Milky Way’s Supermassive Black Hole Still Smoldering Long After Powerful “Death-Ray” Beam Outburst

“>Milky Way galaxy was once thought to have a sleeping monster at its core, a black holeA black hole is a place in space where the pull of gravity is so strong not even light can escape it. Astronomers classify black holes into three categories by size: miniature, stellar, and supermassive black holes. Miniature black holes could have a mass smaller than our Sun and supermassive black holes could have a mass equivalent to billions of our Sun.”>black hole weighing 4 million times our Sun’s mass. But there is increasing evidence the black hole occasionally awakens to devour a hapless star or gas cloud that falls into it. The black hole then burps out powerful “death-ray” beams of radiation and particles traveling at nearly the speed of light. The biggest outburst on record was 2 million years ago. This is evident in expanding plumes of plasmaPlasma is one of the four fundamental states of matter, along with solid, liquid, and gas. It is an ionized gas consisting of positive ions and free electrons. It was first described by chemist Irving Langmuir in the 1920s.”>plasma that form an hourglass shape, extending far above and below the plane of our galaxy. Bipolar shock waves from the black hole outburst heated the gas outside the galactic plane to glow in gamma-rays and X-rays.

Hubble has found circumstantial evidence that the black hole is still smoldering long after the earlier outburst. Hubble astronomers’ evidence is like doing an archeological dig to try and peer through the interstellar pollution of dense sheets of dust and gas between Earth and the galactic center, 27,000 light-years away. Hubble photographed a bright knot of gas that has been impacted by an invisible jet from the black hole, that is merely 15 light-years from it. The black hole must have shown brilliantly billions of years ago as a quasar (quasi-stellar object), when our young galaxy was feeding on lots of infalling gas. But after all this time the black hole still goes through fits and starts, and is not ready for napping as long as there is a snack around.

[embedded content]

Mini-Jet Found Near Milky Way’s Supermassive Black Hole

“>NASA’s Hubble Space TelescopeThe Hubble Space Telescope (often referred to as Hubble or HST) is one of NASA’s Great Observatories and was launched into low Earth orbit in 1990. It is one of the largest and most versatile space telescopes in use and features a 2.4-meter mirror and four main instruments that observe in the ultraviolet, visible, and near-infrared regions of the electromagnetic spectrum. It was named after astronomer Edwin Hubble.”>Hubble Space Telescope hasn’t photographed the phantom jet but has helped find circumstantial evidence that it is still pushing feebly into a huge hydrogen cloud and then splattering, like the narrow stream from a hose aimed into a pile of sand.

This is further evidence that the black hole, with a mass of 4.1 million Suns, is not a sleeping monster but periodically hiccups as stars and gas clouds fall into it. Black holes draw some material into a swirling, orbiting accretion disk where some of the infalling material is swept up into outflowing jets that are collimated by the black hole’s powerful magnetic fields. The narrow “searchlight beams” are accompanied by a flood of deadly ionizing radiation.

“The central black hole is dynamically variable and is currently powered down,” said Gerald Cecil of the University of North Carolina in Chapel Hill. Cecil pieced together, like a jigsaw puzzle, multiwavelength observations from a variety of telescopes that suggest the black hole burps out mini-jets every time it swallows something hefty, like a gas cloud. His multinational team’s research has just been published in the Astrophysical Journal.

In this annotated composite image, yellow represents Hubble data, blue is Chandra data, green is Alma data, and red is VLA data. The graphic of a translucent, vertical white fan is added to show the suggested axis of a mini-jet from the supermassive black hole at the galaxy’s heart. Credit: NASA, ESA, and Gerald Cecil (UNC-Chapel Hill); Image Processing: Joseph DePasquale (STScI)

In 2013 evidence for a stubby southern jet near the black hole came from X-rays detected by NASA’s Chandra X-ray Observatory and radio waves detected by the Jansky Very Large Array telescope in Socorro, New Mexico. This jet too appears to be plowing into gas near the black hole.

Cecil was curious if there was a northern counter-jet as well. He first looked at archival spectra of such molecules as methyl alcohol and carbon monosulfide from the ALMAThe Atacama Large Millimeter/submillimeter Array (ALMA) is the largest ground-based facility for observations in the millimeter/submillimeter regime in the world. ALMA comprises of 66 high-precision dish antennas of measuring either 12 meters across or 7 meters across and is an international partnership between Europe, the United States, Japan and the Republic of Chile. “>ALMA Observatory in Chile (Atacama Large Millimeter/submillimeter Array), which uses millimeter wavelengths to peer through the veils of dust between us and the galactic core. ALMA reveals an expanding, narrow linear feature in molecular gas that can be traced for 15 light-years back towards the black hole.

By connecting the dots, Cecil next found in Hubble infrared-wavelength images a glowing, inflating bubble of hot gas that aligns to the jet at a distance of at least 35 light-years from the black hole. His team suggests that the black hole jet has plowed into it, inflating the bubble. These two residual effects of the fading jet are the only visual evidence of it impacting molecular gas.

This schematic is based on multiwavelength observations of a suspected jet from the massive black hole at the center of our Milky Way galaxy. The wide view shows our galaxy edge-on, with two huge bubbles of plasma glowing in gamma-rays and X-rays. These are evidence for an explosive outburst from the black hole about 2 million years ago. Probing deep into the galaxy’s core (inset), astronomers using the Hubble Space Telescope have captured a glowing cloud of hydrogen near the black hole. The interpretation is that the cloud is being hit by a narrow, columnated jet of material that was blasted out of the black hole merely 2,000 years ago. The black hole is still active, but on a smaller scale of energy output than previously known outbursts. When the jet slams into the hydrogen knot the outflow scatters into octopus-like tendrils that continue along a trajectory out of our galaxy. Credit: NASA, ESA, Gerald Cecil (UNC-Chapel Hill), and Dani Player (STScI)

As it blows through the gas the jet hits material and bends along multiple streams. “The streams percolate out of the Milky Way’s dense gas disk,” said co-author Alex Wagner of Tsukuba University in Japan. “The jet diverges from a pencil beam into tendrils, like that of an octopus.” This outflow creates a series of expanding bubbles that extend out to at least 500 light-years. This larger “soap bubble” structure has been mapped at various wavelengths by other telescopes.

Wagner and Cecil next ran supercomputer models of jet outflows in a simulated Milky Way disk, which reproduced the observations. “Like in archeology, you dig and dig to find older and older artifacts until you come upon remnants of a grand civilization,” said Cecil. Wagner’s conclusion: “Our central black hole clearly surged in luminosity at least 1 millionfold in the last million years. That sufficed for a jet to punch into the Galactic halo.”

Previous observations by Hubble and other telescopes found evidence that the Milky Way’s black hole had an outburst about 2-4 million years ago. That was energetic enough to create an immense pair of bubbles towering above our galaxy that glow in gamma-rays. They were first discovered by NASA’s Fermi Gamma-ray Space Telescope in 2010 and are surrounded by X-ray bubbles that were discovered in 2003 by the ROSAT satellite and mapped fully in 2020 by the eROSITA satellite.

The nearby barred-spiral galaxy NGC 1068 serves as a proxy for helping astronomers understand the fireworks taking place at the center of our Milky Way galaxy, driven by eruptions from a supermassive black hole. Because we live inside the Milky Way, much of our view of the galaxy’s center is blocked by intervening clouds of gas and dust. But, looking 45 million light-years away at NGC 1068 gives astronomers a birds-eye view of similar black hole outbursts. The inset Hubble Space Telescope image resolves hydrogen clouds as small as 10 light-years across within 150 light-years of the core. The clouds are glowing because they are caught in a “searchlight” of radiation beamed out of the galaxy’s black hole, which is larger and more active than the black hole in the heart of our galaxy.
Credit: NASA, ESA, Alex Filippenko (UC Berkeley), William Sparks (STScI), Luis C. Ho (KIAA-PKU), Matthew A Malkan (UCLA), Alessandro Capetti (STScI), Alyssa Pagan (STScI)

Hubble ultraviolet-light spectra have been used to measure the expansion velocity and composition of the ballooning lobes. Hubble spectra later found that the burst was so powerful that it lit up a gaseous structure, called the Magellanic stream, at about 200,000 light-years from the galactic center. Gas is glowing from that event even today.

To get a better idea of what’s going on, Cecil looked at Hubble and radio images of another galaxy with a black hole outflow. Located 47 million light-years away, the active spiral galaxy NGC 1068 has a string of bubble features aligned along an outflow from the very active black hole at its center. Cecil found that the scales of the radio and X-ray structures emerging from both NGC 1068 and our Milky Way are very similar. “A bow shock bubble at the top of the NGC 1068 outflow coincides with the scale of the Fermi bubble start in the Milky Way. NGC 1068 may be showing us what the Milky Way was doing during its major power surge several million years ago.”

The residual jet feature is close enough to the Milky Way’s black hole that it would become much more prominent only a few decades after the black hole powers up again. Cecil notes that “the black hole need only increase its luminosity by a hundredfold over that time to refill the jet channel with emitting particles. It would be cool to see how far the jet gets in that outburst. To reach into the Fermi gamma-ray bubbles would require that the jet sustain for hundreds of thousands of years because those bubbles are each 50,000 light years across!”

The anticipated images of the black hole’s shadow made with the National Science Foundation’s Event Horizon Telescope may reveal where and how the jet is launched.

Reference: “Tracing the Milky Way’s Vestigial Nuclear Jet” by Gerald Cecil, Alexander Y. Wagner, Joss Bland-Hawthorn, Geoffrey V. Bicknell and Dipanjan Mukherjee, 6 December 2021, Astrophysical Journal.
DOI: 10.3847/1538-4357/ac224f

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.