Astronomers have just found a new way to listen to the cosmic gravitational symphony – using quasars

Astrophysicist pioneer method to measure cosmic ripple through quasar motion
Scientists have developed a promising new method to detect gravitational waves in the universe—the ripples of space-time constantly wash over our planets, but are largely invisible by traditional observation methods. This innovative technology can have a deeper understanding of how supermass black holes interact and have the potential to change our understanding of fundamental physics.
Jeremy Darling, astrophysicist at the University of Colorado Boulder University, published a study in the journal Letters of the Astrophysics, examining gravitational waves from a unique perspective—by precisely tracking the obvious movement of distant objects, called carsars. His approach provides a complementary approach to recent breakthrough measurements and ultimately provides a more complete picture of cosmic gravitational phenomena.
“We can learn a lot from these precise measurements of gravitational waves,” explains Darling, a professor in the Department of Astrophysics and Planetary Sciences. “The different flavors of gravity can lead to many different kinds of gravity waves.”
Capture the hidden ripples of the universe
The Earth can be regarded as a float that surfaces in a stormy ocean in space-time. Throughout the history of the universe, countless supermass black holes have participated in gravitational dances, spinning each other until they collide into catastrophic events, creating ripples that spread throughout the universe.
Last year, scientists from Nanograv collaborated to make a breakthrough by measuring this gravitational wave background through pulsar observations. However, these measurements capture only how waves stretch and squeeze space-time in one dimension—similar to waves that flow directly to and away from the coastline.
Darling’s research extends this understanding by studying how gravitational waves move relative to other dimensions of the Earth – left and right motion movements, creating a more complete image of these cosmic ripples.
Major findings in gravity wave research
- This study analyzes more than one million quasar species observed by the European Space Agency Gaia satellite
- Researchers examined 2,104,609,881 quasars to detect related motion patterns
- The spatial correlation measured by this technique is reduced to ±0.005 micro-arcseconds of each year in square squares.
- This study established the upper limit of gravity wave density at 0.0096
- This represents the first time that the light wavelength exceeds the RF measurement value
“Gravity waves operate in three dimensions,” Darling noted. “They stretch and squeeze space and time along our sight, but they also cause objects to appear to move back and forth in the sky.”
Observation is unobservable
The research focuses on quasars – bright objects powered by super black holes in the center of distant galaxies. Although quasars are millions of light years, their light rays deflected subtly by transmitting gravitational waves, creating a distinct “swing” motion when viewed from the earth.
Detection of this movement requires extraordinary precision. The measured values required are about 10 times more accurate than watching human nails grow from Earth. Furthermore, researchers must consider the complex movement of the Earth itself through space to isolate gravitational wave signals.
“If you’ve lived for millions of years and can actually observe these incredible little movements, you’ll see these quasars swing back and forth,” Darling said.
Although the current data are not detailed enough to ultimately prove that gravitational waves are causing quasars to swing, the study establishes an important methodological basis and increasingly stringent constraints on the energy levels of gravity waves.
Future prospects of cosmic detection
Do we want to detect these elusive signals? The Gaia satellite team plans to release a 5.5-year quasar observation in 2026, providing astronomers with a large data set that may ultimately reveal clear evidence of the impact of gravity waves on the location of the quasar.
“If we could see millions of quasars, then maybe we could find these signals buried in that very large data set,” Darling said.
The meaning of this study goes beyond pure astronomy. Understanding gravitational waves can help scientists track the evolution of galaxies and test basic assumptions about gravity itself. It is an important step in developing a more complete toolkit to observe some of the most powerful and mysterious phenomena in our universe.
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