Not exact matches
With much longer arms than the detectors on Earth, it should be sensitive to
gravitational waves from many
more sources.
Pinpointing the
sources of
gravitational waves will allow astronomers to point other telescopes their way, boosting the chances of learning
more about them via x-rays, gamma - rays, radio
waves, neutrinos and
more.
Because all three
gravitational -
wave detectors saw the signal, physicists could triangulate and locate the
source to within a 30 - square - degree patch of sky — about 60 times the size of the moon and much
more precise than Fermi's localization.
Rochester Institute of Technology professors have developed a faster,
more accurate way to assess
gravitational wave signals and infer the astronomical
sources that made them.
LIGO's goal, of course, is to see
more sources of
gravitational waves.
A third LIGO detector will allow researchers to triangulate
gravitational wave sources and train other telescopes on the same part of the sky to learn
more.
In this case, they have been able to narrow the possible regions of sky that could host the
source of the
gravitational waves by 10 times
more than with LIGO alone.
Having
more gravitational -
wave observatories around the globe helps scientists pin down the locations and
sources of
gravitational waves coming from space.
The fifth
gravitational wave event (GW170817), detected in mid-August 2017, was probably even
more important than the first detection because it was the first one whose
source also produced electromagnetic radiation we could observe with ground and space - based telescopes.
LIGO and Virgo have detected
more gravitational waves, but this time from an entirely different
source.