An artist’s conception visualizes the gravitational waves given off by a neutron star collision. (LIGO / MIT / Caltech Illustration)
Another big announcement about gravitational waves is coming up, and this time the hints point to observations in electromagnetic wavelengths as well — emissions of light that may have come from the collision of neutron stars.
That would be a biggie for astronomers: So far, the scientists behind the Laser Interferometer Gravitational-wave Observatory, or LIGO, have detected three confirmed collisions of black holes, but no smash-ups of dense neutron stars.
All will be revealed at 7 a.m. PT on Monday, when representatives from LIGO, Europe’s Virgo gravitational-wave observatory, and a sampling of researchers from 70 other observatories are to share new findings during a briefing at the National Press Club in Washington, D.C.
That was the place where the LIGO team reported its first-ever detection of gravitational waves last year.
The European Southern Observatory is planning a news conference at the same time at its headquarters in Germany.
The fact that so many observatories around the world are in on multiple briefings is a sign that a gravitational-wave detection has matched up with emissions in the electromagnetic spectrum — something that hasn’t been reported previously.
Could this be neutron stars? Advance speculation favors that scenario, because it’s thought that the clash of black holes doesn’t produce light. Last month, scientists said they weren’t able to match up the most recently reported LIGO detection of a black hole merger with any electromagnetic observations.
Unlike telescopes that monitor electromagnetic wavelengths — ranging from radio and infrared, to visible light, to X-rays and gamma rays — LIGO and Virgo look for ripples in the fabric of spacetime. Only the most violent cosmic events, such as supernova blasts and the mergers of black holes and neutron stars, are strong enough to trigger detectable ripples.
The current hubbub actually dates back to August, when the LIGO team put out the word that astronomers should turn their telescopes toward the galaxy NGC 4993 in the constellation Hydra.
Some astronomers, including the University of Washington’s Peter Yoachim and the University of Texas-Austin’s Craig Wheeler, issued tweets hinting at an “optical counterpart” to gravitational-wave observations — and alluding to the possibility that it was a neutron star collision.
New LIGO. Source with optical counterpart. Blow your sox off!
— J Craig Wheeler (@ast309) August 18, 2017
merging neutron-neutron star is the initial call.
— peterpeter🎃spiceeat (@PeterYoachim) August 18, 2017
At the time, the rumors were picked up by publications including the journal Nature, Science News and astronomer Ethan Siegel’s “Starts With a Bang” blog on Forbes.com. Siegel also noted that the Hubble Space Telescope had spotted a candidate for a binary neutron star merger in NGC 4993 on Aug. 22.
In the days before September’s LIGO briefing about a black hole detection, some wondered whether that announcement was going to focus on the neutron star smash-up. Now there’s an even bigger production coming up, and it’s natural to think about neutron stars once again.
If Monday’s revelations relate to optical observations plus gravitational-wave observations, that would mark a big advance for what scientists call “multi-messenger astronomy” — the ability to combine different ways of detecting extreme phenomena to get a more complete picture of the workings of the cosmos.
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