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Refining Our Understanding of Gravitational Waves

Artist’s impression of gravitational waves generated by binary neutron stars.
Artist’s impression of gravitational waves generated by binary neutron stars. Image: R. Hurt/Caltech-JPL

Gravitational waves—ripples in the fabric of spacetime caused by tremendous events like colliding black holes or supernovae—were finally confirmed by scientists in 2016, after being predicted by Albert Einstein a century ago. This monumental discovery, made by the Laser Interferometer Gravitational-wave Observatory (LIGO), might not have been possible had it not been for Arecibo, as NAIC explains:

Indeed, the first evidence for the existence of gravitational waves came from long-term Arecibo observations of a pulsar in a decaying orbit with another neutron star, where the rate of orbital shrinkage matched the rate expected from the loss of energy carried away by emitted gravitational waves.