Where Did Those Gravitational Waves Come From? There's a Map
This map of the Southern Hemisphere skies shows the probably location of the gravitational wave source (a merging black hole) well beyond our Local Group of galaxies.
Credit: LIGO Science Collaboration

With today’s historic and incredibly exciting announcement of the first ever detection of gravitational waves came the news that these waves were generated by two merging black holes approximately 1.3 billion light-years away — an astrophysical event that is mind-blowing in its own right. So the next question that comes to mind is, unsurprisingly, in which direction did this black hole merger occur?

As it turns out, scientists of the Laser Interferometer Gravitational-Wave Observatory (LIGO) already have an answer, albeit a very general one.

ANALYSIS: We Just Heard the Spacetime 'Chirp' of Black Hole Rebirth

As previously reported, LIGO is composed of two stations — one in Washington and the other nearly 2,000 miles away in Louisiana. The reason for having 2 stations is logical: should a gravitational wave pass through our volume of space (yes, these spacetime ripples pass through the Earth and us unimpeded), it must be detected by both stations to be confirmed as being “real” and not a false positive caused by some kind of local disturbance near one of the stations. Secondly, having 2 stations allows LIGO scientists to triangulate the signal to derive a very general idea as to where these waves are coming from.

Thursday’s grand announcement pointed out that the Livingston station (Louisiana) “heard” the gravitational wave "chirp" 7 milliseconds before the Hanford station (Washington) on Sept. 14, 2015. As gravitational waves travel at the speed of light, this timing difference confirmed that the two detections were indeed the same event. Scientists were immediately able to deduce the direction the gravitational waves were traveling.

NEWS: Gravitational Waves Detected for First Time

Now, the LIGO collaboration has released a map of the Southern Hemisphere skies, giving us a glimpse at the promising future of gravitational wave astronomy. In the map, contours have been added that represent the different probabilities for where the signal originated. The outermost purple line represents a 90 percent certainty that the signal’s source (the colliding black holes) is contained within that area. The innermost white contour line highlights a possible source region to a 10 percent certainty.

The band of stars through the middle of the image is the edge-on disk of the Milky Way and the Large Magellanic Cloud and Small Magellanic Cloud (two small nearby galaxies) can also be seen in the bottom portion of the image. It is worth noting that, although there is some uncertainty in the black hole’s distance, its location is far beyond our own galaxy and Local Group of galaxies.

EXPLAINER: What You Need to Know About Gravitational Waves

As more gravitational wave detectors go online and their observations added to LIGO’s detections, better precision of the locations of gravitational wave sources will be pinpointed, making for highly detailed gravitational wave maps of the cosmos. So though it may not be precise, this is the first map of its kind where inside its contours two black holes merged 1.3 billion years ago.

Source: Caltech

This article was provided by Discovery News.