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Gravitational Waves Create A 'Cosmic Symphony' That Scientists Are Tuning Into
Space.com
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21/03/2025
Scientists are using pulsars to detect the gravitational wave 'hum' created from supermassive black hole mergers.
Credit: National Science Foundation (NSF)
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00:00
Supermassive Black Hole
00:29
Supermassive black holes lurk in the hearts of most galaxies, and galaxies grow by merging
00:34
with other galaxies. When that happens, their black holes also merge and grow, becoming
00:40
more and more massive over time. How exactly this happens is not fully understood, but
00:47
the universe is telling us its secrets in gravitational whispers. We just have to listen.
00:54
Just as sound waves are vibrations of air molecules, gravitational waves are vibrations
00:59
in the fabric of space-time. When two massive black holes spiral toward each other, they
01:05
produce gravitational waves that travel through the cosmos at the speed of light. If we imagine
01:10
the universe as a grand symphony, these merging supermassive black holes are the bass players.
01:17
As they orbit each other, these black holes play the deep bass notes that echo throughout
01:22
the cosmic concert hall. But that's not all there is to the symphony. In the background
01:28
is a faint but pervasive hum produced by the collective motion of massive objects throughout
01:33
the universe, from the earliest moments of the Big Bang until now. This gravitational
01:38
wave background is truly a harmony of space and time.
01:44
Nanograv is an NSF-funded collaboration of astronomers and astrophysicists. Our goal
01:49
is to solve some of the deepest mysteries of the universe by studying the gravitational
01:53
waves produced by these dancing monster black holes. These waves are light-years long and
02:00
can only be detected by the most extraordinary instruments.
02:05
To measure these giant but subtle ripples in space-time, Nanograv created a galaxy-sized
02:10
detector using some of the most incredible objects in the cosmos, rapidly rotating neutron
02:16
stars known as millisecond pulsars. Pulsars are the ultra-dense remnants left behind when
02:23
massive stars reach the end of their lives and explode as supernovae. These pulsars are
02:29
also cosmic beacons. They spin extraordinarily rapidly and with startling regularity, releasing
02:35
pulses of radio waves with each rotation. Astronomers detect those pulses using giant
02:41
radio telescopes.
02:44
By monitoring the radio pulses from these ultra-precise cosmic clocks, Nanograv can
02:48
detect the slightest deviations in the regularity of their timekeeping, and these deviations
02:54
trace ripples in space-time.
02:57
This galactic-scale detector is called a Pulsar Timing Array. Nanograv has now observed an
03:02
array of dozens of pulsars for more than 15 years, and the results are astounding.
03:09
We are finally hearing the faint background hum likely coming from in-spiraling pairs
03:13
of supermassive black holes. With time, astronomers expect to pick out the individual instruments
03:20
in this cosmic symphony, revealing unique insights into the evolution of galaxies and
03:25
the history of the cosmos.
03:39
Transcription by ESO. Translation by —
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