Galaxy-size jet from monster black hole blasts mystery object in deep space (video)

Astronomers using NASA's Chandra X-ray space telescope have witnessed a massive black hole jet slam into an unknown object in space. Astronomers have seen black hole jets blasting cosmic objects before, but this one appears different from these events.

The discovery came in the form of a strange mark in the bright jet erupting from the supermassive black hole at the heart of the galaxy Centaurus A (Cen A), located about 12 million light-years from Earth. The new research also revealed that at several points along its galaxy-scale length, the jet of high-energy particles from this black hole is traveling at near-light speed.

Though the jet of Cen A's supermassive black hole has been well-studied in the past, the Chandra data revealed something new and unexpected about this outflow.

The source of X-rays in Cen A known as "C4" seen in detail by Chandra

The source of X-rays in Cen A known as "C4" seen in detail by Chandra (Image credit: NASA/CXC/SAO/D. Bogensberger et al; Image Processing: NASA/CXC/SAO/N. Wolk;)

The team found the emission that contects to a bright V-shaped source of X-rays in Cen A. This source has been labeled "C4," and it is located close to the origin point of the black hole jet.

According to NASA, the "arms" of this V-shaped emission are around 700 light-years long. For context, that's around 175 times the distance between the sun and the closest star to the solar system, Proxima Centauri.

A golden swirl with a black orb at its heart

Artist's illustration of a supermassive black hole emitting a jet of energetic particles. (Image credit: NASA/JPL-Caltech)

What we know and what we don't know about this black hole jet

Jets from supermassive black holes don't come from the black holes themselves but from around them. These cosmic titans suggest that because they are marked by a boundary called an "event horizon," at which not even light moves fast enough to escape. Nothing with mass can move as fast as light, which means nothing can escape a black hole.

Some black holes are surrounded by flattened clouds of gas and dust called "accretion disks" that gradually feed them. Not all this material is destined to fall into the maw of the central black hole, however, as black holes are "messy eaters."

This is because powerful magnetic fields around the black hole can channel matter to its poles. From there, these particles are accelerated to high speeds and high energies and are blasted out as astrophysical jets that can stretch out for millions of light-years.

Blue filaments from which a bright orange jet emerges

An artist's illustration of the longest black hole jet system ever observed. Nicknamed Porphyrion after a mythological Greek giant, these jets span roughly 7 megaparsecs, or 23 million light- years. That is equivalent to lining up 140 Milky Way galaxies back-to-back. (Image credit: E. Wernquist / D. Nelson (IllustrisTNG Collaboration) / M. Oei 2.)

While astronomers have a good idea about the physics that launch the jet from the supermassive black holes at the heart of Cen A, they don't know what object it is they blasted. That is because it is too far away for even the most powerful current telescopes to distinguish in detail.

This is not the first time that scientists have seen a black hole jet blasting an object in space. These other target objects have included clouds of gas and even unfortunate stars.

This collision stands distinct from those events because while they have produced elliptical "blobs" in X-ray images, this event created a v-shaped structure.

The team will now attempt to determine why this particular collision has produced a strange shape. This investigation will be conducted with Chandra, the only X-ray telescope currently sensitive enough to see this collision feature.

The team's research is published in The Astrophysical Journal.

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Robert Lea
Senior Writer

Robert Lea is a science journalist in the U.K. whose articles have been published in Physics World, New Scientist, Astronomy Magazine, All About Space, Newsweek and ZME Science. He also writes about science communication for Elsevier and the European Journal of Physics. Rob holds a bachelor of science degree in physics and astronomy from the U.K.’s Open University. Follow him on Twitter @sciencef1rst.

  • Torbjorn Larsson
    This collision stands distinct from those events because while they have produced elliptical "blobs" in X-ray images, this event created a v-shaped structure.

    The team will now attempt to determine why this particular collision has produced a strange shape.

    My bold:
    The incognito object being rammed may be a massive star, either by itself or with a companion star. The X-rays from C4 could be caused by the collision between the particles in the jet and the gas in a wind blowing away from the star. This collision can generate turbulence, causing a rise in the density of the gas in the jet. This, in turn, ignites the X-ray emission seen with Chandra.
    The shape of the “V,” however, is not completely understood. The stream of X-rays trailing behind the source in the bottom arm of the “V” is roughly parallel to the jet, matching the picture of turbulence causing enhanced X-ray emission behind an obstacle in the path of the jet. The other arm of the “V” is harder to explain because it has a large angle to the jet, and astronomers are unsure what could explain that.
    https://www.nasa.gov/image-article/black-hole-jet-stumbles-into-something-in-the-dark/
    Reply