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."
No comments:
Post a Comment