This is a huge step forward.
Neutron stars are one of the things that can happen at the end of a life-cycle of a supermassive star. The core collapses, squeezing the protons and electrons into neutrons and neutrinos. The neutrinos escape, but the neutrons are incredibly densely packed into a core between just 10 and 20 kilometres (6-12 miles) in diameter.
If this core is less than about three stellar masses, the pressure of this density supports the neutron star. If the core is any larger, it collapses into a black hole.
Because black holes absorb light, they can’t be observed directly. We infer their existence based on the reaction of space around them.
Neutron stars, on the other hand, are highly energetic, emitting immense amounts of light. This means that if we were looking at the right place at the right time, we could get real optical evidence of a gravitational wave source.
We could actually see what it looks like when those shockwaves propagate through the universe.
The kicker is that they are much smaller than the black hole collisions previously detected by our Earth-based interferometer – around 10-20 percent of the mass. This means they will be much, much harder to detect.
In fact, we may have to wait until the Laser Interferometer Space Antenna, or LISA, comes online in 2034, a space-based interferometer that will be at least five times more accurate than LIGO, based on the performance of pathfinder technology.
In the meantime, Virgo and LIGO are planning to continue their collaboration, with the next observation run scheduled to commence in the third quarter of 2018. And we’re sure they will find more exciting stuff then.
Below is our live blog with updates from the press announcement of this discovery:
12:15pm EST: It’s 15 minutes to go until the announcement starts! Anyone else super-excited? We’re super-excited despite the fact it’s past 2am here in Sydney, Australia. While we’re waiting for the press conference to kick off, here’s some more background on why a gravitational wave detection from neutron stars would be such a big deal.
Since its first 2016 announcement, LIGO made two more detections from black hole collisions. Then earlier this year, LIGO and another gravitational wave detector, VIRGO, took observations together, allowing for more precise signal triangulation.
If they have now achieved a detection of gravitational waves from a neutron star merger, it means not only we may learn something new about this type of cosmic collision, but it will also be the very first time we have detected gravitational waves of this particular type – another breakthrough for the new era of gravitational wave astronomy.
12:30pm EST: The announcement is starting! We’re watching the webcast live from G7 Science at Reggia di Venaria Media Center in Turin, Italy.
12:32pm EST: Actually, we’re still waiting for the livestream to start. We hope they haven’t forgotten about us!
12:37pm EST: Still no livestream, but this press release just went live on the LIGO website.
“The LIGO Scientific Collaboration and the Virgo collaboration report the first joint detection of gravitational waves with both the LIGO and Virgo detectors. This is the fourth announced detection of a binary black hole system and the first significant gravitational-wave signal recorded by the Virgo detector, and highlights the scientific potential of a three-detector network of gravitational-wave detectors.”
Doesn’t look like we have neutron stars.
12:40pm EST: WE HAVE THE LIVESTREAM!
12:42pm EST: France Córdova, Director of the National Science Foundation, is taking the floor.
12:43pm EST: The event is named GW 170814, after the date it was detected. It’s the first detection made using three detectors – two of LIGO’s, and one Virgo detector.
12:45pm EST: Jo van den Brand, spokesperson of the Virgo collaboration is taking the floor.
12:46pm EST: The gravitational wave signal arrived first at the LIGO Livingston detector; then six milliseconds later it arrived at the Hanford detector; then another six milliseconds later it arrived at the Virgo detector. Using three detectors has allowed the research team to locate the source of the waves with greater accuracy.
12:50pm EST: We’re now hearing from Frédérique Marion, Senior Scientist, Virgo Collaboration. She specialises in data analysis.
Virgo is aligned slightly differently to the two LIGO detectors. This difference has allowed the team to access something called the polarisation of gravitational waves, which is the distortion of spacetime in the three spatial dimensions.
GW 170814’s polarisation was consistent with Einstein’s theory of general relativity, and this is the first time we’ve been able to make that confirmation.
12:55pm EST: David Shoemaker, Spokesperson, LIGO Scientific Collaboration is now explaining how using three detectors lets scientists triangulate the location of the source of the gravitational waves.
12:57pm EST: The next observing run will commence in about a year from now.
“The future is incredibly bright for Virgo, for LIGO, for the Virgo-LIGO network, for gravitational wave astronomy, and for the greater astronomical environment which we can now do in common with gravitational waves and electromagnetic radiation.”
1:00pm EST: We’re now hearing from Giovanni Losurdo, Advanced Virgo Project Leader, Virgo Collaboration.
“As with Galileo, humankind has a new instrument with which to look towards the skies. Every time we use a new instrument, there is a new prospect for knowledge, and we provide knowledge, knowledge that can serve as inspiration for the imagination and intuition of the young, and can bring about change in thousands of minds, and therefore science as a whole.”
1:06pm EST: This image shows how much better simply adding one more detector improves the location of the source of gravitational waves:
The broad streaks show the area to which previous collisions were pinpointed. The small green blob in the bottom left is where GW 170814 originated. Amazing!
1:08pm EST: While we wait, here’s a little bit more information on the actual collision:
“The detected gravitational waves – ripples in space and time – were emitted during the final moments of the merger of two black holes with masses about 31 and 25 times the mass of the sun and located about 1.8 billion light-years away.
“The newly produced spinning black hole has about 53 times the mass of our sun, which means that about 3 solar masses were converted into gravitational-wave energy during the coalescence.”
1:09pm EST: And the livestream has ended before we had a chance to listen to question time.
We have to admit, we’re a little disappointed that we didn’t actually get to see a collision between two neutron stars, but this news is still incredibly exciting.
With Virgo and LIGO working together, Shoemaker says, we may be able to make detections like this as often as once a week!