<p>What would be heard is vibrations set up by the gravitational wave in the atmosphere, although presumably they would also directly stimulate the parts of the ear too.</p>
<p>The amplitude of gravitational waves fall off as <span class="math-container">$1/r$</span>. The proportional change in lengths near (e.g. about a Schwarzschild radius <span class="math-container">$R_S$</span> away) the merger is <span class="math-container">$\approx 1$</span>. So at 1 AU it would be <span class="math-container">$R_S$</span>/1 AU. For stellar mass black holes this makes the amplitude <span class="math-container">$\delta\approx 3\cdot 10^{-8}$</span>.</p>
<p>But if we think in terms of sound pressure, the pressure in dB is <span class="math-container">$20 \log_{10}(P/P_0)$</span> where <span class="math-container">$P_0$</span> is the reference power  20 μPa in air. How do we get a pressure from displacements? <a href="https://en.wikipedia.org/wiki/Sound_pressure" rel="nofollow noreferrer">This Wikipedia page</a> gives an expression in terms of the <a href="https://en.wikipedia.org/wiki/Acoustic_impedance" rel="nofollow noreferrer">acoustic impedance</a>: <span class="math-container">$P=\delta Z$</span>. Normally this is about 413.3 Pa s/m in 20 degree air, which would give us -4.2 dB for the stellar mass black holes. Which is below the threshold of hearing.</p>
<p>If we instead use <span class="math-container">$R_S=0.08$</span> AU for a Sgr A* mass hole pair, now we get 124 dB! That ought to be noticeable... beside the other effects of the merger.</p>
<p>Generally <a href="https://www.ligo.org/science/GW-Inspiral.php" rel="nofollow noreferrer">the frequency rises, going up in a chirp</a>, followed by a quick ringing. But the time from the sound becomes noticeable and the merger is likely very quick. Heavy holes merge fast, light ones merge slowly but would be too quiet. However, as Emil pointed out, <a href="https://astronomy.stackexchange.com/questions/25397/why-is-frequency-different-for-gravitational-waves-coming-from-smbhs-vs-small-co#:%7E:text=As%20a%20note%2C%20the%20frequency,10%20to%2010%E2%88%927%20Hertz.">the frequency is very low for supermassive black holes</a>, maximally about <span class="math-container">$10^{-2}$</span> Hz which is below the hearing limit. Stellar mass holes can reach hundreds of Hz, but as discusses above are too quiet at 1 AU.</p>
<p><a href="https://i.sstatic.net/119Qk.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/119Qk.png" alt="Induced sound from black hole mergers at 1 AU versus human hearing limit" /></a></p>
<p>However, for hole pairs with a combined mass between a few and 200 solar masses the sound intensity does get above the human hearing limit!</p>

CC BY-SA 4.0
2022-11-28T00:09:14.353Z
perhaps even louder (underwater) than whales!? [How much power and energy is (actually) in a 230 dB "click" from a whale?](https://physics.stackexchange.com/q/272680/83380)
uhoh
CC BY-SA 4.0
2022-11-28T11:02:28.147Z
One problem with the example of a Sag A* mass hole pair is that the merger frequency at the end of the chirp would probably be too low to be perceived as sound (in the order of mHz, so minutes per cycle or more).
Emil
CC BY-SA 4.0
2022-11-28T21:01:45.557Z
@Emil - Good point, added it.
Anders Sandberg
CC BY-SA 4.0
2022-11-29T03:42:14.983Z
So stellar mass is the right pitch but too quiet; Sag A* is the volume of a rock concert but too low in pitch. Is there a mass somewhere in between where it's both loud enough and high enough in frequency to be audible?
N. Virgo
CC BY-SA 4.0
2022-11-30T00:22:58.910Z
@N.Virgo - Thanks for making me check! I have added a plot versus a measurement of the human hearing limit. It does look like there is a mass interval where it can be heard!
Anders Sandberg
CC BY-SA 4.0
2022-11-28T00:04:23.750Z
2022-11-30T00:21:49.827Z
2022-11-30T00:21:49.827Z
Anders Sandberg
<p>If we were in an earthlike planet at 1AU from a black hole merger, would we be able to hear the spacetime strains as the black holes orbit around each other? How would it sound?</p>

CC BY-SA 4.0
2022-11-27T22:07:06.507Z
Cool question! A different but related one in Physics SE: [How would a passing gravitational wave look or feel?](https://physics.stackexchange.com/q/338912/83380)
uhoh
CC BY-SA 4.0
2022-11-28T02:43:03.477Z
Of course, there are some technical difficulties in having an Earth-like planet 1 AU from a pair of merging black holes. ;) It needs a heat source, otherwise its atmosphere will be frozen solid.
PM 2Ring
<gravitational-waves>
Sound of a black hole merger
SummaLummaDumma
# Sound of a black hole merger

(Asked by: username_0 on 2022-11-27)

If we were in an earthlike planet at 1AU from a black hole merger, would we be able to hear the spacetime strains as the black holes orbit around each other? How would it sound?

**Tags:** gravitational-waves

> **Comments:**
> **username_1**: Cool question! A different but related one in Physics SE: [How would a passing gravitational wave look or feel?](https://physics.stackexchange.com/q/338912/83380)  
> **username_2**: Of course, there are some technical difficulties in having an Earth-like planet 1 AU from a pair of merging black holes. ;) It needs a heat source, otherwise its atmosphere will be frozen solid.  

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## 1 answers

### Answer by username_3 on 2022-11-28. Score: 17

What would be heard is vibrations set up by the gravitational wave in the atmosphere, although presumably they would also directly stimulate the parts of the ear too.

The amplitude of gravitational waves fall off as $1/r$. The proportional change in lengths near (e.g. about a Schwarzschild radius $R\_S$ away) the merger is $\approx 1$. So at 1 AU it would be $R\_S$/1 AU. For stellar mass black holes this makes the amplitude $\delta\approx 3\cdot 10^{-8}$.

But if we think in terms of sound pressure, the pressure in dB is $20 \log\_{10}(P/P\_0)$ where $P\_0$ is the reference power 20 μPa in air. How do we get a pressure from displacements? [This Wikipedia page](https://en.wikipedia.org/wiki/Sound_pressure) gives an expression in terms of the [acoustic impedance](https://en.wikipedia.org/wiki/Acoustic_impedance): $P=\delta Z$. Normally this is about 413.3 Pa s/m in 20 degree air, which would give us -4.2 dB for the stellar mass black holes. Which is below the threshold of hearing.

If we instead use $R\_S=0.08$ AU for a Sgr A\* mass hole pair, now we get 124 dB! That ought to be noticeable... beside the other effects of the merger.

Generally [the frequency rises, going up in a chirp](https://www.ligo.org/science/GW-Inspiral.php), followed by a quick ringing. But the time from the sound becomes noticeable and the merger is likely very quick. Heavy holes merge fast, light ones merge slowly but would be too quiet. However, as username_4 pointed out, [the frequency is very low for supermassive black holes](https://astronomy.stackexchange.com/questions/25397/why-is-frequency-different-for-gravitational-waves-coming-from-smbhs-vs-small-co#:%7E:text=As%20a%20note%2C%20the%20frequency,10%20to%2010%E2%88%927%20Hertz.), maximally about $10^{-2}$ Hz which is below the hearing limit. Stellar mass holes can reach hundreds of Hz, but as discusses above are too quiet at 1 AU.

[![Induced sound from black hole mergers at 1 AU versus human hearing limit](https://i.sstatic.net/119Qk.png)](https://i.sstatic.net/119Qk.png)

However, for hole pairs with a combined mass between a few and 200 solar masses the sound intensity does get above the human hearing limit!

> **Comments:**
> **username_1**: perhaps even louder (underwater) than whales!? [How much power and energy is (actually) in a 230 dB "click" from a whale?](https://physics.stackexchange.com/q/272680/83380)  
> **username_4**: One problem with the example of a Sag A* mass hole pair is that the merger frequency at the end of the chirp would probably be too low to be perceived as sound (in the order of mHz, so minutes per cycle or more).  
> **username_3**: @username_4 - Good point, added it.  
> **username_5**: So stellar mass is the right pitch but too quiet; Sag A* is the volume of a rock concert but too low in pitch. Is there a mass somewhere in between where it's both loud enough and high enough in frequency to be audible?  
> **username_3**: @N.username_5 - Thanks for making me check! I have added a plot versus a measurement of the human hearing limit. It does look like there is a mass interval where it can be heard!  

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