Binary Inspiral
Description
The <A Href="Https://En.Wikipedia.Org/Wiki/First_Observation_Of_Gravitational_Waves">Gravitational Waves</A> Recently Detected By <A Href="Http://Www.Ligo.Org/">Ligo,</A> The Laser Interferometer Gravitational-Wave Observatory, Were Produced By The <A Href="Http://Www.Ligo.Org/Science/Gw-Inspiral.Php">Merger Of Two Black Holes.</A> The Binary Black Holes Orbit Each Other, Spiraling Closer And Closer Together As They Lose Energy Due To The Emission Of Gravitational Waves, Until They Finally Merge. When Galaxies Merge, The <A Href="Https://En.Wikipedia.Org/Wiki/Supermassive_Black_Hole">Supermassive Black Holes</A> At Their Centers Are Also Expected To Merge And Produce Gravitational Waves. These <A Href="Http://Nanograv.Org/Science/Index.Html">May Be Detected</A> By Observations Of <A Href="Https://En.Wikipedia.Org/Wiki/Pulsar_Timing_Array">Pulsars.</A> This Is A Small Model Of The Inspiraling Binary Black Hole System Just Before Merging, With The Spiral Representing The Gravitational Waves. The Model Includes A Small Loop For Attaching To A Chain.
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