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Black Hole Recoil Measured: Scientists Detect Cosmic Kick

by Rachel Kim – Technology Editor

Scientists Measure “Kick” of Newly Formed Black Hole

An international team of researchers has, ⁢for the ‍first time, directly measured the powerful recoil – dubbed a “cosmic kick” – experienced by a black hole immediately after its formation through the ​merger of two smaller black holes. This breakthrough provides unprecedented insight into one of‌ the⁢ universe’s most energetic events.

The team reconstructed the three-dimensional motion of the collision, which occurred 2.4 ​billion years ago, by meticulously analyzing gravitational waves – ripples in spacetime. The event, designated GW190412, was initially detected in 2019‍ by the LIGO and⁢ Virgo gravitational wave⁣ observatories. It ⁢involved the collision of black holes with ⁤masses 8 and 30 times that of our Sun.

The resulting, larger black hole was propelled into space at a velocity of⁣ tens⁣ of kilometers per second ‌due ‍to this “kick.” Measuring this recoil has long been a goal for physicists, as ⁤it confirms ‍theoretical predictions about black hole mergers.

Professor Juan Calderon-Bustillo explained the precision of ‍the measurement by comparing it to listening to an orchestra. “Different⁣ listeners hear different combinations of instruments. We analyzed the mixture of signals within the ⁢gravitational waves to pinpoint the source and determine the direction of‍ the black hole’s movement.”

Researchers emphasize the meaning of reconstructing the ‌full 3D movement of an event billions of⁤ light-years away using only spacetime fluctuations.This demonstrates ⁣the immense potential of gravitational wave astronomy.

Published in Nature Astronomy, the findings pave ​the way for further study of black hole mergers. Scientists ⁢hope to utilize this method to detect not only gravitational waves but also electromagnetic signals,like light,emitted during these events. This combined approach could usher in a new era of revelation in our understanding of the universe.

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