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#61
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"OG" wrote in message ... you started with the following Two identical oscillators are positioned at different distances from a distant 'detection point', D. They are emitting continuous waves and are initially in phase. S1_________________________________D S2 Since the distance between the oscillators and point D is different,the number of wavelengths in each path is not the same. At a particular instant, they are set moving towards D at different speeds, such that they arrive at D together. At which I asked When you say '*they* arrive at D together' - what is the *they* that you are referring to? 'S1 & S2 themselves' or the 'waves from S1 and S2' |
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#62
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"Dr. Henri Wilson" HW@.... wrote in message ... On Sun, 27 Apr 2008 03:10:37 +0100, "OG" wrote: So complete the explanation of your own exact words "spectrum lines would be doppler shifted 180 out of phase wrt the star." Listen you bloody idiot, if you knew anything about physics or astronomy you would know that the light from the two members of a binary pair is doppler shifted roughly sinusoidally because of the sources' relative velocity wrt earth. The doppler shift of the spectrum of one is 180 out of phase wrt that of the other. This is very basic stuff...so stop making a fool of yourself.. Finally, you have explained yourself. Your inept initial phrase "spectrum lines would be doppler shifted ... out of phase wrt the star" and your aborted explanation of what you meant made me wonder whether you had some insight into physics; but in fact it was my error was in taking your words at face value. |
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#63
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"Dr. Henri Wilson" HW@.... wrote in message ... On Sun, 27 Apr 2008 03:13:09 +0100, "OG" wrote: "OG" wrote in message ... you started with the following Two identical oscillators are positioned at different distances from a distant 'detection point', D. They are emitting continuous waves and are initially in phase. S1_________________________________D S2 Since the distance between the oscillators and point D is different,the number of wavelengths in each path is not the same. At a particular instant, they are set moving towards D at different speeds, such that they arrive at D together. At which I asked When you say '*they* arrive at D together' - what is the *they* that you are referring to? 'S1 & S2 themselves' or the 'waves from S1 and S2' Run this program: http://www.users.bigpond.com/hewn/rayphases.exe It explains everything. It may do lots of other things as well - so I'd rather an explanation if you are able. |
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#64
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On Sun, 27 Apr 2008 21:01:48 +0100, "OG" wrote:
"Dr. Henri Wilson" HW@.... wrote in message .. . On Sun, 27 Apr 2008 03:13:09 +0100, "OG" wrote: "OG" wrote in message ... you started with the following Two identical oscillators are positioned at different distances from a distant 'detection point', D. They are emitting continuous waves and are initially in phase. S1_________________________________D S2 Since the distance between the oscillators and point D is different,the number of wavelengths in each path is not the same. At a particular instant, they are set moving towards D at different speeds, such that they arrive at D together. At which I asked When you say '*they* arrive at D together' - what is the *they* that you are referring to? 'S1 & S2 themselves' or the 'waves from S1 and S2' Run this program: http://www.users.bigpond.com/hewn/rayphases.exe It explains everything. It may do lots of other things as well - so I'd rather an explanation if you are able. How could it do any damage when I wrote the thing. If you want to see why a ring gyro works, run it. Henri Wilson. ASTC,BSc,DSc(T) www.users.bigpond.com/hewn/index.htm .....specialising in teaching physics to engineers and mathematicians.... |
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#65
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OG wrote:
..... It may do lots of other things as well - so I'd rather an explanation if you are able. Arguing with Ralph Rabbidge (aka Henry Wilson) is quite a pleasant game, and a useless one isn't it ? I'd undertand how successfull you feel to show how right you are in front of such elementary stupidity. You are completely right : Wilson is an idiot of the worse kind. BTW, you was supposed to enlight all of us by explaining us how using c=1 (or 2, or whatever) would break dimensional analysis as you are suposed to have studied it (what I doubt). Then you became suddenly silent. Did you lost your thongue ? |
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#66
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OG wrote:
..... It may do lots of other things as well - so I'd rather an explanation if you are able. Arguing with Ralph Rabbidge (aka Henry Wilson) is quite a pleasant game, and a useless one isn't it ? I'd undertand how successfull you feel to show how right you are in front of such elementary stupidity. You are completely right : Wilson is an idiot of the worse kind. BTW, you was supposed to enlight all of us by explaining us how using c=1 (or 2, or whatever) would break dimensional analysis as you are suposed to have studied it (what I doubt). Then you became suddenly silent. Did you loose your thongue ? |
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#67
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Dr. Henri Wilson wrote:
On Fri, 25 Apr 2008 12:04:23 +0200, "Paul B. Andersen" wrote: Dr. Henri Wilson wrote: On Thu, 24 Apr 2008 13:32:32 +0200, "Paul B. Andersen" wrote: like the Sun. Of course there would be differences telling you that the spectrum isn't from a star, but the main point is that it cannot be mistaken for any other type of spectrum than G2. Oh, rubbish. Do you really believe that our sun's spectrum could be determined solely by examining the spectrum of Jupiter? Is Jupiter one of the terrestrial planets? (We have to exclude Venus as well, because of it's atmosphere.) Look: The colour of Mars and Mercury is mainly grey, (even if Mars is slightly reddish). That means that the albedo is approximately independent of the wavelength for light in the visible range. So the light reflected off them will contain exactly the same set of absorption lines as the Sun, which is a G2 spectrum. No new lines will appear, and no lines will disappear. So even if the continuum may be altered, the light can still be identified as originally coming from a G2 star, and _never_ from any other spectral class. If you don't believe it, look at: http://www.marstoday.com/news/viewsr.html?pid=13877 download the full text. Look at the Sun's spectrum in fig.5 and compare that to the visible part of the spectrum of the reflected light in the lower diagram in fig.8. (The spectra are very different in IR, because of the albedo's strong dependence of wavelength in that range. That's why I explicitly said the _visible_ spectrum.) I did however say that there are differences which will reveal that the light is _not_ coming directly from a star, and the most important difference will be change in the continuum because the albedo is not strictly independent of the wavelength. Of course it is not. Our own planet is a good example of that. If we include the spectrum outside of the visible range, the difference is very obvious. The spectrum of the light reflected off the gas planets or Venus will be very different, because of the spectral lines from the atmosphere. The spectrum will be nothing like the spectrum from any star, and can never be confused with a stellar spectrum. The bottom line is that when the light from a star is reflected off a planet, the spectrum of the reflected light can never be confused with the spectrum of a star, and certainly not with the spectrum of a star of a different spectral class. You are rambling. Why don't you just admit you are wrong. A large planet or cool object with an atmosphere will reflect the light from a nearby star. The relected spectrum will likely contain the same lines but in different proportions. You pointed out, yourself, some time ago that a star's temperature was assessed from the ratios of various emission and absorption lines not from the spectrum's peak value. Quite. So your statement below _is_ ridiculous, isn't it? :-) Your statement was: "A small hot star reflecting off a very large orbiting WCH could easily result in two different spectra, B and K, shifted 180 out of phase." The idea is absolute ridiculous, and reveals a complete ignorance of what a stellar spectrum is and how it is identified. Much of physics today would have been classified as ridiculous even one hundred years ago. You should bring youself up to date. In the rest of this posting, you yet again demonstrate your utter ignorance and your inability and unwillingness to even consider remedy that ignorance. Inability to learn is the hallmark of a moron. ..takes on to know one... I have told you this numerous times, PLEASE LEARN IT THIS TIME: The spectral class of a star is determined by the relative positions and strengths of the absorption lines, not by where the black body spectrum peaks. As I already stated, both emission and absorption lines are reflected from the planet. Their relative proportions will likely be considerably affected by the planet's albedo and atmosphere. That's why a Doppler shift doesn't affect the determination of the spectral class. I didn't mention doppler shift. You are becoming quite confused. There is a strong (one to one) correlation between the spectral class and the temperature of a star, so when the spectral class is determined, so is the temperature. Of course. . You are now hopelessly confused. But staying ignorant about the issues you talk about every day for years is a speciality of yours. Isn't it? Quod erat demonstrandum. Yes. You have an inability to learn. Henri Wilson wrote: "A small hot star reflecting off a very large orbiting WCH could easily result in two different spectra, B and K, shifted 180 out of phase." That says it all. And he is calling himself a "Doctor"! :-) Maybe it's time for Ralph Rabbidge to change his name again? http://users.pandora.be/vdmoortel/di...hangeName.html "We can say what we like without fear of losing our reputation. We can put forward any hypothesis no matter how stupid it might appear." Quod erat demonstrandum. -- Paul http://home.c2i.net/pb_andersen/ |
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#68
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This message is brought to you by Androcles
http://www.androcles01.pwp.blueyonder.co.uk/ "Paul B. Andersen" wrote in message ... | Henri Wilson wrote: | "A small hot star reflecting off a very large orbiting WCH could | easily result in two different spectra, B and K, shifted 180 out | of phase." | | That says it all. Pick the spectral type out of this: http://www.adlerplanetarium.org/cybe...spectrum02.jpg That says it all. |
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#69
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On Mon, 28 Apr 2008 11:07:40 +0200, "Paul B. Andersen"
wrote: Dr. Henri Wilson wrote: On Fri, 25 Apr 2008 12:04:23 +0200, "Paul B. Andersen" wrote: You are rambling. Why don't you just admit you are wrong. A large planet or cool object with an atmosphere will reflect the light from a nearby star. The relected spectrum will likely contain the same lines but in different proportions. You pointed out, yourself, some time ago that a star's temperature was assessed from the ratios of various emission and absorption lines not from the spectrum's peak value. Quite. So your statement below _is_ ridiculous, isn't it? :-) Your statement was: "A small hot star reflecting off a very large orbiting WCH could easily result in two different spectra, B and K, shifted 180 out of phase." The idea is absolute ridiculous, and reveals a complete ignorance of what a stellar spectrum is and how it is identified. Much of physics today would have been classified as ridiculous even one hundred years ago. You should bring youself up to date. In the rest of this posting, you yet again demonstrate your utter ignorance and your inability and unwillingness to even consider remedy that ignorance. Inability to learn is the hallmark of a moron. ..takes on to know one... I have told you this numerous times, PLEASE LEARN IT THIS TIME: The spectral class of a star is determined by the relative positions and strengths of the absorption lines, not by where the black body spectrum peaks. As I already stated, both emission and absorption lines are reflected from the planet. Their relative proportions will likely be considerably affected by the planet's albedo and atmosphere. That's why a Doppler shift doesn't affect the determination of the spectral class. I didn't mention doppler shift. You are becoming quite confused. There is a strong (one to one) correlation between the spectral class and the temperature of a star, so when the spectral class is determined, so is the temperature. Of course. . You are now hopelessly confused. But staying ignorant about the issues you talk about every day for years is a speciality of yours. Isn't it? Quod erat demonstrandum. Yes. You have an inability to learn. Henri Wilson wrote: "A small hot star reflecting off a very large orbiting WCH could easily result in two different spectra, B and K, shifted 180 out of phase." Quite easily. That says it all. You are still rambling. Why don't you just admit you are wrong. Henri Wilson. ASTC,BSc,DSc(T) www.users.bigpond.com/hewn/index.htm .....specialising in teaching physics to engineers and mathematicians.... |
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#70
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"YBM" wrote in message ... OG wrote: .... It may do lots of other things as well - so I'd rather an explanation if you are able. Arguing with Ralph Rabbidge (aka Henry Wilson) is quite a pleasant game, and a useless one isn't it ? I'd undertand how successfull you feel to show how right you are in front of such elementary stupidity. You are completely right : Wilson is an idiot of the worse kind. BTW, you was supposed to enlight all of us by explaining us how using c=1 (or 2, or whatever) would break dimensional analysis as you are suposed to have studied it (what I doubt). Then you became suddenly silent. Did you loose your thongue ? No, I've been thinking about it. Explain again how c can be be made to be dimensionless - given that it represents both distance and time I'm listening. |
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