<p>The waves pass by at the speed of light. So you you would'nt see ripples, they would pass too fast, and remember the waves would be passing through you too. The wavelength was (relativly) long about 3000km. The wave doesn't pass you, you are inside the wave.</p>
<p>The amplitude of the waves detected by LIGO was small, one part in <span class="math-container">$10^{21}$</span>, Now while the intensity of the waves follows an inverse square law, because intensity is proportional to amplitude squared, the amplitude is inversely proportional to distance from source.</p>
<p>We are familiar with strains that are one part in 1000, that is a variation of one millimetre for every metre. To get that we would have to be a lot closer to the source, <span class="math-container">$10^{18}$</span> times closer. Since the black holes were about 1 billion light years distant, to get a strain of 1 part in 1000, the black hole merger would have to be <strong>about 10000km away</strong></p>
<p>Now if you are 10000km from a merging pair of 30 solar mass black holes, the strain of gravitational radiation is the least of your problems. If it is any consolation, your problems won't lost long.</p>

CC BY-SA 4.0
2020-09-05T23:28:36.950Z
A typical LIGO event seems to last c 100ms, so the wave pulse is about 30 000 km "long". Will light coming from a direction not parallal to the GW transmission get gravitationally lensed by the wave at all (I'm not looking for detectable, just theoretical)? It doesn't seem unreasonable, and could result in very small distortions of the sky to the sides as the wave passes.
Steve Linton
CC BY-SA 4.0
2016-02-15T16:52:13.333Z
2020-09-04T18:28:56.197Z
2020-09-04T18:28:56.197Z
James K
<p>If I understand it well enough, gravitational waves cause ripples in the space-time fabric. To our eyes, that would look like those rippling-effects on amateur videos. </p>

<p>Where does a source have to be, in order for the effects of gravitational waves to be visible, here, on Earth. </p>

CC BY-SA 3.0
2016-02-15T16:22:24.353Z
You cannot "see" a gravitational wave. Light is an electromagnetic wave, which is completely different. The videos are, to say the least, misleading.
HDE 226868
<general-relativity><gravitational-waves>
How far should the source be, for the gravitation waves to be visible on Earth?
sudo --do-it
# How far should the source be, for the gravitation waves to be visible on Earth?

(Asked by: username_0 on 2016-02-15)

If I understand it well enough, gravitational waves cause ripples in the space-time fabric. To our eyes, that would look like those rippling-effects on amateur videos.

Where does a source have to be, in order for the effects of gravitational waves to be visible, here, on Earth.

**Tags:** general-relativity, gravitational-waves

> **Comments:**
> **username_1**: You cannot "see" a gravitational wave. Light is an electromagnetic wave, which is completely different. The videos are, to say the least, misleading.  

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## 1 answers

### Answer by username_2 on 2016-02-15. Score: 13 | Accepted answer

The waves pass by at the speed of light. So you you would'nt see ripples, they would pass too fast, and remember the waves would be passing through you too. The wavelength was (relativly) long about 3000km. The wave doesn't pass you, you are inside the wave.

The amplitude of the waves detected by LIGO was small, one part in $10^{21}$, Now while the intensity of the waves follows an inverse square law, because intensity is proportional to amplitude squared, the amplitude is inversely proportional to distance from source.

We are familiar with strains that are one part in 1000, that is a variation of one millimetre for every metre. To get that we would have to be a lot closer to the source, $10^{18}$ times closer. Since the black holes were about 1 billion light years distant, to get a strain of 1 part in 1000, the black hole merger would have to be **about 10000km away**

Now if you are 10000km from a merging pair of 30 solar mass black holes, the strain of gravitational radiation is the least of your problems. If it is any consolation, your problems won't lost long.

> **Comments:**
> **username_3**: A typical LIGO event seems to last c 100ms, so the wave pulse is about 30 000 km "long". Will light coming from a direction not parallal to the GW transmission get gravitationally lensed by the wave at all (I'm not looking for detectable, just theoretical)? It doesn't seem unreasonable, and could result in very small distortions of the sky to the sides as the wave passes.  

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