red-shifted and dimmed off the scale. We only see the Cepheid. Thoughts? Roland |
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#14
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On Jun 24, 2:51 pm, Roland PJ wrote:
On Jun 24, 1:20 pm, "CWatters" wrote: "Roland PJ" wrote in message oups.com... On Jun 24, 10:33 am, wrote: On Jun 24, 12:01 am, Roland PJ wrote: Red-shiftof distant objects could be due to ... 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. How does your theory explains the fact that thered-shiftis larger for galaxies that are farther away? Should you assume that far galaxies are more massive? It depends what you've used to determine that the galaxies are further away. Have you used brightness? If so, then you haven't eliminated the possibility that both the dimness _and_ the red-shift are due to the galaxy being not necessarily further away, but either denser (more tightly packed with stars), or more massive. And note that using brightness seems to be the first rung in the standard 'distance ladder' of cosmological measurement. Roland Certain types of star are known to have a certain brightness.... http://hubblesite.org/newscenter/arc.../49/astrofile/ "Two well-defined primary distance indicators, or "standard candles," are the Cepheids and fainter RR Lyrae stars. They have a regular variation in brightness, and the period of this pulsation is closely linked to the star's intrinsic brightness. So, if the pulsation period of a star is known, its true brightness can be deduced. The distance to the star can then be calculated by comparing its true brightness with its apparent brightness." That may be true for observers at the same GR time-dilation as the Cepheid stars, but if a Cepheid is close to a large and/or dense mass, then we, on earth, will observe the period to be longer, and the brightness to be less, both to tue GR time-dilation. Unfortunately for this 'standard candle', these errors don't cancel out, but rather compound each other. A Cepheid with a longer observed period is deemed to be intrinsically brighter, and when we observe it to be dimmer than it is (due to GR time-dilation), we will interpret the longer period and lower brightness as indicating the star is significantly further than it really is. In the limit case of a Cepheid orbiting a near-black-hole, this error compounds essentially towards infinity. Of course, we don't observer the near-black-hole cos it's red-shifted and dimmed off the scale. We only see the Cepheid. Thoughts? Roland Interesting. The question is observational.. what are the distributions of cepheids and other standard candles such as supernovae that have been measured with parallax? How good is the luminosity - period relationship really? |
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#15
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On Jun 24, 3:01 am, Roland PJ wrote:
Red-shift of distant objects could be due to two different reasons: 1. Recession speed away from the earth, a special relativistic effect. 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. It seems that most discussion of red-shift centres around the assumption that SR recession is the cause (and hence that the universe is expanding). Why has GR time dilation been eliminated as a cause? So, why should most objects exhibit a red-shift, rather than a neutral average shift? My best answer is that we, on earth, are at the edge of our galaxy (the milky way), and hence quite far from the concentration of mass near the centre of our galaxy. On the other hand, most matter (stars) in the universe are close to the centre of their galaxies, so, on average, most objects should exhibit a red-shift to us on earth. A corollary of this is that stars near the centre of our own galaxy (the milky way) should also exhibit red-shift to us (even though they are clearly not moving away from us on average). This should be testable, although I'm not sure how one would identify a bright object as a star in the center of our galaxy, rather than a distant object shining through (brightness?). Hubble, Edwin, "A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae" (1929) Proceedings of the National Academy of Sciences of the United States of America, Volume 15, Issue 3, pp. 168-173 Note that Hubble (and presumably all that follow) use _luminosity_ as a measure of _distance_. However, luminosity is actually also a measure of GR time dilation, independent of distance, as described above. Just some ideas. Flame away ![]() Roland So you're suggesting that objects in the universe become more massive the further away from us they are located? And, since our view of the universe isn't considered to be very special, how would you reconcile that with the notion that the mass distribution of the universe must be observer independent? |
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#16
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Dear Roland PJ:
"Roland PJ" wrote in message oups.com... Red-shift of distant objects could be due to two .... or more ... different reasons: 1. Recession speed away from the earth, a special relativistic effect. .... also just classical Doppler. 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. No. We can measure gravitational time dialtion in the spectrum of the sources. Distant sources are more redshifted... regardless of their mass, only their distance. It seems that most discussion of red-shift centres around the assumption that SR recession is the cause (and hence that the universe is expanding). Absolutely incorrect. SR is limited to evaluating jets of ejected material. It is GR that is used to describe expansion, and the Hubble shift. Why has GR time dilation been eliminated as a cause? It hasn't, in fact it is key. Just not time dilation from individual masses. What you picture will require special physics as a function of distance, to red shift more distant stars more than gravitation red shift shifts the same size and type of star locally. So, why should most objects exhibit a red-shift, rather than a neutral average shift? Because there is increased space(time) between you and the source between instants. Imagine space(time) as sal****er taffy stretched between your two hands, with your hands as two distant stars. As time goes on (weather permitting) the taffy stretches, and the distance between the two "stars" (measured along the taffy) increases and signals between them take longer (red shift). From this poor analogy, better ones are the balloon analogy and the raisin bread analogy. My best answer is that we, on earth, are at the edge of our galaxy (the milky way), Not quite... we are about halfway out. and hence quite far from the concentration of mass near the centre of our galaxy. Doesn't matter. The spectra locally (inclusive of even the Andromeda galaxy) are unsurprising. And we have all sorts of candidates visible locally. .... Just some ideas. Flame away ![]() If you are interested in more than your own ideas, you can start he http://www.astro.ucla.edu/~wright/cosmolog.htm http://www.astro.ucla.edu/~wright/cosmo_01.htm .... and if you have questions, you can either ask here or on sci.astro. David A. Smith |
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#17
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On Jun 24, 7:53 pm, Igor wrote:
On Jun 24, 3:01 am, Roland PJ wrote: Red-shift of distant objects could be due to two different reasons: 1. Recession speed away from the earth, a special relativistic effect. 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. It seems that most discussion of red-shift centres around the assumption that SR recession is the cause (and hence that the universe is expanding). Why has GR time dilation been eliminated as a cause? So you're suggesting that objects in the universe become more massive the further away from us they are located? And, since our view of the universe isn't considered to be very special, how would you reconcile that with the notion that the mass distribution of the universe must be observer independent? No, I'm suggesting that we might have _both_ their distance and recession speed wrong. At the moment we interpret faint objects as being distant, and red- shifted objects as being receding. And we find there's a correlation between distance and recession speed. However, a faint and red-shifted object could simply be a nearby, stationary object under the influence of nearby mass (perhaps invisible to us), as a result of GR time dilation. Roland |
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#18
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On Jun 24, 2:02 pm, Roland PJ wrote:
On Jun 24, 7:53 pm, Igor wrote: On Jun 24, 3:01 am, Roland PJ wrote: Red-shift of distant objects could be due to two different reasons: 1. Recession speed away from the earth, a special relativistic effect. 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. It seems that most discussion of red-shift centres around the assumption that SR recession is the cause (and hence that the universe is expanding). Why has GR time dilation been eliminated as a cause? So you're suggesting that objects in the universe become more massive the further away from us they are located? And, since our view of the universe isn't considered to be very special, how would you reconcile that with the notion that the mass distribution of the universe must be observer independent? No, I'm suggesting that we might have _both_ their distance and recession speed wrong. At the moment we interpret faint objects as being distant, and red- shifted objects as being receding. And we find there's a correlation between distance and recession speed. However, a faint and red-shifted object could simply be a nearby, stationary object under the influence of nearby mass (perhaps invisible to us), as a result of GR time dilation. Roland Maybe so, but the GR time dilation effect cannot be the dominate one for the reasons I previously stated. |
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#19
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On Jun 24, 8:02 pm, "N:dlzc D:aol T:com \(dlzc\)"
wrote: Dear Roland PJ: "Roland PJ" wrote in message oups.com... Red-shift of distant objects could be due to two ... or more ... different reasons: 1. Recession speed away from the earth, a special relativistic effect. ... also just classical Doppler. Except it needs finite light speed doesn't it, which was one of the foundations of SR? I'd better check ![]() 2. Time dilation due to proximity to a concentration of mass, a general relativistic effect. No. We can measure gravitational time dialtion in the spectrum of the sources. Distant sources are more redshifted... regardless of their mass, only their distance. Um, how can spectral analysis discriminate between time-dilation and recession (or expansion, if you like)? The spectra are shifted in both case, not so? Can you explain some more? What you picture will require special physics as a function of distance, to red shift more distant stars more than gravitation red shift shifts the same size and type of star locally. OK, I have no idea what you mean by this. So, why should most objects exhibit a red-shift, rather than a neutral average shift? Because there is increased space(time) between you and the source between instants. Imagine space(time) as sal****er taffy stretched between your two hands, with your hands as two distant stars. As time goes on (weather permitting) the taffy stretches, and the distance between the two "stars" (measured along the taffy) increases and signals between them take longer (red shift). From this poor analogy, better ones are the balloon analogy and the raisin bread analogy. Note that I was trying to answer this question according to my theory, not pose it . Yes, I can see that expansion theories explain theHubble red-shift phenomenon. I was simply trying to propose a simpler solution, namely plain old GR in a non-expanding universe. Occam's razor and all. My best answer is that we, on earth, are at the edge of our galaxy (the milky way), Not quite... we are about halfway out. 2/3 if you want to nit-pick ![]() and hence quite far from the concentration of mass near the centre of our galaxy. Doesn't matter. The spectra locally (inclusive of even the Andromeda galaxy) are unsurprising. And we have all sorts of candidates visible locally. Yes it does matter. GR time dilation is directly related to your matter/energy environment. The fact that we are at the edge of our galaxy means that matter near the denser core is red-shifted relative to us. As Eric has pointed out, this difference might be too small to matter, but you can't just wave it away with a magic wand without doing the sums (which I intend to do... see questions below). Or perhaps we are missing each other here - I'm not sure how your 'spectra' comment relates. Or are you saying that the spectra from stars all over the milky way display no shift at all? In which case time dilation clearly can't be a factor within our own galaxy. If you are interested in more than your own ideas, you can start hehttp://www.astro.ucla.edu/~wright/co...t/cosmo_01.htm ... and if you have questions, you can either ask here or on sci.astro. Thanks for the links. Will follow them up. Now, what I really need to see whether my idea has any legs is an accurate map of the Milky Way. Specifically, the density of matter along the radial arms, and the shape of, and density of matter, within the 'core'. What's crucial is the density gradient of stars within the core. I can't find this anywhere at the moment. It seems pretty obvious that the core is not entirely homogeneous, but rather gets increasingly densely populated with stars towards the middle. But what's the density curve here? Thanks again for the response Roland |
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#20
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On Jun 24, 8:16 pm, Igor wrote:
On Jun 24, 2:02 pm, Roland PJ wrote: However, a faint and red-shifted object could simply be a nearby, stationary object under the influence of nearby mass (perhaps invisible to us), as a result of GR time dilation. Roland Maybe so, but the GR time dilation effect cannot be the dominate one for the reasons I previously stated. I think I missed that. Would you mind repeating? Thanks Roland |
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