GW170817
GW170817: A landmark multi-messenger cosmic collision
In August 2017, scientists detected GW170817, a gravitational wave signal from the collision of two neutron stars in the galaxy NGC 4993, about 140 million light-years away. This was the first time a cosmic event was seen in both gravitational waves and light, marking a new era of multi-messenger astronomy.
What happened
- Gravity waves came from the stars spiraling toward each other and merging, producing a signal that lasted about 100 seconds.
- The gravitational waves were picked up by the LIGO and Virgo detectors, with the signal arriving at different detectors in a few milliseconds due to their locations on Earth.
- About 1.7 seconds after the merger, a short gamma-ray burst called GRB 170817A was detected by space missions Fermi and INTEGRAL, helping scientists locate the source.
Following the discovery
- Roughly 11 hours after the merger, an optical glow in NGC 4993 was identified and named AT 2017gfo (also known as SSS17a). This optical counterpart, a kilonova, brightened and then cooled, shifting from blue to red as it expanded.
- Over the next days and weeks, more than 70 observatories across the electromagnetic spectrum—from radio to X-rays—tracked the event. The data showed material being blown off the merger at high speeds and cooling over time.
- The observations provided strong evidence that neutron star mergers create heavy elements, including gold and platinum, through rapid neutron capture (the r-process).
Key scientific impacts
- It confirmed that neutron star mergers are a major source of heavy elements in the universe.
- The near-simultaneous arrival of gravitational waves and light allowed precise tests of fundamental physics: gravity travels at the speed of light to an extraordinary degree of accuracy, and the observations constrained several alternative theories of gravity.
- The event helped measure the expansion rate of the universe (the Hubble constant) more independently and with increasing precision as more such events are observed.
- Scientists learned about the possible remnants after a neutron star merger, including the idea that a short-lived hypermassive neutron star might form before collapsing into a black hole.
The big picture
GW170817 showed that gravitational waves and electromagnetic waves can tell a single, coherent story about a dramatic cosmic collision. The milestone demonstrated the power of coordinating observations across different kinds of detectors and opened new paths for understanding the cosmos, including how the heaviest elements are formed and how the universe expands.
This page was last edited on 2 February 2026, at 09:36 (CET).