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We Just Got an Image of a Plasma Jet From Another Supermassive Black Hole, And Whoa

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Two years ago, the Event Horizon Telescope gave us the first breathtaking image of the supermassive black hole at the centre of the M87 galaxy.

Now, the same telescope has presented an unprecedentedly detailed view of a plasma jet being spat out by the supermassive black hole at the centre of the nearby Centaurus A galaxy.

Screen Shot 2021 07 19 at 3.59.00 pmThe newly imaged plasma jet. (Nature Astronomy)

This is a pretty huge announcement for a couple of reasons, so let’s break it down.

 

First, the image is not only beautiful to look at but mind-boggling to consider – at an average distance of 12 million light-years away, the weirdly shaped Centaurus A galaxy is the closest radio-loud source to Earth. It’s known for its black hole, which spits out powerful plasma jets that we can detect here on Earth.

In the new image, a jet is captured on less than a ‘light-day’ scale, showing us in never-before-seen detail what is happening in these plasma jets.

“Usually we see these jets … at larger scales, and now we’re really peering down into the center of the source,” explains first author Michael Janssen from the Max-Planck-Institut für Radioastronomie, Bonn in Germany, in a video Q&A released alongside the paper

“Centaurus A is the closest radio galaxy to Earth [and] was actually discovered as one of the first extragalactic radio sources. Because of that feedback we can resolve and see the outflow [of the jet] as it ploughs through the galaxy and what it does to the gas and how it may trigger star formation, which is a very broad research project.”

 

Second, the high-resolution observations of the jet match what we’d expect to see based on general relativity – meaning once again, the Event Horizon Telescope’s imaging shows Einstein was right.

The theory of general relativity was also confirmed by the observations made of M87* and released back in 2019, but until now it remained to be seen if the same held true for less massive black holes, sucking up less matter.

The black hole at the center of Centaurus A has a mass of around 55 million solar masses (55 million times the mass of our Sun) – around 100 times less massive than M87*.

But it’s also bigger than the EHT’s second primary target, Sagittarius A*, the black hole at the center of our own Milky Way galaxy – which is estimated to be only around 4.1 million times as massive as our Sun.

Sitting in between these masses, the black hole of Centaurus A offered a good mid-point to test Einstein’s theory.

In the latest image, the EHT is unable to image the shadow of the black hole itself – which is what it did in the iconic donut image of M87* from 2019 – but they could peer down as close as 0.6 light-days away from the black hole to see almost to the origin of the jet.

 

As you can see, the jet looks like a hollow 3D cone with bright edges. Overall, its properties and geometry are very similar to the jets in M87, and also similar to the jets that have been observed coming out of smaller, stellar mass black holes. 

“This finding supports the idea that massive black holes are scaled-up versions of their lighter counterparts,” explains a press release.

You can see the latest image in the middle, below (b), when compared to the until-now highest-resolution image of the Centaurus A black hole jet on the left (a), and a jet from M87* as a comparison on the right (c).

Image one (Nature Astronomy)

Above: (a) The previous highest resolution image of the Centaurus A jet taken with the TANAMI VLBI array. (b) the new EHT image which has a 16x zoom compared to the TANAMI image. (c) The M87 jet for comparison. 

The new image also shows us where the jet terminates, which is pretty important, as Janssen explains the outer edges of jets are where particle acceleration likely happens, and are a candidate source for ultra-high-energy cosmic rays. We see actually where the jet terminates. 

 

So what are these plasma jets? They’re released when matter from the galaxy falls toward its black hole – and as a result energy is blasted back out, often at speeds close to the speed of light.

We’ve detected these powerful radio sources from lots of galaxies, but still don’t quite understand how they work.

All of this detail is important, as it’s giving astronomers the data they need to be able to model general relativity in the lab.

“We’re able at this point now to generate effectively a black hole in a box to some extent,” explains researcher Sera Markoff from the University of Amsterdam, who is involved with the EHT project.

But of course there are limitations to what a model can do – as they still don’t understand enough about what forms the shape of these plasma jets.

While the image provides new insight, we still have a lot to learn – like what exactly happens at the boundary between the plasma jet and the black hole itself.

The team has calculated that this is something that they would be able to image in Centaurus A using the EHT at terahertz frequencies, whereas this image was captured at 228 gigahertz. Alternatively, they could use space-based telescopes instead of Earth-based telescopes to get a closer look.

For now, there is plenty of data from this image for astronomers to sink their teeth into, and hopefully this new view will help us get a better understanding of black holes, which remain some of the most mysterious objects in the known Universe.

The research has been published in Nature Astronomy.

Top image credit: Color composite image of Centaurus A and its jets. (ESO/WFI; MPIfR/ESO/APEX/A.Weiss et al.; NASA/CXC/CfA/R.Kraft et al.)

 

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Indian Coast Guard to get three more pollution control vessels to enhance capabilities

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Panaji: As a marine pollution control response, three more pollution control vessels (PCVs) will be added to the Indian Coast Guard’s (ICG) fleet, Union Defence Secretary Ajay Kumar said on Tuesday.

Speaking to reporters on the sidelines of the 8th National Pollution Response Exercise currently taking place in Goa, Kumar said that India is also willing to help friendly countries in upgrading their capabilities.

Around 19 friendly countries are participating in the exercise.

The Union government is continuously trying to upgrade the ICG’s capabilities to face pollution hazards in the ocean.

“Today, the Indian Coast Guard is capable of handling the highest level of oil spills in this region, which is 700 tonnes and above. Only a few countries in the world have this capability,” Kumar said.

Currently, the ICG has two dedicated vessels for pollution response, while three more will be added to its fleet to enhance its capability, he said.

The Indian Ocean is one of the busiest routes in the world and half of the trade takes place in the region, the senior official said, adding that oil exploration has also increase and accidents can happen anywhere.

Countries are also battling with the issue of plastic waste being dumped in the ocean, he said.

“We need to fight this (plastic pollution) collectively. It cannot be done by one country. All the coastal countries in the region need to make efforts,” Kumar said.

The defence secretary lauded the Punit Sagar Mission launched by Prime Minister Narendra Modi to clear plastic from the coastline.

“We should ensure that plastic waste is not washed into the ocean. Every year, 15,000 million tonnes of plastic washes into the Indian Ocean from different countries. If this continues, our marine life, environment, ecology and health will be affected,” he said.

Asked about cooperation from Pakistan and China over the pollution response, Kumar said, “This is an environmental issue and all countries should contribute towards it.” Several treaties have been signed to reduce pollution in the Indian Ocean, and friendly nations will have to collectively ensure that these are observed, he said.(GoaNewsHub)

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Brain Implant Translates Paralyzed Man’s Thoughts Into Text With 94% Accuracy

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A man paralyzed from the neck down due to a spinal cord injury he sustained in 2007 has shown he can communicate his thoughts, thanks to a brain implant system that translates his imagined handwriting into actual text.

 

The device – part of a longstanding research collaboration called BrainGate – is a brain-computer interface (BCI), that uses artificial intelligence (AI) to interpret signals of neural activity generated during handwriting.

In this case, the man – called T5 in the study, and who was 65 years of age at the time of the research – wasn’t doing any actual writing, as his hand, along with all his limbs, had been paralyzed for several years.

But during the experiment, reported in Nature earlier in the year, the man concentrated as if he were writing – effectively, thinking about making the letters with an imaginary pen and paper.

As he did this, electrodes implanted in his motor cortex recorded signals of his brain activity, which were then interpreted by algorithms running on an external computer, decoding T5’s imaginary pen trajectories, which mentally traced the 26 letters of the alphabet and some basic punctuation marks.

“This new system uses both the rich neural activity recorded by intracortical electrodes and the power of language models that, when applied to the neurally decoded letters, can create rapid and accurate text,” says first author of the study Frank Willett, a neural prosthetics researcher from Stanford University.

 

Similar systems developed as part of the BrainGate have been transcribing neural activity into text for several years, but many previous interfaces have focused on different cerebral metaphors for denoting which characters to write – such as point-and-click typing with a computer cursor controlled by the mind.

It wasn’t known, however, how well the neural representations of handwriting – a more rapid and dexterous motor skill – might be retained in the brain, nor how well they might be leveraged to communicate with a brain-computer interface, or BCI.

Here, T5 showed just how much promise a virtual handwriting system could offer for people who have lost virtually all independent physical movement.

BrainImpantDevice2A diagram of how the system works. (F. Willett et al., Nature, 2021, Erika Woodrum)

In tests, the man was able to achieve writing speeds of 90 characters per minute (about 18 words per minute), with approximately 94 percent accuracy (and up to 99 percent accuracy with autocorrect enabled).

Not only is that rate significantly faster than previous BCI experiments (using things like virtual keyboards), but it’s almost on par with the typing speed of smartphone users in the man’s age group – which is about 115 characters or 23 words per minute, the researchers say.

 

“We’ve learned that the brain retains its ability to prescribe fine movements a full decade after the body has lost its ability to execute those movements,” Willett says.

“And we’ve learned that complicated intended motions involving changing speeds and curved trajectories, like handwriting, can be interpreted more easily and more rapidly by the artificial-intelligence algorithms we’re using than can simpler intended motions like moving a cursor in a straight path at a steady speed.”

Basically, the researchers say that alphabetical letters are very different from one another in shape, so the AI can decode the user’s intention more rapidly as the characters are drawn, compared to other BCI systems that don’t make use of dozens of different inputs in the same way.

BrainImpantDevice2The man’s imagined handwriting, as interpreted by the system. (Frank Willett)

Despite the potential of this first-of-its-kind technology, the researchers emphasize that the current system is only a proof of concept so far, having only been shown to work with one participant, so it’s definitely not a complete, clinically viable product as yet.

The next steps in the research could include training other people to use the interface, expanding the character set to include more symbols (such as capital letters), refining the sensitivity of the system, and adding more sophisticated editing tools for the user.

There’s plenty of work to still be done, but we could be looking at an exciting new development here, giving the ability to communicate back to people who lost it.

“Our results open a new approach for BCIs and demonstrate the feasibility of accurately decoding rapid, dexterous movements years after paralysis,” the researchers write.

“We believe that the future of intracortical BCIs is bright.”

The findings are reported in Nature.

 

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Astronomers Detect a ‘Tsunami’ of Gravitational Waves. Here’s Where They’re Coming From

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The most recent gravitational wave observing run has netted the biggest haul yet.

In less than five months, from November 2019 to March 2020, the LIGO-Virgo interferometers recorded a massive 35 gravitational wave events. On average, that’s almost 1.7 gravitational wave events every week for the duration of the run.

 

This represents a significant increase from the 1.5-event weekly average detected on the previous run, and a result that has plumped up the number of total events to 90 since that first history-making gravitational wave detection in September 2015.

“These discoveries represent a tenfold increase in the number of gravitational waves detected by LIGO and Virgo since they started observing,” said astrophysicist Susan Scott of the Australian National University in Australia.

“We’ve detected 35 events. That’s massive! In contrast, we made three detections in our first observing run, which lasted four months in 2015-16. This really is a new era for gravitational wave detections and the growing population of discoveries is revealing so much information about the life and death of stars throughout the Universe.”

Of the 35 new detections, 32 are most likely the result of mergers between pairs of black holes. This is when pairs of black holes on a close orbit are drawn in by mutual gravity, eventually colliding to form one single, more massive black hole.

That collision sends ripples through space-time, like the ripples generated when you throw a rock in a pond; astronomers can analyze those ripples to determine the properties of the black holes.

mergersAn infographic showing the masses of all black hole mergers announced to date. (LIGO-Virgo/Aaron Geller/Northwestern University)

The data revealed a range of black hole masses, with the most massive clocking in at around 87 times the mass of the Sun. That black hole merged with a companion 61 times the mass of the Sun, resulting in a single black hole 141 times the mass of the Sun. That event is named GW200220_061928.

Another merger produced a black hole 104 times the mass of the Sun; both of these are considered intermediate mass black holes, a mass range between 100 and around a million solar masses, in which very few black holes have been detected.

 

GW200220_061928 is also interesting, because at least one of the black holes involved in the merger falls into what we call the upper mass gap. According to our models, black holes over about 65 solar masses can’t form from a single star, as stellar mass black holes do.

That’s because the precursor stars are so massive that their supernovae – known as pair-instability supernovae – ought to completely obliterate the stellar core, leaving nothing behind to gravitationally collapse into a black hole.

This suggests that the 87 solar mass black hole might be the product of a previous merger. GW200220_061928 isn’t the first that’s involved a black hole in the upper mass gap, but its detection does suggest that hierarchical black hole mergers are not uncommon.

And another event includes an object in the lower mass gap – a gap of black holes between 2.5 and 5 times the mass of the Sun. We’ve not conclusively found a neutron star larger than the former, or a black hole smaller than the latter; the event named GW200210_092254 involved an object clocking in at 2.8 solar masses. Astronomers have concluded that it’s probably a very small black hole.

 

“Looking at the masses and spins of the black holes in these binary systems indicates how these systems got together in the first place,” Scott said.

“It also raises some really fascinating questions. For example, did the system originally form with two stars that went through their life cycles together and eventually became black holes? Or were the two black holes thrust together in a very dense dynamical environment such as at the centre of a galaxy?”

The other three events out of the 35 involved a black hole and something else much less massive, likely a neutron star. These events are of great interest to astronomers, since they might reveal the stuff that’s inside a neutron star – if we ever detect one that emits light. By finding more of these mergers, we can start to build a better understanding of how they actually occur.

“Only now are we starting to appreciate the wonderful diversity of black holes and neutron stars,” said astronomer Christopher Berry of the University of Glasgow in the UK

“Our latest results prove that they come in many sizes and combinations – we have solved some long-standing mysteries, but uncovered some new puzzles too. Using these observations, we are closer to unlocking the mysteries of how stars, the building blocks of our Universe, evolve.”

The team’s paper has been submitted for publication, and can be found on preprint server arXiv.

 

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