3rd Gravitational Wave Detection Is About Much More Than Black Holes

D-brief
By Eric Betz
Jun 1, 2017 7:00 PMJan 24, 2020 2:43 AM
Ligo Installation - LIGO Lab
More than a year after detecting the first confirmed gravitational waves, researchers were busy at the Laser Interferometer Gravitational-wave Observatory (LIGO) in Livingston, La., upgrading the massive instrument. (Credit: LIGO Lab)

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Our sun was still dim. Waves crashed on martian beaches. Life was emerging on Earth. That’s when the ghosts of two dead stars — black holes dozens of times more massive than our sun — merged in a far-off corner of the universe. In their final moments, these binary black holes were circling each other hundreds of times per second, as each one spun at 10 times that rate.

The rumbles of distant thunder from that collision reached Earth on Jan. 4 of this year, passing through the detector at the Laser Interferometer Gravitational-Wave Observatory (LIGO) in Hanford, Washington. Then, traveling at the speed of light, this wrinkle in space-time passed through LIGO’s second detector in Livingston, Louisiana, just a fraction of a second later. The results were published Thursday in the journal Physical Review Letters.

Cosmic Forces

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