<p><span class="math-container">$$\lambda_\mathrm{peak} \approx \frac{2.898 \times 10^6\ \mathrm{nm \cdot K}}{T}$$</span></p>
<p>With <span class="math-container">$T = 5000\ \mathrm{K}$</span>, that <span class="math-container">$\lambda_\mathrm{peak}$</span> is about <strong>580 nm</strong>, which is <strong>visible</strong> light.</p>
<p>Because everything was a hot plasma with unbound electrons there are no elemental spectral lines, which are generated by orbital jumps of electrons.</p>
<p>The stars would not have spectral lines either if they did not shine through a colder region of gases around them. The spectral lines from stars are less ionized  elements surrounding the star further away than the central plasma, that emit photons at specific wavelengths according to the electron orbits.</p>
<p>Hot plasma itself has atoms where the electrons are dissociated and have variable distances from the nuclei so plasma emits a broad spectrum a plasma tube...
That's actually how Bunsen and his colleague discovered what the sun was made of... by analyzing plasma tubes through prisms and lining up a prism on a telescope at the sun, then burning elements in colder flames in front of the plasma to see how the spectral signature of combusting elements adds to the spectrum of a plasma tube.</p>
<p>Check this thread for the maths: <a href="https://physics.stackexchange.com/questions/477758/what-wavelength-was-the-cmb-originally">https://physics.stackexchange.com/questions/477758/what-wavelength-was-the-cmb-originally</a></p>

CC BY-SA 4.0
2023-05-09T04:56:16.413Z
2023-05-10T02:26:05.140Z
2023-05-10T02:26:05.140Z
bandybabboon
<p>The redshift of the Cosmic Microwave Background (CMB) is not measured in the same way as the redshift of a galaxy. It is inferred from the measured temperature now compared with the calculated temperature at recombination.</p>
<p>The brief explanation is that as the universe expands and cools, it becomes energetically favourable to form bound atoms (known as recombination). The reduction in free electrons allows the universe to become transparent and photons escape as a blackbody radiation field and eventually form the CMB.</p>
<p>The temperature at recombination, <span class="math-container">$T$</span>, can be calculated using well understood physics (see <a href="https://en.m.wikipedia.org/wiki/Recombination_(cosmology)" rel="nofollow noreferrer">https://en.m.wikipedia.org/wiki/Recombination_(cosmology)</a>) and if the current temperature <span class="math-container">$T_0$</span> is known, then the redshift is simply given by <span class="math-container">$$ z = \frac{T}{T_0} -1\ .$$</span></p>
<p>Since the CMB is an almost (see below) perfect example of blackbody radiation, it is a smooth continuum with no lines, and the spectrum is given by the <a href="https://en.wikipedia.org/wiki/Planck%27s_law" rel="nofollow noreferrer">Planck function</a>.</p>
<p>There should be some <em>very weak</em> recombination lines, caused by capture of electrons into upper atomic energy levels, which then cascade to lower energy levels. But these have not yet been observed, since no instruments have had sufficient sensitivity to get the signal to noise required to find them. The reason they are expected to be so weak is that there are <span class="math-container">$\sim 10^9$</span> photons for every proton in the universe, and therefore the recombination lines are a tiny perturbation (1 part in a billion at most) on the blackbody background. See for example <a href="https://astronomy.stackexchange.com/a/48635/2531">https://astronomy.stackexchange.com/a/48635/2531</a></p>

CC BY-SA 3.0
2017-07-30T01:22:48.593Z
What about the spectral lines OP asked for?  Is it valid to say that there are none?  Maybe also because the CMB's origin lies within a time frame where there were no atoms (but only plasma) to produce such spectral absorption lines?
Alfe
CC BY-SA 4.0
2018-09-18T19:26:28.690Z
A nice summary is also given at https://thecuriousastronomer.wordpress.com/2015/07/30/what-is-the-redshift-of-the-cosmic-microwave-background-cmb/ (Also perhaps worth a look there: https://thecuriousastronomer.wordpress.com/2016/06/13/the-temperature-of-the-universe-at-recombination-decoupling/ )
Jacob C.
CC BY-SA 4.0
2016-04-22T19:34:37.613Z
2023-05-11T12:50:42.730Z
2023-05-11T12:50:42.730Z
ProfRob
<p>Are there any known <strong>spectral lines</strong> shifted by ~1100? If not, then how certain is mainstream that the CMB has a redshift of ~1100? All I see is a blackbody radiation curve void of spectral lines.</p>

CC BY-SA 3.0
2016-04-22T17:38:12.560Z
Possibly relevant: http://arxiv.org/abs/astro-ph/0607373
called2voyage
<universe><redshift><cosmic-microwave-background>
Evidence of CMB redshift
Paul
# Evidence of CMB redshift

(Asked by: username_0 on 2016-04-22)

Are there any known **spectral lines** shifted by ~1100? If not, then how certain is mainstream that the CMB has a redshift of ~1100? All I see is a blackbody radiation curve void of spectral lines.

**Tags:** universe, redshift, cosmic-microwave-background
> **Comments:**
> **username_1**: Possibly relevant: http://arxiv.org/abs/astro-ph/0607373  

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## 2 answers

### Answer by username_3 on 2016-04-22. Score: 7 | Accepted answer

The redshift of the Cosmic Microwave Background (CMB) is not measured in the same way as the redshift of a galaxy. It is inferred from the measured temperature now compared with the calculated temperature at recombination.

The brief explanation is that as the universe expands and cools, it becomes energetically favourable to form bound atoms (known as recombination). The reduction in free electrons allows the universe to become transparent and photons escape as a blackbody radiation field and eventually form the CMB.

The temperature at recombination, $T$, can be calculated using well understood physics (see <https://en.m.wikipedia.org/wiki/Recombination_(cosmology)>) and if the current temperature $T\_0$ is known, then the redshift is simply given by $$ z = \frac{T}{T\_0} -1\ .$$

Since the CMB is an almost (see below) perfect example of blackbody radiation, it is a smooth continuum with no lines, and the spectrum is given by the [Planck function](https://en.wikipedia.org/wiki/Planck%27s_law).

There should be some *very weak* recombination lines, caused by capture of electrons into upper atomic energy levels, which then cascade to lower energy levels. But these have not yet been observed, since no instruments have had sufficient sensitivity to get the signal to noise required to find them. The reason they are expected to be so weak is that there are $\sim 10^9$ photons for every proton in the universe, and therefore the recombination lines are a tiny perturbation (1 part in a billion at most) on the blackbody background. See for example <https://astronomy.stackexchange.com/a/48635/2531>

> **Comments:**
> **username_4**: What about the spectral lines OP asked for?  Is it valid to say that there are none?  Maybe also because the CMB's origin lies within a time frame where there were no atoms (but only plasma) to produce such spectral absorption lines?  
> **username_5**: A nice summary is also given at https://thecuriousastronomer.wordpress.com/2015/07/30/what-is-the-redshift-of-the-cosmic-microwave-background-cmb/ (Also perhaps worth a look there: https://thecuriousastronomer.wordpress.com/2016/06/13/the-temperature-of-the-universe-at-recombination-decoupling/ )  

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### Answer by username_2 on 2023-05-09. Score: -1

$$\lambda\_\mathrm{peak} \approx \frac{2.898 \times 10^6\ \mathrm{nm \cdot K}}{T}$$

With $T = 5000\ \mathrm{K}$, that $\lambda\_\mathrm{peak}$ is about **580 nm**, which is **visible** light.

Because everything was a hot plasma with unbound electrons there are no elemental spectral lines, which are generated by orbital jumps of electrons.

The stars would not have spectral lines either if they did not shine through a colder region of gases around them. The spectral lines from stars are less ionized elements surrounding the star further away than the central plasma, that emit photons at specific wavelengths according to the electron orbits.

Hot plasma itself has atoms where the electrons are dissociated and have variable distances from the nuclei so plasma emits a broad spectrum a plasma tube...
That's actually how Bunsen and his colleague discovered what the sun was made of... by analyzing plasma tubes through prisms and lining up a prism on a telescope at the sun, then burning elements in colder flames in front of the plasma to see how the spectral signature of combusting elements adds to the spectrum of a plasma tube.

Check this thread for the maths: <https://physics.stackexchange.com/questions/477758/what-wavelength-was-the-cmb-originally>


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