GRAVITATIONAL WAVES - SCI & TECH

News: Science for All | Why does observing gravitational waves matter? 

 

What's in the news?

       Last week, scientists revealed evidence that the universe is constantly flooded with low-frequency gravitational waves, unlocking new avenues to expand our knowledge of the universe.

 

Key takeaways:

       Albert Einstein’s theory of relativity also predicted the existence of gravitational waves more than a century ago, but the phenomenon was only directly observed in 2016.

 

Gravitational waves:

       Gravitational waves are defined as “ripples” in space-time.

       The strongest gravitational waves are produced by cataclysmic events such as colliding black holes, supernovae (massive stars exploding at the end of their lifetimes), and colliding neutron stars.

 

Detection:

       Gravitational waves are washing over Earth all the time, but instruments have not been sensitive enough to detect them until very recently.

       The gravitational waves were first seen last year by the ground-based Laser Interferometer Gravitational-Wave Observatory (LIGO).

 

Features:

       They are caused by the acceleration of massive objects.

       They are moving at the speed of light without being scattered significantly.

       They are extremely weak so are very difficult to detect.

 

Significance:

       These waves will be particularly useful for studying black holes (the existence of which was first implied by Einstein’s theory) and other dark objects, because they’ll give scientists a bright beacon to search for even when objects don’t emit actual light.

       With this, mapping the abundance of black holes and frequency of their mergers could get a lot easier.

       Since they pass through matter without interacting with it, gravitational waves would come to Earth carrying undistorted information about their origin.

       They could also improve methods for estimating the distances to other galaxies.