<div dir="ltr"><font size="4">One thing I found mind boggling about the October 12 2015 <div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">event</div> is that in a fraction of a second a amount of matter equivalent to 3 <div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">suns</div> was converted entirely into energy, in this case into gravitational waves<div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">. By comparison the Hiroshima bomb converted less than the mass of a dime into energy. A</div>nd yet spacetime is so stiff <div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">and it's so hard to deform that if you were in orbit around the Black Hole collision site at the same distance the Earth is from the sun the gravitational </div><div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">waves would make your ears pop but that's about it. So how could LIGO detect those waves from a distance of a billion light years? One reason is that LIGO is so sensitive it can tell when the distance between 2 mirrors 4 kilometers apart changes by 1/10000 the width of a proton, the other reason is LIGO detects the displacement the gravitational waves produce not their energy as telescopes do with light, so the strength of the signal LIGO detects decreases linearly with distance not as distance squared as with electromagnetic detection. That means it can hear things far far away. </div></font><div><div><div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline"><font size="4"><br></font></div></div><div><font size="4"><div class="gmail_default" style="font-family:arial,helvetica,sans-serif;display:inline">John K Clark </div> </font><div><div class="gmail_extra"><div class="gmail_quote"><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"></blockquote><br>
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