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Astronomers spot 3,000 light-year 'light echo' of dying supermassive black hole

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This radio band composite image of Arp 187, obtained by the VLA and ALMA telescopes (blue: VLA 4.86 GHz, green: VLA 8.44 GHz, red: ALMA 133 GHz), shows clear bimodal jet lobes. But the central nucleus (center of the image) is dark.
This radio band composite image of Arp 187, obtained by the VLA and ALMA telescopes (blue: VLA 4.86 GHz, green: VLA 8.44 GHz, red: ALMA 133 GHz), shows clear bimodal jet lobes. But the central nucleus (center of the image) is dark. (Image credit: ALMA (ESO/NAOJ/NRAO), Ichikawa et al.)

At the dark hearts of galaxies like the Milky Way lie supermassive black holes, with millions or even billions of times the sun's mass. 

Some of those supermassive black holes are what scientists call active galactic nuclei (AGN), which spew out copious amounts of radiation like X-rays and radio waves. AGN are responsible for the twin jets of ionized gas you see shooting away in pictures of many galaxies.

Ichikawa and his colleagues observed Arp 187 with the radio telescopes at the Atacama Large Millimeter/submillimeter Array (ALMA) in northern Chile and the Very Large Array (VLA) in New Mexico. They spotted twin jet lobes, a telltale sign of an AGN. But they couldn't detect radio waves, which also should have been coming from an active nucleus.

The observational difference between a standard AGN (left) and a dying AGN (right) discovered by Ichikawa et al. In the dying AGN, the nucleus is very faint in all wavelength bands because AGN activity is already dead, while the extended ionized region is still visible for about 3,000 light-years since it takes about 3,000 years for the light to cross the extended region.

The observational difference between a standard AGN (left) and a dying AGN (right) discovered by Ichikawa et al. In the dying AGN, the nucleus is very faint in all wavelength bands because AGN activity is already dead, while the extended ionized region is still visible for about 3,000 light-years since it takes about 3,000 years for the light to cross the extended region. (Image credit: Ichikawa et al.)

So, the researchers took a second look at Arp 187's core with NASA's NuSTAR ("Nuclear Spectroscopic Telescope Array") X-ray satellite. AGN normally produce X-rays in abundance, but no such signal emerges in the NuSTAR data, the team reported in a study presented earlier this month at the 238th meeting of the American Astronomical Society, which was held virtually.

The researchers therefore think that, sometime in the past several thousand years (as observed from Earth), Arp 187's AGN has gone dark.

This observation is possible because an AGN's jets are colossal. Arp 187's stretch out for 3,000 light-years, meaning that you can see their matter stream away for millennia after the AGN core "dies." Astronomers call this mourning period a "light echo." It's like watching smoke from a newly extinguished fire.

The researchers have called their discovery "serendipitous." Arp 187 could be a stepping stone to learning more about what happens at the end of an AGN's life, study team members said.

"We will search for more dying AGN using a similar method as this study," Ichikawa said in a statement. "We will also obtain the high spatial resolution follow-up observations to investigate the gas inflows and outflows, which might clarify how the shutdown of AGN activity has occurred."

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Rahul Rao

Rao is a freelance science journalist based in New York and is a contributor to Live Science’s sister site Space.com, as well as Popular Science, EEE Spectrum and Gizmodo. Rao has a bachelor’s degree in Physics and English from Vanderbilt University, and a master’s degree in Science, Health and Environmental Reporting from New York University.