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China’s FAST telescope helps find key evidence for the existence of nanohertz gravitational waves with its high sensitivity. Photo: National Astronomical Observatories of China.
Opinion
Editorial
by SCMP Editorial
Editorial
by SCMP Editorial

FAST telescope turns out to be cosmic star

  • Once dismissed as a vanity project, China’s giant radio telescope has teamed up with others on Earth to detect evidence of low-frequency gravitational waves

Gravitational waves are making a splash in the news these days, and Chinese scientists are in the thick of it. By using China’s FAST radio telescope, the world’s largest, researchers have been able to detect evidence of low-frequency gravitational waves, a low-pitch hum likely to yield insights into mysterious cosmic activities billions of light years away, from ancient galaxies when the universe was still young. Located in Guizhou, it technically stands for the Five-hundred-metre Aperture Spherical Telescope.

Teams of astronomers from India, Europe, the United States, Australia and China were assigned different distant segments of the universe, and they have managed to track new evidence or provide new analyses of previous data to show the likely existence of low-frequency waves. These can offer tantalising clues into how early galaxies merged and formed ever larger systems of stars, dust and planets that eventually settled into the cosmic structures we observe in the universe today. The collaborative efforts have been especially impressive, given the rising geopolitical tensions between the nations involved. There is surely hope for humanity that while politicians bicker and threaten each other, scientists jointly peer into their telescopes and share data to uncover the secrets of the universe.

Chinese team finds key evidence for low-frequency gravitational waves

Each national team shared data and then published their own independently. The Chinese group spent more than three years tracking 57 neutron stars known as pulsars in the Milky Way to catch the gravitational waves, which are tiny ripples in space-time.

After the binary systems of pulsars or those of black holes collapsed into each other, they could form supermassive black holes – the engines at the heart of galaxies that feed on gas and regulate star formation. Studying the cosmic background of gravitational waves therefore offers insights into fundamental questions of cosmology guided by Albert Einstein’s theory of general relativity.

High-frequency waves have already been detected, but those of low frequency can offer data much further away and older in time. While the latest is not yet conclusive proof of low-frequency waves, the consensus is that researchers are getting close. And the FAST telescope, once dismissed as a vanity project, has shown its worth.

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