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Astronomers take ‘heartbeat’ of black hole

Two screenshots of the animation of two phases of a black hole. On the left, a big and hot corona, the disk of material depicted in blue, has formed around the center of the black hole and there is no jet. On the right, the corona is smaller and cooler (depicted in red/orange) and the black hole ejects the jet. Credit: Méndez et al.

A black hole gets a large corona before it emits jets. This is revealed, among other things, by the heartbeat graph that an international team of astronomers has made of a black hole and a star orbiting around each other. The team, led by Mariano Méndez from the University of Groningen (the Netherlands), will publish their results on Monday in Nature Astronomy.

Just as the blood in a human heart cannot be in the atrium and the ventricles at the same time, a black hole also appears to first collect material and heat it up in a so-called corona, only then to spit it out in jets. “It sounds logical, but there has been a debate for 20 years about whether the corona and the jet were simply the same thing. Now we see that they arise one after the other and that the jet follows from the corona,” says principal investigator Mariano Méndez (Kapteyn Institute).

“It was quite a challenge to demonstrate this sequential nature. We had to compare data of years with that of seconds, and of very high energies with very low ones.”

15 years of data

The researchers collected 15 years of data from several telescopes. Amongst others, they pointed the Rossi X-ray Timing Explorer at the black hole GRS 1915+105 from space about every three days and collected high-energy X-ray radiation from the corona. The astronomers combined the X-ray data with those of the Ryle Telescope. This is a collection of radio dishes about ninety kilometers north of London, which collect low-energy radio radiation from the jet of the black hole almost every day.

Fragment of the ‘heartbeat’ of a black hole. The horizontal x-axis shows the days. The green curve is the radio emission. At the green peaks the jet is the strongest. The red and blue dots show the X-ray radiation and are a measure of the size of the corona. The blue dots show that the corona is smallest and the jet is strongest, so the jets always occur when the corona is smallest. Credit: Méndez et al.

The black hole GRS 1915+105 is not an isolated black hole, but a double system consisting of a black hole and a normal star that circle around each other. This double system lies in our Milky Way at about 36,000 light years from us in the direction of the constellation Aquila. The black hole weighs about 12 times as much as our Sun, making it one of the heaviest known stellar black holes.






Movie with sound like a heart monitor. Credit: Méndez et al.





Movie with sound and comparison with a heart monitor. Credit: Méndez et al.





Movie of the animation of two phases of a black hole. Credit: Méndez et al.

Unanswered questions

Now that the researchers have proven the sequence, there are still some unanswered questions. For example, the X-ray radiation that the telescopes collect from the corona contains more energy than can be explained by the temperature of the corona alone. The researchers suspect that a magnetic field provides extra energy. This magnetic field and the accompanying energy could also explain why jets are formed. If the magnetic field is chaotic, the corona heats up. If the magnetic field then becomes less chaotic, material can escape via the field lines into a jet.

The researchers suggest that the principle they demonstrated may also apply to heavier black holes, for example to the supermassive black hole at the center of our galaxy.


Less powerful black hole blows environment clean after all


More information:
Mariano Méndez, Coupling between the accreting corona and the relativistic jet in the microquasar GRS 1915+105, Nature Astronomy (2022). DOI: 10.1038/s41550-022-01617-y. www.nature.com/articles/s41550-022-01617-y
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Astronomers take ‘heartbeat’ of black hole (2022, March 7)
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Radioactive Kilonova Glow Suggests Rapid Spin Delayed Collapse of Neutron Stars Into Black Hole

In this artist’s representation, the merger of two neutron stars to form a black hole (hidden within bright bulge at center of image) generated opposing, high-energy jets of particles (blue) that heated up material around the stars, making it emit X-rays (reddish clouds). The Chandra X-ray Observatory is still detecting X-rays from the event today. They could be produced by a shock wave in the material around the black hole, or by material falling violently into the black hole (yellowish disk around central bulge). Credit: X-ray data from NASA, CXC and Northwestern Univ./A. Hajela; visual by NASA/CXC/M. Weiss

Excess X-ray emissions from remnant four years after merger hint at bounce from delayed collapse.

When two neutron stars spiral into one another and merge to form a

X-ray sources captured by Chandra, including, at top, the black hole that formed from the merger of two neutron stars and was first observed in 2017. Credit: NASA, CXC and Northwestern Univ./A. Hajela

Chandra, too, pivoted to observe GW170817, but saw no X-rays until nine days later, suggesting that the merger also produced a narrow jet of material that, upon colliding with the material around the neutron stars, emitted a cone of X-rays that initially missed Earth. Only later did the head of the jet expand and begin emitting X-rays in a broader jet visible from Earth.

The X-ray emissions from the jet increased for 160 days after the merger, after which they steadily grew fainter as the jet slowed down and expanded. But Hajela and her team noticed that from March 2020 — about 900 days after the merger — until the end of 2020, the decline stopped, and the X-ray emissions remained approximately constant in brightness.

“The fact that the X-rays stopped fading quickly was our best evidence yet that something in addition to a jet is being detected in X-rays in this source,” Margutti said. “A completely different source of X-rays appears to be needed to explain what we’re seeing.”

The researchers suggest that the excess X-rays are produced by a shock wave distinct from the jets produced by the merger. This shock was a result of the delayed collapse of the merged neutron stars, likely because its rapid spin very briefly counteracted the gravitational collapse. By sticking around for an extra second, the material around the neutron stars got an extra bounce that produced a very fast tail of kilonova ejecta that created the shock.

“We think the kilonova afterglow emission is produced by shocked material in the circumbinary medium,” Margutti said. “It is material that was in the environment of the two neutron stars that was shocked and heated up by the fastest edge of the kilonova ejecta, which is driving the shock wave.”

The merger of two neutron stars produced a black hole (center, white) and a burst of gamma-rays generated by a narrow jet or beam of high-energy particles, depicted in red. Initially, the jet was narrow and undetectable by Chandra, but as time passed the material in the jet slowed down and widened (blue) as it slammed into surrounding material, causing the X-ray emission to rise as the jet came into direct view by Chandra. This jet and its oppositely directed counterpart were likely generated by material falling onto the black hole after it formed. Credit: NASA/CXC/K. DiVona

The radiation is reaching us only now because it took time for the heavy kilonova ejecta to be decelerated in the low-density environment and for the kinetic energy of the ejecta to be converted into heat by shocks, she said. This is the same process that produces radio and X-rays for the jet, but because the jet is much, much lighter, it is immediately decelerated by the environment and shines in the X-ray and radio from the very earliest times.

An alternative explanation, the researchers note, is that the X-rays come from material falling towards the black hole that formed after the neutron stars merged.

“This would either be the first time we’ve seen a kilonova afterglow or the first time we’ve seen material falling onto a black hole after a (function(d, s, id){ var js, fjs = d.getElementsByTagName(s)[0]; if (d.getElementById(id)) return; js = d.createElement(s); js.id = id; js.src = "https://connect.facebook.net/en_US/sdk.js#xfbml=1&version=v2.6"; fjs.parentNode.insertBefore(js, fjs); }(document, 'script', 'facebook-jssdk'));

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The closest black hole to Earth is no more — in fact, it never existed

In 2020, astronomers identified a nearby star system that appeared to contain something phenomenal: the closest black hole to Earth, sitting a mere 1,000 light-years away (that’s less than 1% of the width of the Milky Way). Now, new research from some of those same astronomers suggests that they may have been deceived by a cosmic illusion.

In a new study published March 2 in the journal Astronomy & Astrophysics, researchers took another look at that star system — named HR 6819 — with the European Southern Observatory’s (ESO) Very Large Telescope. What appeared in 2020 to be a system of three massive objects — a large star orbiting a black hole every 40 days, with a second star orbiting much farther away — actually contains no black hole at all, the researchers wrote.

Instead, HR 6819 now appears to be a system of just two stars orbiting each other very closely, and with a very fraught relationship.

Related: 15 unforgettable images of stars

“Our best interpretation so far is that we caught this binary system in a moment shortly after one of the stars had sucked the atmosphere off its companion star,” study co-author Julia Bodensteiner, an ESO Fellow in Munich, Germany, said in a statement. “This is a common phenomenon in close binary systems, sometimes referred to as stellar vampirism.”

As a result, one star lost a tremendous amount of its mass to the other star around the time astronomers observed them in 2020 — making it appear as though the two stars were orbiting each other very far apart, when in fact one star was just much larger than the other, the researchers said. This vampiric mass transfer also would have made the recipient star spin more rapidly, further amplifying the illusion that it was much closer to Earth than its smaller companion star. No black hole required.

Bodensteiner and her colleagues originally proposed this vampire star hypothesis in a June 2020 paper in Astronomy & Astrophysics — one month after the publication of the paper claiming that HR 6819 contained the closest black hole to Earth. In the new paper, Bodensteiner and the authors of the original HR 6819 study joined forces to find out, once and for all, which one of them had the better theory about the strange star system’s behavior.

Using several of the Very Large Telescope’s high-definition instruments, the researchers found that the two stars in HR 6819 actually orbit one another at only one-third of the distance between Earth and the sun — meaning one of them was much larger and faster-spinning than the other. The vampire star hypothesis won out.

So, while Earth’s nearest known black hole may have just been pushed back a few thousand light-years (the next closest one sits about 3,000 light-years away, Live Science previously reported), HR 6819 remains an intriguing study target for other reasons entirely.

“Catching such a post-[vampirism] phase is extremely difficult as it is so short,” lead study author Abigail Frost, a postdoctoral researcher at KU Leuven in Belgium, said in the statement. “This makes our findings for HR 6819 very exciting, as it presents a perfect candidate to study how this vampirism affects the evolution of massive stars.”

Meanwhile, the search for nearby black holes continues undaunted. According to the study authors, there are tens of millions to hundreds of millions of black holes lurking in the Milky Way alone. It’s only a matter of time before astronomers stumble upon another one in our cosmic backyard.

Originally published on Live Science.

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Two black holes locked in cosmic dance near galaxy’s center are doomed to crash

Two huge black holes are locked together by gravity as they inevitably spiral towards a collision, researchers have found in a new study.

Researchers in a new study have spotted two supermassive black holes that whip around each other every two Earth years, on average, with respective masses each of hundreds of millions of times that of our sun. They found that the pair are also relatively close, being only about 2,000 Earth-sun distances apart (or about 50 times the distance between the sun and Pluto.)

“When the pair merge in roughly 10,000 years, the titanic collision is expected to shake space and time itself, sending gravitational waves across the universe,” the California Institute of Technology said of the objects in a statement.

Related: Did astronomers see light from two black holes colliding for the first time?

Described in the statement as the tightest-knit supermassive black hole duo yet observed, the study provides a unique laboratory to understand the dynamics of a quasar involved, called PKS 2131-021. 

Quasars are distant objects powered by black holes a billion times as massive as our sun. Astronomers are interested in these super-bright objects in part because quasars may give insight into the physics of the early universe.

Two supermassive black holes are seen orbiting each other in this artist’s loopable animation. (Image credit: Caltech/R. Hurt (IPAC))

If the findings from this study are confirmed, PKS 2131-021 is not alone in having a pair of supermassive black holes merging. The first suggested pair in quasar OJ 287, however, are much further apart and take nine years to circle each other.

Researchers in this study used 45 years of observations from multiple radio observatories to catch a powerful jet in action within PKS 2131-021, which appears to be moving back and forth as the pair of black holes orbit each other. The movement in turn causes changes in the brightness of radio waves observed at Earth.

“When we realized that the peaks and troughs of the light curve detected from recent times matched the peaks and troughs observed between 1975 and 1983, we knew something very special was going on,” Sandra O’Neill, lead author of the new study and an undergraduate astronomy student at Caltech, said in the same statement. 

Artist’s animation of a supermassive black hole circled by a spinning disk of gas and dust.  (Image credit: Caltech/R. Hurt (IPAC))

Galaxies commonly have huge black holes in their centers, including our own Milky Way. Galaxy mergers, when they occur, tend to see their respective black holes “sink” to the middle of the now combined, new galaxy and create an accordingly combined and more massive supermassive black hole.

The effects of such mergers create huge ripples across space and time, known as gravitational waves. Gravitational waves have been observed multiple times using the National Science Foundation’s LIGO (Laser Interferometer Gravitational-Wave Observatory) that is jointly managed by Caltech and the Massachusetts Institute of Technology.

That said, the supermassive black holes would not be visible to LIGO, as the black holes produce lower frequencies of gravitational waves that are undetectable in LIGO’s sensors. Caltech researchers say that the way to catch this in the future would be to use pulsar timing arrays, referring to radio telescopes that look at blinking stars called pulsars, according to the statement. In the meantime, light waves can show supermassive black holes in action.

A study based on this research was published Wednesday (Feb. 23) in the Astrophysical Journal Letters.

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2 monster black holes are headed toward a collision that will rock the fabric of space-time

Astronomers have discovered two supermassive black holes that are 99% of the way to a violent collision that will rock the very fabric of space-time.

The black holes, which share the name PKS 2131-021, are locked in a dance of doom about 9 billion light-years from Earth, according to a study published Feb. 23 in The Astrophysical Journal Letters. The two objects have moved steadily toward each other for about 100 million years, according to a statement from NASA, and now they share a binary orbit, with the two black holes orbiting each other every two years or so.

About 10,000 years from now, the two black holes will merge, sending gravitational waves — ripples in the fabric of space-time originally predicted by Albert Einstein — surging across the universe, the researchers said. Though none of us will witness that epic collision, studying PKS 2131-021 now could reveal new information about how supermassive black holes form and what happens when two of them collide.

Flickers of a monster

The binary black holes swirl around each other in this artist’s animation. The larger black hole blasts a jet of matter at near-light speed into space, allowing astronomers to detect it from Earth. (Image credit: Caltech/ R. Hurt)

Supermassive black holes — extremely dark, dense objects that are hundreds of millions of times more massive than Earth‘s sun — sit at the hearts of most, if not all, galaxies in the universe. Astronomers don’t know how these objects get to be quite so big, but one possibility is that the universe’s largest black holes result from at least one merger between two smaller black holes, according to NASA. The new study may help to confirm that hypothesis.

PKS 2131-021 is a special type of black hole known as a blazar — basically, a supermassive black hole that happens to be pointing a jet of supercharged matter directly at Earth. That matter originates from the rings of hot gas that form around certain black holes; when a black hole draws in that gas with its powerful gravity, some matter may escape, instead being propelled away in a jet of plasma traveling at nearly the speed of light.

The authors of the new study were monitoring the brightness of about 1,800 blazars scattered around the universe when they noticed something peculiar: The brightness of blazar PKS 2131-021 fluctuated at regular intervals — so predictably, in fact, that the study authors likened the fluctuations to the ticking of a clock.

The researchers suspected that these variations were the result of a second black hole tugging on the first as the two objects orbit each other every two years or so, but the team needed more data to see how long this pattern held. So the researchers dug into data from five observatories, spanning 45 years. All of the additional data matched the team’s predictions for how the binary blazar’s brightness should change over time.

If the findings are confirmed, PKS 2131-021 would be the second pair of binary black holes ever discovered — and the tightest-knit pair scientists have found. Scientists discovered the universe’s first known black hole binary candidate in 2020 in a galaxy about 3.5 billion light-years from Earth. However, those black holes orbit each other every nine years, suggesting there is a much greater distance between them than there is between the two members of PKS 2131-021.

The two monster black holes are large enough and close enough that they could unleash gravitational waves in advance of their inevitable collision, the study authors said in a statement. Future observations of PKS 2131-021 will focus on catching those waves in the act.

Originally published on Live Science.

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Astronomers Find Two Supermassive Black Holes Spiraling Toward a Cataclysmic Collision

A supermassive

If the team is correct, the diameter of the binary’s orbit is 10 to 100 times smaller than the only other known supermassive binary, and the pair will merge in roughly 10,000 years. That might seem like a long time, but it would take a total of about 100 million years for black holes of this size to begin orbiting one another and finally come together. So this pair is more than 99% of the way to a collision.

Joseph Lazio and Michele Vallisneri, at

In this illustration, light from a smaller black hole (left) curves around a larger black hole and forms an almost-mirror image on the other side. The gravity of a black hole can warp the fabric of space itself, such that light passing close to the black hole will follow a curved path around it. Credit: Caltech/R. Hurt (IPAC)

Evidence that this supermassive black hole may have a companion comes from observations by radio telescopes on Earth. Black holes don’t emit light, but their gravity can gather disks of hot gas around them and eject some of that material into space. These jets can stretch for millions of light-years. A jet pointed toward Earth appears far brighter than a jet pointed away from Earth. Astronomers call supermassive black holes with jets oriented toward Earth blazars, and a blazar named PKS 2131-021 is at the heart of this recent paper.

Located about 9 billion light-years from Earth, PKS 2131-021 is one of 1,800 blazars that a group of researchers at Caltech in Pasadena has been monitoring with the Owens Valley Radio Observatory in Northern California for 13 years as part of a general study of blazar behavior. But this particular blazar exhibits a strange behavior: Its brightness shows regular ups and downs as predictably as the ticking of a clock.

Researchers now think this regular variation is the result of a second black hole tugging on the first as they orbit each other about every two years. Each of the two black holes in PKS 2131-021 is estimated to be a few hundred million times the mass of our Sun. To confirm the finding, scientists will try to detect gravitational waves – ripples in space – coming from the system. The first detection of (function(d, s, id){ var js, fjs = d.getElementsByTagName(s)[0]; if (d.getElementById(id)) return; js = d.createElement(s); js.id = id; js.src = "https://connect.facebook.net/en_US/sdk.js#xfbml=1&version=v2.6"; fjs.parentNode.insertBefore(js, fjs); }(document, 'script', 'facebook-jssdk'));

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Supermassive black holes will smash into each other and warp space and time, scientists warn

Two massive black holes will merge in 10,000 years, in a collision that will send ripples across the universe, a new study finds.

The research, led by a team of astronomers from CalTech, found that two colossal black holes, about 9 billion light-years away in deep space, are revolving around one another every two years.

Each of the supermassive black holes has a mass that is hundreds of millions of times larger than that of our sun.

Furthermore, the two bodies are relatively close at just 1,950 astronomical units apart (about 50 times more than the distance between our Sun and Pluto)

The two objects are due to collide about 10,000 years from now, in a clash so intense that it will send gravitational waves across the fabrics of space and time.

The study, titled The Unanticipated Phenomenology of the Blazar PKS 2131–021: A Unique Supermassive Black Hole Binary Candidate, was published in The Astrophysical Journal Letters on Wednesday.

The authors say that despite the fact that galaxy mergers are not uncommon, “there are relatively few instances of two galaxies with supermassive black holes (SMBHs) in their nuclei being seen in the actual process of the merging.”

The researchers discovered the two bodies in an energy-packed object known as a quasar, which is a highly-luminous and active galactic nucleus that is powered by a supermassive black hole.

The collision isn’t expected to happen for another 10,000 years.
Getty Images

According to CalTech, some quasars’ supermassive black holes shoot a jet out at near the speed of light – in the new study, the quasar, designated PKS 2131-021, belongs to a subclass of quasars called blazars that shoot its jet toward our Earth.

The researchers posit that PKS 2131-021, which has been observed for over 45 years, is now the second known quasar with a pair of supermassive black holes that are due to merge.

The first known quasar is dubbed OJ 287, and it possesses two black holes that are further apart and circle one another every nine years.

So how do two supermassive black holes merge?

Typically when galaxies come together, their black holes are drawn in towards the middle of the new conjoined galaxy and eventually form an even bigger black hole.

And as the black holes are merging, their massive force disrupts the fabric of the universe with gravitational waves.

This article originally appeared on The Sun and was reproduced here with permission.

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2 Supermassive Black Holes Are Locked in The Tightest Orbit We’ve Seen Yet

A dance of death is taking place at the heart of a galaxy in the distant Universe.

Some 10 billion light-years away, two supermassive black holes are locked in an orbit so tight that they will collide with each other and form one much larger black hole in the relatively short time of just 10,000 years.

 

That equates to an orbital distance of just 0.03 light-years, around 50 times the average distance between the Sun and Pluto. Yet, so fast are they moving that it takes just two Earth years for the two objects to complete a binary orbit, compared to Pluto’s 248 years.

There are multiple reasons why supermassive black hole binaries are of interest to astronomers.

Supermassive black holes are found at the centers of most galaxies, the nuclei around which everything else whirls. When two are found together, it indicates that two galaxies have come together.

We know this process occurs, so finding a supermassive black hole binary can tell us what it looks like in the final stages.

Supermassive black hole binaries can also tell us something about how these colossal objects – millions to billions of times the mass of the Sun – can get so incredibly massive.

Binary black hole mergers are one way this growth can occur. Finding binary supermassive black holes will help us understand if it’s a common pathway for this growth, and that could lead to more accurate modeling.

 

The object in question is a quasar, named PKS 2131-021. These are galaxies in which the galactic nucleus is active; that is, the supermassive black hole is accreting matter at a furious rate, blazing with the heat generated by friction and gravity in the material roiling around the nucleus.

Some quasars blast jets of plasma almost at light-speed from the polar regions of the black hole, funneled along and accelerated by magnetic field lines around the object’s exterior. PKS 2131 is a quasar blasting out a jet right in the direction of Earth, making it what we call a blazar.

A team of astronomers studying brightness variations in quasars noticed something odd about the PKS 2131 blazar beam in radio frequencies, finding the same signature in data collected back in 2008. It seemed to oscillate on regular timescales, its brightness fluctuating with an almost perfect sine wave pattern never before seen in a quasar.

“PKS 2131 was varying not just periodically, but sinusoidally,” astronomer Tony Readhead of Caltech said. “That means that there is a pattern we can trace continuously over time.”

The trail seemed to end when only two more peaks were found in archival data, one in 2005, and another in 1981. But then, in 2021, the project piqued the interest of astronomer Sandra O’Neill of Caltech. She and a team of researchers revisited data archives to see how far back in time they could trace this strange pattern.

 

They hit paydirt. In data from the Haystack Observatory made between 1975 and 1983, more of the pattern emerged, consistent with the timing of the rest of the observations.

“When we realized that the peaks and troughs of the light curve detected from recent times matched the peaks and troughs observed between 1975 and 1983, we knew something very special was going on,” O’Neill said.

According to the team’s analysis, the regular ‘ticking’ of the signal is generated by the orbital motion of the two black holes. As they go around each other on two-year timescales, the radio light dims and brightens, due to the orbital motion of the jet, which causes a Doppler shift that boosts the light when the black hole is moving towards us.

The archival data shows that this sine wave can be observed consistently for eight years from 1976, after which it disappeared for 20 years. This was probably due to a change or disruption in the supply of material feeding into the supermassive black hole. After 20 years, the pattern re-emerged, and has continued ever since, about 17 years now, the researchers said.

Another similar system, OJ 287, suggests that the interpretation is valid. This blazar has two close supermassive black holes orbiting each other every 12 years, at a separation of a third of a light-year. It shows fluctuations in radio brightness, too, albeit more irregularly and without the sinusoidal waveform.

Although we won’t be around to see the eventual merger of the supermassive black holes in PKS 2131, they could show us how to look for similar systems. In turn, these could bring us closer to understanding how these colossal collisions take place.

The research has been published in The Astrophysical Journal Letters.

 

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A Black Hole Spins on Its Side – “Completely Unexpected”

Researchers from the University of Turku, Finland, found that the axis of rotation of a

Artist impression of the X-ray binary system MAXI J1820+070 containing a black hole (small black dot at the center of the gaseous disk) and a companion star. A narrow jet is directed along the black hole spin axis, which is strongly misaligned from the rotation axis of the orbit. Image produced with Binsim. Credit: R. Hynes

Often for the space systems with smaller objects orbiting around the central massive body, the own rotation axis of this body is to a high degree aligned with the rotation axis of its satellites. This is true also for our solar system: the planets orbit around the Sun in a plane, which roughly coincides with the equatorial plane of the Sun. The inclination of the Sun rotation axis with respect to orbital axis of the Earth is only seven degrees.

“The expectation of alignment, to a large degree, does not hold for the bizarre objects such as black hole X-ray binaries. The black holes in these systems were formed as a result of a cosmic cataclysm – the collapse of a massive star. Now we see the black hole dragging matter from the nearby, lighter companion star orbiting around it. We see bright optical and X-ray radiation as the last sigh of the infalling material, and also radio emission from the relativistic jets expelled from the system,” says Juri Poutanen, Professor of Astronomy at the University of Turku and the lead author of the publication. 


Artist impression of the X-ray binary system MAXI J1820+070 containing a black hole (small black dot at the center of the gaseous disk) and a companion star. A narrow jet is directed along the black hole spin axis, which is strongly misaligned from the rotation axis of the orbit. Image produced with Binsim. Credit: R. Hynes

By following these jets, the researchers were able to determine the direction of the axis of rotation of the black hole very accurately. As the amount of gas falling from the companion star to the black hole later began to decrease, the system dimmed, and much of the light in the system came from the companion star. In this way, the researchers were able to measure the orbit inclination using spectroscopic techniques, and it happened to nearly coincide with the inclination of the ejections.

“To determine the 3D orientation of the orbit, one additionally needs to know the position angle of the system on the sky, meaning how the system is turned with respect to the direction to the North on the sky. This was measured using polarimetric techniques,” says Juri Poutanen.

The results published in the Science magazine open interesting prospects towards studies of black hole formation and evolution of such systems, as such extreme misalignment is hard to get in many black hole formation and binary evolution scenarios.

“The difference of more than 40 degrees between the orbital axis and the black hole spin was completely unexpected. Scientists have often assumed this difference to be very small when they have modeled the behavior of matter in a curved time space around a black hole. The current models are already really complex, and now the new findings force us to add a new dimension to them,” Poutanen states.

Reference: “Black hole spin–orbit misalignment in the x-ray binary MAXI J1820+070” by Juri Poutanen, Alexandra Veledina, Andrei V. Berdyugin, Svetlana V. Berdyugina, Helen Jermak, Peter G. Jonker, Jari J. E. Kajava, Ilia A. Kosenkov, Vadim Kravtsov, Vilppu Piirola, Manisha Shrestha, Manuel A. Perez Torres and Sergey S. Tsygankov, 24 February 2022, Science.
DOI: 10.1126/science.abl4679

The key finding was made using the in-house built polarimetric instrument DIPol-UF mounted at the Nordic Optical Telescope, which is owned by the University of Turku jointly with the (function(d, s, id){ var js, fjs = d.getElementsByTagName(s)[0]; if (d.getElementById(id)) return; js = d.createElement(s); js.id = id; js.src = "https://connect.facebook.net/en_US/sdk.js#xfbml=1&version=v2.6"; fjs.parentNode.insertBefore(js, fjs); }(document, 'script', 'facebook-jssdk'));

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Ketanji Brown Jackson to be nominated as first Black woman to sit on Supreme Court

Biden will deliver remarks on Friday afternoon announcing the selection, the White House said. CNN first reported Biden’s decision.

She received and accepted Biden’s offer in a call Thursday night, a source familiar with the decision told CNN, but was present for DC Circuit Court hearings Friday morning.

Biden met with Jackson for her Supreme Court interview earlier this month, a senior administration official said, in a meeting that the White House managed to keep secret.

For more than a year, the President had familiarized himself with her work, reading many of her opinions and other writings, along with those of other contenders.

But the official said Biden also was impressed by her life story, including her rise from federal public defender to federal appellate judge — and her upbringing as the daughter of two public school teachers and administrators.

“President Biden sought a candidate with exceptional credentials, unimpeachable character and unwavering dedication to the rule of law,” the senior official said.

From the beginning, Jackson was the leading contender, but the official said the President gave “considerable weight” to other finalists, including Judge J. Michelle Childs and California Supreme Court Justice Leondra Kruger.

The President reached his final decision this week, the official said, and extended the offer to her in a phone call on Thursday evening. She accepted in the call, which lasted several minutes.

The White House considered delaying the announcement, given the Russian invasion in Ukraine, but believed it was critical to get the second phase of the confirmation process moving, the official said.

In a statement, the White House cited Jackson’s “broad experience across the legal profession,” pointing to her career as a federal appellate judge, a federal district court judge, a member of the US Sentencing Commission, an attorney in private practice and as a federal public defender. The White House described Jackson as “an exceptionally qualified” and “historic” nominee, calling on the Senate to “move forward with a fair and timely hearing and confirmation.”

Jackson clerked for Breyer and served as a federal public defender in Washington — an experience that her backers say is fitting, given Biden’s commitment to putting more public defenders on the federal bench. She was also a commissioner on the US Sentencing Commission and served on the federal district court in DC, as an appointee of President Barack Obama, before Biden elevated her to the DC Circuit last year.

Opportunity for Biden to excite Democrats

Biden’s pick is a chance for him to fire up a Democratic base that is less excited to vote in this year’s midterm elections than it has been over the past several election cycles. It’s also a welcome change of topic for the President, whose approval ratings have been sagging in recent months as the Covid-19 pandemic has dragged on and inflation has affected consumers across the nation. The selection gives Biden a chance to deliver on one of his top campaign promises, and he’ll hope that the Black voters who were crucial to his election win will see this as a return on their investment.

Though it is historic, the choice of Jackson will not change the ideological makeup of the court. The court currently has six conservative justices and three liberal justices — and the retiring Breyer comes from the liberal camp. The court is already poised to continue its turn toward the right with high-profile cases and rulings expected from the court in the coming months on abortion, gun control and religious liberty issues.

Eyes will now turn to the Senate, where Biden’s Democratic Party holds the thinnest possible majority. The President will hope that Jackson can garner bipartisan support, but Democrats will need all their members in Washington to ensure her confirmation. Unlike for most major pieces of legislation, Democrats do not need Republican help to confirm a Supreme Court justice and can do it with their 50 votes and Vice President Kamala Harris breaking a deadlock. When Jackson was confirmed to the appellate bench, she had the support of three Republican senators.

Jackson is expected to have her courtesy meetings with senators next week, according to a person familiar with the plans. It’s common for Supreme Court nominees to meet with the leadership on both sides, then members of the Senate Judiciary Committee.

As a judge in DC — where some of the most politically charged cases are filed — Jackson’s issued notable rulings touching on Congress’ ability to investigate the White House. As a district court judge, she wrote a 2019 opinion siding with House lawmakers who sought the testimony of then-White House Counsel Don McGahn. Last year, she was on the unanimous circuit panel that ordered disclosure of certain Trump White House documents to the House January 6 committee.

The White House indicated her time in the federal public defenders’ office was critical to Biden’s selection, setting her apart from other candidates. Biden sought “an individual who is committed to equal justice under the law and who understands the profound impact that the Supreme Court’s decisions have on the lives of the American people,” the White House said.

Following Breyer’s retirement announcement in late January, Biden began reviewing background materials, such as legal records and writings, about his potential picks.

Biden first committed to nominating a Black female US Supreme Court justice when he was running for president in 2020. On a debate stage in South Carolina, Biden argued that his push to make “sure there’s a Black woman on the Supreme Court” was rooted in an effort to “get everyone represented.”

Coming from ‘a background of public service’

Jackson was born in the nation’s capital but grew up in the Miami area. She was a member of the debate team at Miami Palmetto Senior High School before earning both her undergraduate degree and law degree at Harvard.

At her 2021 confirmation hearing for the appellate court, she connected her family’s professions — her parents worked in public schools — to her decision to work as a public defender.

“I come from a background of public service. My parents were in public service, my brother was a police officer and (was) in the military,” she said at the time, “and being in the public defenders’ office felt very much like the opportunity to help with my skills and talents.”

Former House Speaker Paul Ryan, a Republican, is a relative by marriage and introduced her at the 2013 hearing for her district court nomination.

Conservatives have already previewed how they will scrutinize her record defending Guantanamo Bay detainees as a public defender. The role she played in her uncle’s successful efforts to seek a commutation from former President Barack Obama has also attracted attention. When she was in private practice in 2008, she referred her uncle’s file to the firm Wilmer Hale, which several years later submitted the file.

As a judge, some other notable cases she has in her record are a 2018 case brought federal employee unions where she blocked parts of executive orders issued by former President Donald Trump, and a case where she ruled against Trump policies that expand the categories of non-citizens who could be subject to expedited removal procedures without being able to appear before a judge.

Jackson penned more than 500 opinions in the eight years she spent on the district court.

Republicans signal potential opposition

Though Biden has said that he’d pick a nominee with bipartisan appeal who is “worthy of Justice Breyer’s legacy of excellence and decency,” his decision to name the first Black woman to the court is already facing Republican opposition. Several Senate Republicans have told CNN they disagreed with the President’s decision to name a Black woman to the court rather than judging a nominee squarely on their credentials, even though Ronald Reagan and Trump both said they’d name a female justice to the Supreme Court when they were on the campaign trail.

Even before Biden nominated Jackson, GOP senators and Senate candidates were already concluding that she’d be far left, throwing cold water on the names floated as being on Biden’s potential short list and calling for a slow confirmation process. Still, Republicans are limited in their ability to block a Supreme Court nominee, and Jackson may win the support of some GOP senators.

Sens. Lisa Murkowski of Alaska, Lindsey Graham of South Carolina and Susan Collins of Maine all voted for Jackson last summer when she was confirmed as a circuit court judge on the US Court of Appeals for the District of Columbia, the second most important court in the country.

But on Friday, Graham, who had expressed support for Childs, suggested Jackson does not have his approval, saying in a tweet that the choice of Jackson “means the radical Left has won President Biden over yet again.” Graham added that he expects a “respectful but interesting hearing in the Senate Judiciary Committee.”

Senate Minority Leader Mitch McConnell called for a “rigorous, exhaustive” review of Jackson in a statement.

“I also understand Judge Jackson was the favored choice of far-left dark-money groups that have spent years attacking the legitimacy and structure of the Court itself,” McConnell said.

Senate Majority Leader Chuck Schumer has indicated that he wants to push a nominee through the process quickly, using Supreme Court Justice Amy Coney Barrett’s Senate proceedings as a model for Jackson’s confirmation timeline. And Sen. Dick Durbin, the chairman of the Senate Judiciary Committee, told CNN recently that he expects to have a hearing within a few weeks of the selection. The goal of the leadership is to have the nominee confirmed by the April 11 recess.

This story has been updated with additional developments, reaction and background information.

CNN’s John Harwood, and Manu Raju contributed to this report.

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