Photon coming from a far away star is redshifted?

In summary, space Tiger believes that since we only measure light over a certain range of wavelengths, we can't really say that the laws of physics are the same in all places and all times. He argues that since heavier elements (like iron) are only formed by supernovae explosions, we can say that there are galaxies far away that don't have any iron, which would be a sign that the laws of physics have changed over time.
  • #1
Ratzinger
291
0
How do we know that a photon coming from a far away star is redshifted?
Since we only can measure wavelength here on Earth how do we know that its wavelength was shorter when emited?

thanks
 
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  • #2
Ratzinger said:
How do we know that a photon coming from a far away star is redshifted?
Since we only can measure wavelength here on Earth how do we know that its wavelength was shorter when emited?

thanks

Exicted atoms emit specific, unique spectra. It is these fingerprint-like patterns which are shifted. Since these patterns are conserved, we can determine the redshift.
 
  • #3
There's a picture at wikipedia;

http://en.wikipedia.org/wiki/Redshift

That might help. You can see the pattern of lines in a nearby object (the sun) and compar them to the lines in a distant star. The pattern of lines is nearly identical, and if you take the near object and move all its spectral lines just a little bit toward the red, they match up perfectly with the spectral lines of the more distant light source. The very likely conclusion; the two are emitting the same spectrum of light, and light from the more distant objected is shifting towards the red.
 
  • #4
Basically, we don't.
Trouble is that these photons set off a very long time ago. Arp says that maybe some of these constants like the Plank constant are time dependent and had a different value a few million years ago.
After all, we have only been measuring them for 100 years so how can we extrapolate back and say that since they have been constant for the last 100 year or so (- within expermental error) they have been constant for all time?
E = hf,
if h changes the frequency changes and so wavelength was different when they set off. hence redshfted
 
  • #6
ratfink said:
Basically, we don't.
Trouble is that these photons set off a very long time ago. Arp says that maybe some of these constants like the Plank constant are time dependent and had a different value a few million years ago.
After all, we have only been measuring them for 100 years so how can we extrapolate back and say that since they have been constant for the last 100 year or so (- within expermental error) they have been constant for all time?
E = hf,
if h changes the frequency changes and so wavelength was different when they set off. hence redshfted
Most scientists assume the laws of physics are the same at all times and places in this universe. Of course, this assumption is unprovable. But, when you apply that assumption to observational evidence, you get answers that make sense. On the other hand, if you attempt to get cute and 'tweak' things, like h, you get bizarre results that throw everything out of synch - sort of like the string landscape [sorry, I coudn't resist].
 
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  • #7
ratfink said:
After all, we have only been measuring them for 100 years so how can we extrapolate back and say that since they have been constant for the last 100 year or so (- within expermental error) they have been constant for all time?
That is not true. Since a look into space is a look back in time and the universe looks the same everywhere, we can say with a high degree of certainty that the laws of physics are the same everywhere and have been for at least most of the way back to the Big Bang. If things like the Planck constant were even a little different a billion years ago, the universe of a billion years ago would look vastly different from what we see.
 
  • #8
russ_watters said:
That is not true. Since a look into space is a look back in time and the universe looks the same everywhere, we can say with a high degree of certainty that the laws of physics are the same everywhere and have been for at least most of the way back to the Big Bang. If things like the Planck constant were even a little different a billion years ago, the universe of a billion years ago would look vastly different from what we see.
Space Tiger will be proud of me here.
In the BB, as one looks further and further out one looks further and further back in time. Heavier elements are formed by supernovae explosions and so one would not expect to find iron in distant early, unformed galaxies. And we, followers of the BB, say that that is what you find. That is, you do see aging (or should that be un ageing?) as you look at galaxies further and further away.
Without it the BB would be incorrect.
Cheers,
A truly converted Ratfink.
 
  • #9
Iron enrichment is not really an issue in the early universe. Population III stars can easily explain that observation.
 
  • #10
Chronos said:
Iron enrichment is not really an issue in the early universe. Population III stars can easily explain that observation.
Actually it is an issue - the accretion disks of some high-z quasars show an iron abundance 3 x solar, e.g. APM 08279+5255at z = 3.91 whose estimated age is 2.1 Gyr when the universe was only 1.6 Gyrs old (according to LCDM model expansion).
The discovery of the quasar, the APM 08279+5255 at z = 3.91 whose age is 2-3 Gyr has once again led to ``age crisis''.
There are several more high-Fe high-z quasars known.

Although PopIII stars can explain other high-z metallicity, it is difficult to explain how so much iron formed so early as iron is the last element to be created in the nuclear fusion process.

This point is emphasised by Drs. Norbert Schartel, Fred Jansen and Prof. Guenther Hasinger in their ESA web-page article Is the universe older than expected?
Since iron is released by exploding stars, according to precise physical phenomena, and scientists think it builds up across the Universe gradually with time. The Solar System formed just 5 thousand million years ago, so it should contain more iron than the quasar, which formed over 13.5 thousand million years ago. The fact that the quasar contains three times more iron than the Sun is therefore a major puzzle
What might this be telling us?
One possible explanation is that something is wrong with the way astronomers measure the age of objects in the Universe. The almost-holy red shift-distance-age conversion would therefore be wrong. Fred Jansen, ESA's project scientist for XMM-Newton, explains that this would mean rewriting the textbooks. "If you study the evolution of the Universe, one of the basic rules is that we can tie redshift to age. One distinct possibility to explain these observations is that, at the redshift we are looking at, the Universe is older than we think."

You do not have to throw out the 'z' - 'observed age' relationship, that depends on the cosmological scale factor R(t), which occurs in the Robertson-Walker metric.

Perhaps R(t) simply needs adjusting? (again!)

Garth
 
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  • #11
ratfink said:
Space Tiger will be proud of me here.
In the BB, as one looks further and further out one looks further and further back in time. Heavier elements are formed by supernovae explosions and so one would not expect to find iron in distant early, unformed galaxies. And we, followers of the BB, say that that is what you find. That is, you do see aging (or should that be un ageing?) as you look at galaxies further and further away.
Without it the BB would be incorrect.
Cheers,
A truly converted Ratfink.
I recognize that we see differences in age as we look further away. I wasn't saying we don't.
 
  • #12
russ_watters said:
I recognize that we see differences in age as we look further away. I wasn't saying we don't.
So are you taking this back?
That is not true. Since a look into space is a look back in time and the universe looks the same everywhere, we can say with a high degree of certainty that the laws of physics are the same everywhere and have been for at least most of the way back to the Big Bang.
Cheers,
Ratfink
 
  • #13
Hubbleshift & Dopplershift

Talking about redshifted radiation in our universe it seems good to me to take into consideration the 2 sorts of shift mechanisms.
The first one is the Doppler-effect (speed difference dependent) en the second one is the Hubble-shift (distance difference dependent). Whenever the expansion stops, its related frequency shift (Hubble-shift) of radiation during its trip through the universe will be frozen while its related Doppler-effect disappears. Other Dopper-effects of relatively moving radiation-sources will continue.
I suppose I am right.
 

1. What is redshifting in terms of a photon coming from a far away star?

Redshifting refers to the phenomenon in which the wavelength of light from an object moving away from an observer appears longer, or "shifted" towards the red end of the light spectrum. This can occur when the object is moving away from the observer at high speeds, causing the light waves to stretch out.

2. How does redshifting affect the color of a photon from a distant star?

The longer wavelength of a redshifted photon means that it appears more red to the observer. This is because different colors of light have different wavelengths, and when the wavelength increases, the color shifts towards the red end of the spectrum.

3. What causes a photon coming from a far away star to become redshifted?

The most common cause of redshifting in photons from distant stars is the expansion of the universe. As the universe expands, objects that are far away from us are moving away at faster speeds, causing their light to be redshifted. Other factors, such as the gravitational pull of massive objects, can also cause redshifting.

4. Is redshifting the same as doppler shifting?

Yes, redshifting is a type of doppler shifting, which refers to the change in wavelength of a wave due to the motion of the source or observer. Redshifting specifically refers to the increase in wavelength, while blueshifting refers to the decrease in wavelength.

5. How can we use redshifted photons to study distant stars and galaxies?

By analyzing the amount of redshift in the light from distant stars and galaxies, scientists can determine their distance from Earth as well as their velocity. This information can then be used to study the expansion of the universe, the formation of galaxies, and other important aspects of cosmology.

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