NASA's Laser Interferometer Gravitational-Wave Observatory (LIGO) is celebrating its 10th anniversary since the groundbreaking moment when it directly detected gravitational waves as predicted by Albert Einstein a century ago. These invisible ripples in space are created by massive objects accelerating in space, such as during black hole mergers or supernovae explosions.
The detection process works like this: two long tunnels, each approximately 2.5 miles long, are arranged in an 'L' shape. At the end of each tunnel, a mirror is mounted that reflects laser beams sent from the observatory room. The returning beams are then recombined and analyzed for any distortions caused by gravitational waves passing through space-time.
When the beams return with slightly different lengths due to the wave's effect, a flicker of light reveals the presence of the wave. This detection method relies on extremely sensitive instruments and highly polished mirrors that can detect even tiny changes in distance between the laser beams.
The discovery has led to 300 confirmed black hole mergers detected in the past decade, with more expected as new data arrives from additional gravitational-wave observatories like VIRGO and KAGRA. The public can also get involved by contributing to research projects like Black Hole Hunters and Gravity Spy, which rely on analyzing stellar brightness changes or identifying glitches that may mimic gravitational waves.
For a hands-on experience, NASA's Dropping In With Gravitational Waves activity allows users to create their own simulation of gravitational waves using gelatin, magnetic marbles, and a small mirror. This experiment demonstrates how these invisible ripples in space can have a profound impact on our understanding of the universe.
				
			The detection process works like this: two long tunnels, each approximately 2.5 miles long, are arranged in an 'L' shape. At the end of each tunnel, a mirror is mounted that reflects laser beams sent from the observatory room. The returning beams are then recombined and analyzed for any distortions caused by gravitational waves passing through space-time.
When the beams return with slightly different lengths due to the wave's effect, a flicker of light reveals the presence of the wave. This detection method relies on extremely sensitive instruments and highly polished mirrors that can detect even tiny changes in distance between the laser beams.
The discovery has led to 300 confirmed black hole mergers detected in the past decade, with more expected as new data arrives from additional gravitational-wave observatories like VIRGO and KAGRA. The public can also get involved by contributing to research projects like Black Hole Hunters and Gravity Spy, which rely on analyzing stellar brightness changes or identifying glitches that may mimic gravitational waves.
For a hands-on experience, NASA's Dropping In With Gravitational Waves activity allows users to create their own simulation of gravitational waves using gelatin, magnetic marbles, and a small mirror. This experiment demonstrates how these invisible ripples in space can have a profound impact on our understanding of the universe.