The detector consists of four huge mirrors (40 kilograms, 34 centimeters in diameter) that hang from overhead supports at the ends of two perpendicul… - Kip S. Thorne

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The detector consists of four huge mirrors (40 kilograms, 34 centimeters in diameter) that hang from overhead supports at the ends of two perpendicular arms. The waves’ tendex lines stretch one arm while squeezing the other, and then squeeze the first while stretching the second, over and over and over again. The oscillating separation between mirrors is monitored with laser beams, by a technique called interferometry. Hence LIGO’s name: Laser Interferometer Gravitational Wave Observatory.

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About Kip S. Thorne

Kip Stephen Thorne (born June 1, 1940) is an American physicist at the California Institute of Technology who specializes in the cosmological implications of the general theory of relativity.

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Birth Name: Kip Stephen Thorne
Alternative Names: Kip Thorne K.S. Thorne Dr. Kip Thorne
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By laws that we humans are capable of discovering, deciphering, mastering, and using to control our own fate. Even without bulk beings to help us, we humans are capable of dealing with most any catastrophe the universe may throw at us, and even those catastrophes we throw at ourselves — from climate change to biological and nuclear catastrophes.

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