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Detecting gravity waves is exactly as hard as it sounds. The Laser Interferometer Gravitational-Wave Observatory consists of two separate detectors: one in Hanford, Washington, and the other in Livingston, Louisiana. To ensure that their detected signals are genuine and not a result of environmental disturbances, each detector is fitted with seismometers, accelerometers, microphones, magnetometers, radio receivers, weather sensors, AC-power line monitors, and a cosmic-ray detector.

LIGO's detectors use orthagonal laser beams to detect gravity waves. When a wave passes through the detecors, they will alter the length of the laser being shone inside of the detector arms, which is how they are detected. This graph shows the detected signal unnderneath a graphical representation of what is happening in space:

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The gravity waves themselves were registered to be in the 35-350 Hz band of frequencies, and the actual detection happened within half a second. This means that the black holes orbiting each other were orbiting each other upwards of 350 times per second, and the detected merger happened within half a second. Below is the actual data from humanities very first detection of gravitational waves:

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To learn more about LIGO and its 2015 discovery, check out the video below.

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Made by Jacob Torres
Last Revision: Apr. 13th, 2019
Class: Physics 212X (Spring 2019)

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