A Tour of the Black Hole Jet in M87
(Credit: NASA/CXC/A. Hobart)
[Runtime: 03:45]

With closed-captions (at YouTube)

Using NASA's Chandra X-ray Observatory, astronomers have seen that the famous giant black hole in Messier 87, or M87, is propelling particles at speeds greater than 99% of the speed of light.

The Event Horizon Telescope Collaboration released the first image of a black hole with observations of Messier 87 last April, making it arguably the Universe's most famous black hole.

Meanwhile, astronomers have studied a jet of high energy particles — powered by the black hole — blasting out of the center of M87 in radio, optical, and X-ray light for many years.

Over its two decades of operations, Chandra has observed M87 many times. And now, researchers used Chandra's data to determine that sections of the jet in M87 are moving at nearly the speed of light.

While astronomers have observed features in the M87 jet blasting away from its black hole this quickly at radio and optical wavelengths for many years, this provides the strongest evidence yet that actual particles are travelling this fast.

When matter gets close enough to a black hole, it enters into a swirling pattern called an accretion disk. Some material from the inner part of the accretion disk falls onto the black hole and some of it is redirected away from the black hole in the form of narrow beams, or jets, of material along magnetic field lines. Because the material can fall onto the black hole erratically, the jets are made of clumps or knots that can sometimes be identified with Chandra and other telescopes.

A team of astronomers recently used Chandra observations from 2012 and 2017 to track the motion of two X-ray knots located within the jet about 900 and 2,500 light years away from the black hole. The X-ray data show motion with apparent speeds of 6.3 times the speed of light for the X-ray knot closer to the black hole and 2.4 times the speed of light for the other.

While this sounds like it breaks the laws of physics, it's actually an illusion that occurs when objects are traveling close to the speed of light along a direction that is close to our line of sight. The jet travels almost as quickly towards us as the light it generates, giving the illusion that the jet's motion is much more rapid than the speed of light. In the case of M87, the jet is pointing close to our direction, resulting in these exotic apparent speeds.

The Chandra data are an excellent complement to what the Event Horizon Telescope, or EHT, found. The jet Chandra sees is five hundred thousand times larger in size than the ring imaged by the EHT. Another difference is that the EHT observed M87 over six days in April 2017, giving a recent snapshot of the black hole. The Chandra observations investigate ejected material within the jet that was launched from the black hole hundreds and thousands of years earlier. Astronomers are looking forward to seeing what else these telescopes can learn about black holes in the years to come.

A Quick Look at the Black Hole Jet in M87
(Credit: NASA/CXC/A. Hobart)
[Runtime: 01:12]

Astronomers have shown that the black hole in Messier 87 is propelling particles faster than 99% of the speed of light using NASA's Chandra X-ray Observatory.

The black hole in Messier 87, or M87, became famous in April 2019 when the Event Horizon Telescope released the first direct image of a black hole in this galaxy.

Chandra has observed M87 for many years and can see the effects from its black hole on much bigger scales — both across space and over time — than the EHT.

When material swirling around it falls towards the black hole in M87, some of it is redirected outward into powerful narrow beams, or jets.

Using Chandra data, astronomers zoomed into small regions of the jet and compared the changes in X-ray light over five years.

This evidence showed that particles in the jet are being propelled by the black hole right up to the ultimate cosmic speed limit.

Close-Up Comparison of "Knots" in the M87 Jet
(Credit: NASA/CXC/A. Hobart)
[Runtime: 00:14]

A close-up comparison of Chandra observations from 2012 and 2017 tracking the motion of two X-ray knots located within the M87 jet.