It
 was one of the biggest moments in recent memory when an international 
team of physicists announced that they’d made the first direct 
observations of gravitational waves since Einstein first proposed them a
 century ago. 
Now, just four months later, an 
Australian team has announced the second such achievement - they’ve 
directly detected gravitational waves caused by the collision of two 
black holes that are up to 14 times the size of our Sun.
"This 
has cemented the age of gravitational wave astronomy," said one of the 
team, Susan Scott, an astrophysicist from the Australian National 
University (ANU) in Canberra. "This shows data is going to flow, that 
will enable us to map a lot more of the Universe than we’ve seen 
before."
Scott and her team have been analysing data collected by
 the two Laser Interferometer Gravitational-Wave Observatory (LIGO) 
detectors in the US - the same detectors that picked up that historic 
gravitational wave signal on 14 September 2015, before it was analysed 
and announced in February. 
On 26 December 2015, Australian 
researchers caught a glimpse of two black holes orbiting each other 27 
times in their last second before colliding. The blast signal that 
resulted was 10 times longer than that of the first gravitational wave, 
and now the team has finally had a chance to analyse it.
They’ve 
figured out that this collision actually happened 1.4 billion years ago,
 in a galaxy so distant, the resulting shockwaves have only just reached
 us. 
Predicted by Einstein back in 1916, gravitational waves are
 ripples in the curvature of spacetime that emanate from the most 
explosive and violent events in the Universe, such as a star exploding 
or a black hole merger. 
These ripples spread out through space 
like the ripples in a pond after a stone’s been tossed in, and - in the 
two cases we’ve been able to detect them - by the time those ripples get
 to us on Earth, they’re tiny. We’re talking around a billionth of the 
diameter of an atom.
Einstein himself predicted that humans would
 never be able to detect them because of how minuscule their signal 
would be. Until these LIGO observations, scientists have been making 
sense of the Universe based on electromagnetic observations that our 
instruments can detect, such as visible light emissions, radio waves, 
and X-rays.
Being able to reliably detect gravitational waves too
 means we have an entirely new way to 'see' and measure the objects and 
events in space around us. 
"I'd always imagined there would be 
electromagnetic counterparts in our first discoveries, but instead we 
found these invisible collisions of black holes purely through the 
gravitational waves they emitted, with no counterparts at all," says one
 of the team, Rob Ward. "Gravitational wave astronomy is going to 
revolutionise our understanding of the Universe."

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