字幕表 動画を再生する 英語字幕をプリント [MUSIC PLAYING] Exactly 100 years ago, in 1916, Albert Einstein predicted the existence of gravitational waves, ripples in the fabric of spacetime that are produced by cataclysmic astrophysical events, such as the collision of two black holes. As they travel across the universe, gravitational waves stretch and squeeze space and time. One and a half billion years ago, two black holes that were 30 to 40 times the size of the sun collided and they bent spacetime around themselves. This created waves that propagated, traveled through the universe at the speed of light. And on September 14, 2015, they've reached Earth and we were ready to catch them. We were able to do so thanks to a facility called LIGO, the Laser Interferometer Gravitational-Wave Observatory. In Louisiana and in Washington state there are two almost identical L-shaped detectors that use lasers to measure the change in distance between mirrors that are two and a half miles apart. We're talking about changes in distance that are one and 10,000th the size of a proton because that's how small the effects of gravitational wave is on Earth. When gravitational waves hits LIGO they stretched and squeezed its arms. And by doing so, they conveyed the message of something that happened 1.5 billion years ago. Within three minutes, we were alerted of this signal and it was perfect, just as theory predicted it would be. Within fractions of a second, the frequency and the amplitude of the vibration increased with the unmistakable chirp pattern that is expected for colliding black holes. This is a groundbreaking discovery that will open a new field of gravitational wave astronomy where gravitational waves will be a new probe to explore the mysteries of the universe. [MUSIC PLAYING]