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The Binary Pulsar PSR 1913+16, one of about 50 known systems of the type. It contains two neutron stars orbiting around one another. One of the neutron strs is a pulsar and emits pulses of radio waves which can be measured to high precision. These observations show that the orbital period of the pulsar is changing by 2.7 parts in a billion per year. This is the change predicted by the general theory of relativity due to the loss of energy by the radiation of gravitational waves from the neutron stars
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In the next few years, ambitious new experiments will attempt to detect these waves directly. They are like tidal forces in their effects. When a gravitational wave passes through the page that you are reading it will slightly stretch the book sideways and squeeze it longways without changing its volume. The effects is tiny but with elaborate apparatus, similar to the interferometer used by Michelson en.wikipedia.org/wiki/Michelson_interferomete r to test the existence of the ether, we may be able to detect gravitational waves from violent events far away in our own galaxy and beyond. The prime candidates for detection are waves from very dense stars or black holes that are in the final throes of circling each other in orbits that are getting closer and closer to each other. In the end they will spiral together and merge in a cataclysmic event that produces huge amounts of outgoing light and gravitational waves. In the far future the binary pulsar will collapse into this state and provide a spectacular explosion of gravitational waves. Pages 173-175
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