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Originally posted by alfa1
Originally posted by UnixFE
Blinking as there is a short timeframe without light/photon reaching the detector.
Yes, as I understand it, if a star is faint enough, you could measure the average photon rate at less than one per second (as an example).
If it expands like a sphere like for example the radio wave is it possible to drain this energy so some extraterestial a few planets behind me won't see any light just like it's possible with radio waves?
Originally posted by TheMindWar
reply to post by UnixFE
Your looking at things in a different context, consider the uncertainty principle. The photon can both exist and not exist at the same time. Its up to the observer by just observing to determine which state the photon is in.
Originally posted by TheMindWar
reply to post by Blarneystoner
Indeed, mind you, I like my explanation better
Originally posted by Arbitrageur
I'm not sure how technical you want to get with the answer to your question.
Originally posted by UnixFE
I just refered to my eyes as it was easier to describe than a detector in a lab. So this would mean stars do indeed blink if you just look close enough? Blinking as there is a short timeframe without light/photon reaching the detector.
When the star is very dim, there's another problem besides the number of photons being emitted, which is atmospheric distortion. This might actually cause the star to start blinking out visually even if a sufficient number of photons are headed in your direction. You can see this effect on brighter stars too, we call it "twinkling" which is a cute name but it's a big problem for astronomers viewing through the atmosphere, though they have fancy technology to compensate for it partially, it's something the Hubble doesn't have to deal with.
If you set twinkling aside though and just focus on the number of photons, this physicist has written more detail about the subject than you could ask for:
Ten photons per hour
the number of photons from the galaxy seen with the unaided eye is more like two hundred per hour, and in the telescope it is of about 350 per second
Now let's take the naked eye rate of two hundred photons per hour coming from the galaxy.
I am not sure how many stars are in that galaxy but we think ours has 400 billion or so, so let's say that's a smaller galaxy with 100 billion stars.
take 200 photons per hour, multiply that by 24 to get per day and by 365 to get per year = 1,752,000 photons per year.
divide that by 100 billion stars, and you get the photon rate coming from each star, which is 0.00000876 photons per year per star, or in other words, the typical time period between photons hitting your eye from each one of those stars is about 114,000 years.
Edit to add: I think that calculation, in addition to answering your question, also solves Olber's paradox, don't you? That doesn't seem like any paradox to me.edit on 29-11-2011 by Arbitrageur because: clarification
So, after taking care of some other (more legitimate) approximations, if one computes things correctly, the number of photons from the galaxy seen with the unaided eye is more like two hundred per hour, and in the telescope it is of about 350 per second.
Originally posted by TheMindWar
reply to post by Blarneystoner
If you dont observe a particle then you will not see any results so you wont know if its in a wave or a particle state.
Photons observed through an interference experiment act as waves.
That was intentional, why is that a problem?
Originally posted by Blarneystoner
The only problem with your summation is that you only calculated using the amount of photons hitting the eye at 200 per hour. That doesn't mean that the total amount of photons coming from the galaxy is only 200 per hour, that's the amount that your eye can take in. Notice that the rate per hour changes for telescopes.
Originally posted by UnixFE
I have a question about light and/or maybe quantum physics in general. I am no newbie in quantum physics and read many books about it (some from Richard Feynman) but while falling asleep I thought about light and can't solve the problem.
As far as we know a star (and our sun of cause) has some fusion going on releasing photons we see as light. Thats not hard to understand but what I thought about is: This photon has to fly in my direction (if it is a particle) and hit a cell in my eye so I can see the light from this star. If you take into account the distance of a star ( several light years) is it really possible that this star genertes photons that reach every part of the virtual sphere around it in my distance to it so that every millisecond there is a photon that can hit my eye? I haven't calculated this but a sphere with a radius of several lightyears should have a huge surface. Than dividing this surface into small pieces (to the size of my eye or better ever the cells in my eye). Of cause there would be billions of photons generated but really enough for each part and every millisecond in each area of this surface?
So as stars don't blink (they do but I asume this is just a visual effect through our atmosphere as I have learned) is this a prove for the wave nature of light. So each photon that is generted in that fusion expands into space like an expanding ball until it gets into contact something like my eye to be perceived like a photon/light?
And if this is the case just when do this wave deceide to collapse? I bet that my eye is not the first thing in range so if each of these photon waves expands into space why don't they all collapse in the same place while 'hitting' the first object with the outer surface? And if this wave just expands into a single direction we have the same problem as with a particle.
Is there a possibility that at a given time there is no photon send into my exact direction and the star is not visible for a moment. What if the star is millions of light years away? Would it be possible to see that such a star is blinking as there aren't enough photons for each part of the universe at such a distance?
I hope you understand what I mean as english is not my native langueage and there are probably many mistakes in the text.
edit on 29-11-2011 by UnixFE because: (no reason given)edit on 29-11-2011 by UnixFE because: (no reason given)
Originally posted by Blarneystoner
common sense tells me that the amount of photons hitting my eye from a distant star is more like several hundred per second not 200 per hour. That's just silly.
Source.
The human eye is very sensitive but can we see a single photon? The answer is that the sensors in the retina can respond to a single photon. However, neural filters only allow a signal to pass to the brain to trigger a conscious response when at least about five to nine arrive within less than 100 ms.
Originally posted by CLPrime
Originally posted by Blarneystoner
common sense tells me that the amount of photons hitting my eye from a distant star is more like several hundred per second not 200 per hour. That's just silly.
Your common sense would seem to be wrong, in this instance. Why would it be more reasonable that photons from a single distant star be that much more than 200 per hour? Have you ever seen a star from a distant galaxy with your naked eye?
ETA: the threshold of human eye sensitivity, ignoring the affects of scattering and background light, is about 7 photons in 100 ms:
Source.
The human eye is very sensitive but can we see a single photon? The answer is that the sensors in the retina can respond to a single photon. However, neural filters only allow a signal to pass to the brain to trigger a conscious response when at least about five to nine arrive within less than 100 ms.
That's 70 photons per second, or 252000 per hour - quite a bit more than 200 per hour.edit on 29-11-2011 by CLPrime because: (no reason given)
So, after taking care of some other (more legitimate) approximations, if one computes things correctly, the number of photons from the galaxy seen with the unaided eye is more like two hundred per hour, and in the telescope it is of about 350 per second.
Originally posted by Blarneystoner
a single magnitude 6 star (still visible to unaided eye)
Where he asked for something like the opposite of Olber's paradox.
Originally posted by UnixFE
reply to post by tangonine
Thanks for the link to Olbs paradox. Can't remember that I read about this. It's not exactly what I mean but into the same direction. I would like to know kind of the opposite. Why is there light from distant stars at any given timeframe. Of cause a star produces billions photons a second but is thos really enough for any possible observer millions of lightyears away.