Saturday, August 07, 2021

Space Station Incident Demands Independent Investigation

A space expert warns NASA's safety culture may be eroding again

JAMES OBERG
06 AUG 2021




Russia's "Nauka" Multipurpose Laboratory Module is pictured shortly after docking to the Zvezda service module's Earth-facing port on the International Space Station, with the Brazilian coast 263 miles below. In the foreground is the Soyuz MS-18 crew ship docked to the Rassvet module on 29 July 2021.

NASA

This is a guest post. The views expressed here are solely those of the author and do not represent positions of IEEE Spectrum or the IEEE.

In an International Space Station major milestone more than fifteen years in the making, a long-delayed Russian science laboratory named Nauka automatically docked to the station on 29 July, prompting sighs of relief in the Mission Control Centers in Houston and Moscow. But within a few hours, it became shockingly obvious the celebrations were premature, and the ISS was coming closer to disaster than at anytime in its nearly 25 years in orbit.

While the proximate cause of the incident is still being unravelled, there are worrisome signs that NASA may be repeating some of the lapses that lead to the loss of the Challenger and Columbia space shuttles and their crews. And because political pressures seem to be driving much of the problem, only an independent investigation with serious political heft can reverse any erosion in safety culture.

Let's step back and look at what we know happened: In a cyber-logical process still not entirely clear, while passing northwest to southeast over Indonesia, the Nauka module's autopilot apparently decided it was supposed to fly away from the station. Although actually attached, and with the latches on the station side closed, the module began trying to line itself up in preparation to fire its main engines using an attitude adjustment thruster. As the thruster fired, the entire station was slowly dragged askew as well.

Since the ISS was well beyond the coverage of Russian ground stations, and since the world-wide Soviet-era fleet of tracking ships and world-circling network of "Luch" relay comsats had long since been scrapped, and replacements were slow in coming, nobody even knew Nauka was firing its thruster, until a slight but growing shift in the ISS's orientation was finally detected by NASA.

Nauka approaches the space station, preparing to dock on 29 July 2021. NASA

Within minutes, the Flight Director in Houston declared a "spacecraft emergency"—the first in the station's lifetime—and his team tried to figure out what could be done to avoid the ISS spinning up so fast that structural damage could result. The football-field-sized array of pressurized modules, support girders, solar arrays, radiator panels, robotic arms, and other mechanisms was designed to operate in a weightless environment. But it was also built to handle stresses both from directional thrusting (used to boost the altitude periodically) and rotational torques (usually to maintain a horizon-level orientation, or to turn to a specific different orientation to facilitate arrival or departure of visiting vehicles). The juncture latches that held the ISS's module together had been sized to accommodate these forces with a comfortable safety margin, but a maneuver of this scale had never been expected.

Meanwhile, the station's automated attitude control system had also noted the deviation and began firing other thrusters to countermand it. These too were on the Russian half of the station. The only US orientation-control system is a set of spinning flywheels that gently turn the structure without the need for thruster propellant, but which would have been unable to cope with the unrelenting push of Nauka's thruster. Later mass-media scenarios depicted teams of specialists manually directing on-board systems into action, but the exact actions taken in response still remain unclear—and probably were mostly if not entirely automatic. The drama continued as the station crossed the Pacific, then South America and the mid-Atlantic, finally entering Russian radio contact over central Europe an hour after the crisis had begun. By then the thrusting had stopped, probably when the guilty thruster exhausted its fuel supply. The sane half of the Russian segment then restored the desired station orientation.

Initial private attempts to use telemetry data to visually represent the station's tumble that were posted online looked bizarre, with enormous rapid gyrations in different directions. Mercifully, the truth of the situation is that the ISS went through a simple long-axis spin of one and a half full turns, and then a half turn back to the starting alignment. The jumps and zig-zags were computational artifacts of the representational schemes used by NASA, which relate to the concept of "gimbal lock" in gyroscopes.

How close the station had come to disaster is an open question, and the flight director humorously alluded to it in a later tweet that he'd never been so happy as when he saw on external TV cameras that the solar arrays and radiators were still standing straight in place. And any excessive bending stress along docking interfaces between the Russian and American segments would have demanded quick leak checks. But even if the rotation was "simple," the undeniably dramatic event has both short term and long-term significance for the future of the space station. And it has antecedents dating back to the very birth of the ISS in 1997.

How close the ISS had come to disaster is still an open question.


At this point, unfortunately, is when the human misjudgments began to surface. To calm things down, official NASA spokesmen provided very preliminary underestimates in how big and how fast the station's spin had been. These were presented without any caveat that the numbers were unverified—and the real figures turned out to be much worse. The Russian side, for its part, dismissed the attitude deviation as a routine bump in a normal process of automatic docking and proclaimed there would be no formal incident investigation, especially any that would involve their American partners. Indeed, both sides seemed to agree that the sooner the incident was forgotten, the better. As of now, the US side is deep into analysis of induced stresses on critical ISS structures, with the most important ones, such as the solar arrays, first. Another standard procedure after this kind of event is to assess potential indicators of stress-induced damage, especially in terms of air leaks, and where best to monitor cabin pressure and other parameters to detect any such leaks.

The bureaucratic instinct to minimize the described potential severity of the event needs cold-blooded assessment. Sadly, from past experience, this mindset of complacency and hoping for the best is the result of natural human mental drift that comes when there are long periods of apparent normalcy. Even if there is a slowly emerging problem, as long as everything looks okay in the day to day, the tendency is ignore warning signals as minor perturbations. The safety of the system is assumed rather than verified—and consequently managers are led into missing clues, or making careless choices, that lead to disaster. So these recent indications of this mental attitude about the station's attitude are worrisome. The NASA team has experienced that same slow cultural rot of assuming safety several times over the past decades, with hideous consequences. Team members in the year leading up to the 1986 Challenger disaster (and I was deep within the Mission Control operations then) had noticed and begun voicing concerns over growing carelessness and even humorous reactions to occasional "stupid mistakes," without effect. Then, after imprudent management decisions, seven people died.

The same drift was noticed in the late 1990s, especially in the joint US/Russian operations on Mir and on early ISS flights. It led to the forced departure of a number of top NASA officials, who had objected to the trend that was being imposed by the White House's post-Cold War diplomatic goals, implemented by NASA Administrator Dan Goldin. Safety took a decidedly secondary priority to international diplomatic value. Legendary Mission Control leader Gene Kranz described the decisions that were made in the mid-1990s over his own objections, objections that led to his sudden departure from NASA. "Russia was subsequently assigned partnership responsibilities for critical in-line tasks with minimal concern for the political and technical difficulties as well as the cost and schedule risks," he wrote in 1999. "This was the first time in the history of US manned space flight that NASA assigned critical path, in-line tasks with little or no backup." By 2001-'02, the results were as Kranz and his colleagues had warned. "Today's problems with the space station are the product of a program driven by an overriding political objective and developed by an ad hoc committee, which bypassed NASA's proven management and engineering teams," he concluded.

To reverse the apparent new cultural drift, NASA headquarters or some even higher office is going to have to intervene.

By then the warped NASA management culture that soon enabled the Columbia disaster in 2003 was fully in place. Some of the wording in current management proclamations regarding the Nauka docking have an eerie ring of familiarity. "Space cooperation continues to be a hallmark of U.S.-Russian relations and I have no doubt that our joint work reinforces the ties that have bound our collaborative efforts over the many years" wrote NASA Director Bill Nelson to Dmitry Rogozin, head of the Russian space agency, on July 31. There was no mention of the ISS's first declared spacecraft emergency, nor any dissatisfaction with Russian contribution to it.

To reverse the apparent new cultural drift, and thus potentially forestall the same kind of dismal results as before, NASA headquarters or some even higher office is going to have to intervene. The causes of the Nauka-induced "space sumo match" of massive cross-pushing bodies need to be determined and verified. And somebody needs to expose the decision process that allowed NASA to approve the ISS docking of a powerful thruster-equipped module without the on-site real-time capability to quickly disarm that system in an emergency. Because the apparent sloppiness of NASA's safety oversight on visiting vehicles looks to be directly associated with maintaining good relations with Moscow, the driving factor seems to be White House diplomatic goals—and that's the level where a corrective impetus must originate. With a long-time U.S. Senate colleague, Nelson, recently named head of NASA, President Biden is well connected to issue such guidance for a thorough investigation by an independent commission, followed by implementation of needed reforms. The buck stops with him.

As far as Nauka's role in this process of safety-culture repair, it turns out that quite by bizarre coincidence, a similar pattern was played out by the very first Russian launch that inaugurated the ISS program, the 'Zarya' module [called the 'FGB'] in late 1997. Nauka turns out to be the repeatedly rebuilt and upgraded backup module for that very launch, and the parallels are remarkable. The day the FGB was launched, on 23 November 1997, the mission faced disaster when it refused to accept ground commands to raise its original atmosphere-skimming parking orbit. As it crossed over Russian ground sites, controllers in Moscow sent commands, and the spacecraft didn't answer. Meanwhile, NASA guests at a nearby facility were celebrating with Russian colleagues as nobody told them of the crisis. Finally, on the last available in-range pass, controllers tried a new command format that the onboard computer did recognize and acknowledge. The mission—and the entire ISS project—was saved, and the American side never knew. Only years later did the story appear in Russian newspapers.

Still, for all its messy difficulties and frustrating disappointments, the U.S./Russian partnership turned out to be a remarkably robust "mutual co-dependence" arrangement, when managed with "tough love." Neither side really had practical alternatives if it wanted a permanent human presence in space, and they still don't—so both teams were devoted to making it work. And it could still work—if NASA keeps faith with its traditional safety culture and with the lives of those astronauts who died in the past because NASA had failed them.

Postscript: As this story was going to press, a NASA spokesperson responded to queries about the incident saying:

As shared by NASA's Kathy Lueders and Joel Montalbano in the media telecon following the event, Roscosmos regularly updated NASA and the rest of the international partners on MLM's progress during the approach to station. We continue to have confidence in our partnership with Roscosmos to operate the International Space Station. When the unexpected thruster firings occurred, flight control teams were able to enact contingency procedures and return the station to normal operations within an hour. We would point you to Roscosmos for any specifics on Russian systems/performance/procedures.

James Oberg is a retired "rocket scientist" in Texas, after a 20+ year career in NASA Mission Control and subsequently an on-air space consultant for ABC News and then NBC News. The author of a dozen books and hundreds of magazine articles on the past, present, and potential future of space exploration, he has reported from space launch and operations centers across the United States and Russia and North Korea. His home page is www.jamesoberg.com.

How the space station flipped out of control—and why that's a big problem
An unusual day aboard the ISS.

By Mark Kaufman on August 6, 2021


The International Space Station orbiting above Earth. Credit: Nasa


The International Space Station flipped over on its back on July 29.

This was a significant, though fortunately not disastrous, nearly one-hour episode for humanity's largest and oldest space outpost. The station slowly turned over one and a half times. (Or as NASA describes it, the space station experienced a "total attitude change" of around 540 degrees, with "attitude" being jargon for a spacecraft's orientation.) The new Russian module "Nauka" had docked to the sizeable 356-foot-long station, but Nauka's thrusters fired when they shouldn't have, causing the space station to start unexpectedly spinning.

"It was quite an event," said Keith Crisman, an assistant professor of space studies at the University of North Dakota who researches safety systems for human spaceflight. "It was a potentially serious issue," Crisman added, noting that an out-of-control spacecraft is one of the highest-risk events in space.

Later on July 29, after flight engineers had righted the space station, NASA held a media briefing to address the unusual event. The agency's summary: All is OK, the space station had returned to normal, and nobody aboard was in danger. In fact, a NASA public affairs officer said in an email that the station's spin was "slow enough to go unnoticed by the crew members on board" (until they received warning messages), and everything else operated normally.

While it's fortunate the astronauts and cosmonauts aboard are OK, the event still carries questions about what happened, along with future concerns about space station safety. "When spacecraft misfire it's a serious thing."

"When spacecraft misfire it's a serious thing," said Jonathan McDowell, an astronomer at the Harvard-Smithsonian Center for Astrophysics who tracks rocket and spacecraft launches. "I cannot imagine there aren't some very serious conversations going on at NASA."



What went wrong

As noted above, thrusters on Nauka started firing after the module docked to the space station, forcing the station to (slowly) spin at a maximum of half a degree per second. It ended up upside down, before the correction. On spacecraft, these types of misfires do sometimes happen, and more easily than engineers would like, explained Kurt Anderson, a professor of mechanical aerospace engineering at Rensselaer Polytechnic Institute.

In 2016, for example, a thruster on Japan's 46-foot long astronomy satellite Hitomi misfired. Hitomi spun uncontrollably and broke apart. And perhaps most famously, the small spacecraft Gemini VIII (piloted by legendary astronaut Neil Armstrong in 1966) violently spun out of control after a thruster problem, but Armstrong impressively stopped the wild tumble, and narrowly avoided national tragedy.

(The space station, fortunately, is a big, over 925,000-pound object with lots of material to turn, so Nauka's thrusters didn't have a chance to get the station spinning treacherously.)

Life on the space station in 2020. Credit: NASA

But what triggered Nauka's mishap? A software glitch likely played a role. Nauka experienced some minor software issues before arriving at the space station, noted Crisman. The day after the unexpected flip, the Russian space agency Roscosmos officially blamed the event on a software glitch, causing thrusters to fire out and try to withdraw Nauka, which had just docked several hours before. That's as much as we currently know, which comes from a four-paragraph Roscosmos press release.

After the thrusters began misfiring, the space station soon entered an official "Loss of Attitude Control," the NASA representative told Mashable. The blasting thrusters were countered by other space station thrusters firing in the opposite direction to regain the station's normal orientation, NASA said. The station had to flip completely over — by 180 degrees — to right itself.

Real concerns


The space station excitement comes with some notable concerns, according to experts outside of NASA.

1. The space station is old and not meant for acrobatics. People first inhabited the station over two decades ago. "The ISS is an older piece of equipment. We call it legacy equipment," said Crisman.

It's not a spry vehicle intended to flip around, though the flipping in this case wasn't nearly violent. However, the station experienced thrusters fighting with each other for control of the craft, noted McDowell, which is undoubtedly somewhat strenuous for a spacecraft with attached instruments, like huge solar arrays branching out from the station. "You've got torque on relatively old parts," explained Crisman.

2. Wasted precious fuel: Stopping the station's flip required firing propellant from thrusters, which is problematic because propellant in space is finite, and at times necessary in order to maneuver the space station. There's no other way to purposefully move. "Propellant is blood."

"Propellant is blood," said Anderson. Unlike for most spacecraft, however, NASA can launch more propellant to the space station, though at a cost.

3. The misfiring thrusters couldn't immediately be turned off. To stop the station from spinning, ground control operators in Russia needed to tell the automated Nauka to stop firing. But this didn't work, necessitating the counter-thrusting. "That they couldn't get the thrusters shut off immediately bothers me," said the aerospace engineer Anderson.

4. Things could have been worse — much, much worse.

Any mishap on the space station has the benefit of happening under the watchful eye of NASA's space station team in Houston. "They have a really excellent flight control team," said McDowell, of the Center for Astrophysics.

NASA's flight controllers, like flight director Zebulon Scoville, immediately noticed the station's unexpected behavior, and soon declared a "spacecraft emergency."

Yet there shouldn't have ever been an emergency, emphasized Crisman. Yes, errors are inevitable, but the system shouldn't allow such an issue to percolate down into a potentially serious, active problem. "We should have systems in place to mitigate those errors," he said.

Broadly, these systems should follow the "Swiss Cheese Model," Crisman explained. Different layers of naturally imperfect departments (or layers of Swiss cheese) like mission control, computer programmers, engineers building spacecraft, etc. should make it extremely difficult for an error to find its way through the small holes in each department's slice of Swiss. In the case of the space station flipping, an error slipped through many, many layers of international Swiss cheese. "Humans are perfectly fallible, and machines are perfectly fallible."

Generally, the space station is a quiet place, tranquilly orbiting some 250 miles above Earth. It's an afterthought to many of us. But things can go wrong. It's hugely fortunate, for example, that Nauka didn't start misfiring as it was docking, potentially leading to an impact with the space station.

This recent flip wasn't terrible, but it's a poignant warning of our vulnerabilities in the harsh realm of space, even on the dependable space station.

"Space is dangerous," said Crisman. "Humans are perfectly fallible, and machines are perfectly fallible."













Mysteries of the Oort cloud at the edge of our solar system

The entirely theoretical cloud of icy space debris marks the frontiers of our solar system.
RELATED TOPICS: THE SOLAR SYSTEM
Naeblys/Shutterstock

The Oort cloud represents the very edges of our solar system. The thinly dispersed collection of icy material starts roughly 200 times farther away from the sun than Pluto and stretches halfway to our sun’s nearest starry neighbor, Alpha Centauri. We know so little about it that its very existence is theoretical — the material that makes up this cloud has never been glimpsed by even our most powerful telescopes, except when some of it breaks free.

“For the foreseeable future, the bodies in the Oort cloud are too far away to be directly imaged,” says a spokesperson from NASA. “They are small, faint, and moving slowly.”

Aside from theoretical models, most of what we know about this mysterious area is told from the visitors that sometimes swing our way every 200 years or more — long period comets. “[The comets] have very important information about the origin of the solar system,” says Jorge Correa Otto, a planetary scientist the Argentina National Scientific and Technical Research Council (CONICET).\

A Faint Cloud, in Theory

The Oort cloud’s inner edge is believed to begin roughly 1,000 to 2,000 astronomical units from our sun. Since an astronomical unit is measured as the distance between the Earth and the sun, this means it’s at least a thousand times farther from the sun than we are. The outer edge is thought to go as far as 100,000 astronomical units away, which is halfway to Alpha Centauri. “Most of our knowledge about the structure of the Oort cloud comes from theoretical modeling of the formation and evolution of the solar system,” the NASA spokesperson says.

While there are many theories about its formation and existence, many believe that the Oort cloud was created when many of the planets in our solar system were formed roughly 4.6 billion years ago. Similar to the way the Asteroid Belt between Mars and Jupiter sprung to life, the Oort cloud likely represents material left over from the formation of giant planets like Jupiter, Neptune, Uranus and Saturn. The movements of these planets as they came to occupy their current positions pushed that material past Neptune’s orbit, Correa Otto says.

Another recent study holds that some of the material in the Oort cloud may be gathered as our sun “steals comets” orbiting other stars. Basically, the theory is that comets with extremely long distances around our neighboring stars get diverted when coming into closer range to our sun, at which point they stick around in the Oort cloud.

The composition of the icy objects that form the Oort cloud is thought to be similar to that of the Kuiper Belt, a flat, disk-shaped area beyond the orbit of Neptune we know more about. The Kuiper Belt also consists of icy objects leftover from planet formation in the early history of our solar system. Pluto is probably the most famous object in this area, though NASA’s New Horizons space probe flew by another double-lobed object in 2019 called Arrokoth — currently the most distant object in our solar system explored up close, according to NASA.

“Bodies in the Oort cloud, Kuiper belt, and the inner solar system are all believed to have formed together, and gravitational dynamics in the solar system kicked some of them out,” the NASA spokesperson says.

Visitors from the Edge of our Solar System

Estonian philosopher Ernst Öpik first theorized that long-period comets might come from an area at the edge of our solar system. Then, Dutch astronomer Jan Oort predicted the existence of his cloud in the 1950s to better understand the paradox of long-period comets.

Oort's theory was that comets would eventually strike the sun or a planet, or get ejected from the solar system when coming into closer contact with the strong orbit of one of those large bodies. Furthermore, the tails that we see on comets are made of gasses burned off from the sun’s radiation. If they made too many passes close to the sun, this material would have burned off. So they must not have spent all their existence in their current orbits. “Occasionally, Oort cloud bodies will get kicked out of their orbits, probably due to gravitational interactions with other Oort cloud bodies, and come visit the inner solar system as comets,” the NASA spokesperson says.

Correa Otto says that the direction of comets also supports the Oort cloud’s spherical shape. If it was shaped more like a disk, similar to the Kuiper Belt, comets would follow a more predictable direction. But the comets that pass by us come from random directions. As such, it seems the Oort cloud is more of a shell or bubble around our solar system than a disk like the Kuiper Belt. These long-period comets include C/2013 A1 Siding Spring, which passed close to Mars in 2014 and won’t be seen again for another 740,000 years.

“No object has been observed in the distant Oort cloud itself, leaving it a theoretical concept for the time being. But it remains the most widely-accepted explanation for the origin of long-period comets,” NASA says.

The Oort cloud, if it indeed exists, likely isn’t unique to our own solar system. Correa Otto says that some astronomers believe these clouds exist around many solar systems. The trouble is, we can’t even yet see our own, let alone those of our neighboring systems. The Voyager 1 spacecraft is headed in that direction — it’s projected to reach the inner edge of our Oort cloud in roughly 300 years. Unfortunately, Voyager will have long since stopped working.

“Even if it did [still work], the Sun’s light is so faint, and the distances so vast, that it would be unlikely to fly close enough to something to image it,” the NASA spokesperson says. In other words, it would be difficult to tell you’re in the Oort cloud even if you were right inside it.

Investigation Into the Origin of Elements in the Universe Yields New Insights

Sun Star Animation

A key reaction in the slow neutron-capture process that forms elements occurs less frequently than previously thought.

The Science

The slow neutron-capture process (the s-process) is one of the nucleosynthesis processes that occurs in stars. It results in about half of the elements heavier than iron in the universe. Two important reactions involved in the s-process are Neon-22 (alpha, gamma) and Neon-22 (alpha, neutron). In these reactions, neutron-rich Neon-22 captures alpha-particles. The capture produces Magnesium-26 in an excited state, meaning it has received extra energy. It then releases energy by emitting either a gamma ray, leading to Magnesium-26 in a normal state, or a neutron, leading to Magnesium-25. The rates of both the Neon-22 (alpha, gamma) and Neon-22 (alpha, neutron) reactions have significant effects on the s-process. This affects the abundances of elements such as Selenium, Krypton, Rubidium, Strontium, and Zirconium.

Neon Captures Alpha-Particle To Create Magnesium-26


An isotope of Neon (22Ne) captures an alpha-particle (α) to create Magnesium-26 (26Mg) in an excited state. The excited Magnesium-26 then releases energy by emitting a gamma ray (γ), leading to Magnesium-26 or a neutron, leading to Magnesium-25. Credit: Image courtesy of Dustin Scriven, Texas A&M University

The Impact

Scientists are trying to answer the question, what is the origin of elements in the universe? The answer is extremely complex. It requires a collaborative effort by researchers in many fields and an enormous amount of experimental data. One part of answering this question is understanding the specific processes that create elements heavier than iron. Some of these elements form through particular nuclear reactions inside stars that involve neutron captures (the s-process). Neutrons are unstable and need to be produced continuously to fuel this process. Determining the intensities of neutron source reactions is important to understanding this nucleosynthesis scenario.

Summary

Two reactions have a strong influence on the neutron flux during the s-process, 22Ne(α, γ)26Mg and 22Ne(α, n)25Mg. The probabilities of these reactions occurring are difficult to measure directly because these probabilities (called reaction cross sections) are extremely low at the energies relevant for stellar nucleosynthesis. A team of nuclear physicists used two indirect methods to determine the probabilities for both reactions. Both methods used a 22-Neon beam produced at the Texas A&M University Cyclotron Institute. In one study, the team measured the likelihood for the most relevant excited states in 26-Magnesium to decay by alpha-particles. The other experiment involved direct measurements of neutron/gamma branching ratios for the same excited states. Combining these studies led researchers to a consistent conclusion: that the actual probability of the 22Ne(α, n)25Mg reaction occurring is lower than the widely accepted probability by a factor of three. This finding significantly changes the final s-process abundances of some elements, such as Selenium, Krypton, Rubidium, Strontium, and Zirconium.

References

Jayatissa, H., et al. Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactionsPhysics Letters B 802, 135267 (2020). [DOI: 10.1016/j.physletb.2020.135267]

Ota, S. et al. Decay properties of 22Ne + α resonances and their impact on s-process nucleosynthesisPhysics Letters B 802, 135256 (2020). [DOI: 10.1016/j.physletb.2020.135256]

Funding

This research was supported by the Department of Energy (DOE) Office of Science, Office of Nuclear Physics; by the National Nuclear Security Administration through the Center for Excellence in Nuclear Training and University Based Research (CENTAUR); and the Nuclear Solutions Institute at Texas A&M University. Two of the authors were also supported by The Welch Foundation. Three of the authors were also supported by the U.K. Science and Technology Facilities Council.

Huge ring around a black hole

Credit: X-ray: NASA /


 CXC / U.Wisc-Madison / S.Heinz et al.; Optics / IR: PanSTARRS

This image features a magnificent set of rings around a black hole, captured using NASA’s Chandra X-ray Observatory and Neil Gerelswift Observatory. X-ray images of giant rings reveal information about dust in our galaxy, using principles similar to those used in clinics and airports.

Black holes are part of a star system called V404 Cygni at about 7,800. Light year Away from the earth. Black holes are actively attracting matter from a companion star, which weighs about half the mass of the Sun, to a disk around an invisible object. Astronomers call these systems “X-ray binaries” because this material glows with X-rays.

On June 5, 2015, Swift discovered an X-ray burst from the V404 Cygni. Burst created a high-energy ring from a phenomenon known as the light echo.Instead of the sound waves bouncing off the canyon wall, a light echo was generated around the V404 Cygni when a burst of X-rays from the black hole system bounced off. Dust Clouds between V404 Cygni and the Earth. Cosmic dust is not like household dust, it’s like smoke, it’s made up of small solid particles.

In this composite image, X-rays from Chandra (light blue) are combined with optical data from the PanSTARRS telescope in Hawaii, which shows the stars in the field of view. This image contains eight separate concentric rings. Each ring is created by X-rays from the V404 Cygni flare observed in 2015 and reflects off various dust clouds. (The artist’s illustration illustrates how the rings Chandra and Swift saw were created. To simplify the graphic, the illustration shows only four rings instead of eight.

A team of researchers led by Sebastian Heinz of the University of Wisconsin in Madison has conducted 50 Swift observations of the system between June 30 and August 25, 2015 and July 11-25, 2015. We analyzed the Chandra observations made in. Chandra’s operator intentionally placed the V404 Cygni between the detectors so that another bright burst would not damage the equipment.

The ring tells astronomers not only about the behavior of black holes, but also about the landscape between the V404 signi and the Earth. For example, the diameter of an X-ray ring reveals the distance to an intervening cloud of dust that bounces off light. When the clouds are close to the earth, the ring looks big and vice versa. Since the X-ray burst lasted for a relatively short time, the optical echo appears as a narrow ring rather than a wide ring or halo.

Researchers also used rings to examine the properties of the dust cloud itself. They compared the X-ray spectrum (that is, the brightness of X-rays over a range of wavelengths) with computer models of dust of various compositions. Different dust compositions absorb different amounts of low-energy X-rays and are undetectable by Chandra. This is a principle similar to how different parts of our body and luggage absorb different amounts of x-rays and provide information about their structure and composition.

The team determined that the dust was likely to contain a mixture of graphite and silicate particles. In addition, Chandra’s analysis of the inner ring revealed that the density of dust clouds was not uniform in all directions. Previous studies have assumed that this is not the case.

V404 Cygni: Huge ring around a black hole

This artist’s illustration details how the ring structure seen by Chandra and Swift is made. Each ring is caused by x-rays bouncing off various dust clouds. If the clouds are close to us, the ring will look big. The result is a set of concentric rings of different apparent sizes, depending on the distance of the intervening clouds from us. Credits: University of Wisconsin-Madison / S.Heinz school

A paper explaining the results of V404 Cygni was published in The Astrophysical Journal (preprint) published on July 1, 2016. The authors of this study are Sebastian Heinz, Lia Corrales (University of Michigan). Randall Smith (Center for Astrophysics | Harvard & Smithsonian); Niel Brandt (Penn State University); Peter Jonker (Netherlands Institute for Space Research); Richard Protokin (University of Nevada, Reno); and Joey Nielson (Villanova University).

This result is related to a similar discovery of the X-ray binary Circinus X-1, which contains neutron stars rather than black holes, in the June 20, 2015 issue of The Astrophysical Journal, “The Lord of the Rings: Kinematic Distance from Giant X-ray Light Echo to Circinus X-1” (preprint). The study was also led by Sebastian Heinz.

Several papers are published annually reporting the study of the 2015 V404 Cygni explosion that caused these rings. Earlier explosions were recorded in 1938, 1956, and 1989, so astronomers could still take years to continue analyzing the 2015 explosion.


Swift satellite reveals black hole bullseye


For more information:
S. Heinz et al., V404 Cygni’s 2015 X-ray Dust Scattering Echo Chandra and Swift Joint View, Astrophysical Journal (2016). DOI: 10.3847 / 0004-637X / 825/1/15 , arxiv.org/abs/1605.01648

Quote: V404 Cygni: https: //phys.org/news/2021-08-v404-cygni-huge-black-hole.html Black hole acquired on August 5, 2021 (August 5, 2021) Huge ring around

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Is the Universe a Roguelike? - What Up Science

Aug 6, 2021

IGN
Nobel Laureate Sir Roger Penrose just went to the mat for a cyclical model of the Universe. That means this has all happened before and it will all happen again, including you reading this description of this video. Neat! But is it true? We'll dig into that, trace the history of the cyclical concept of time, and make some spurious claims about whether we may or may not be living in a giant roguelike. It touches on games like Deathloop and 12 Minutes, shows like Rick and Morty and Futurama, and it's all wrapped up in a neat little science news package by your humble host Mr. Michael Swaim. #IGN #WhatUpScience

DOUBLING DOWN ON TROUBLE
Zero-carbon bitcoin? The owner of a Pennsylvania nuclear plant thinks it could strike gold

Talen Energy plans to build a $400 million bitcoin mine at its Pa. nuclear plant.

"I think this is a great opportunity to prolong the life of a lot of plants."

The Susquehanna Steam Electric Station near Berwick, Pa., is a two-unit nuclear reactor owned by Talen Energy. Talen announced the week of Aug. 1, 2021, that it plans to go into partnership with a cryptocurrency producer, TeraWulf Inc., to build a $400 million bitcoin mining operation at the Luzerne County plant that will be called Nautilus Cryptomine.
Talen Energy

by Andrew Maykuth
Published
Aug 6, 2021

Could bitcoin mining be the salvation of the embattled nuclear energy industry in America?

The owners of several nuclear power plants, including two in Pennsylvania, have formed ventures with cryptocurrency companies to provide the electricity needed to run computer centers that “mine” bitcoin. Since nuclear energy does not emit greenhouse gases, the project’s investors say, the zero-carbon bitcoin would address climate concerns that have tarnished the energy-intensive cryptocurrency industry.

Talen Energy, the owner of the Susquehanna Steam Electric Station near Berwick, Pa., announced this week that it has signed a deal with TeraWulf Inc., an Easton, Md. cryptocurrency mining firm, to build a giant bitcoin factory next to its twin reactors in northern Pennsylvania. The first phase of the venture, dubbed Nautilus Cryptomine, could cost up to $400 million.

Talen’s project could eventually use up to 300 megawatts — or 12% of Susquehanna’s 2,500 MW capacity. It’s the second bitcoin-mining venture in the last month that involves owners of Pennsylvania nuclear facilities.

Last month Energy Harbor Corp., the former power-generation subsidiary of First Energy Corp., announced it signed a five-year agreement to provide zero-carbon electricity to a new bitcoin mining center operated by Standard Power in Coshocton, Ohio. Energy Harbor owns two nuclear units in Ohio and the twin-unit Beaver Valley Power Station in Western Pennsylvania.

A nuclear fission start-up, Oklo, also announced last month it signed a 20-year deal with a bitcoin miner to supply it with power, though the company has not yet built a power plant.

In recent years, commercial nuclear operators have struggled to compete in competitive electricity markets against natural gas plants and upstart renewable sources such as wind and solar. Unfavorable market conditions have hastened the retirements of several single-unit reactors, such as Three Mile Island Unit 1 in Pennsylvania. Lawmakers in New Jersey, New York and Illinois have enacted nuclear bailouts, paid by electricity customers, to stave off early retirement for other plants.

The cryptocurrency deals would provide nuclear generators with reliable outlets for their power, and bitcoin miners with predictable sources of power at cheap prices, along with a zero-carbon cachet.
Photo illustration showing the Susquehanna Steam Electric Station near Berwick, Pa., a two-unit nuclear reactor owned by Talen Energy (formerly owned by PPL Corp.), and a proposed 200,000 square-foot Talen Energy

“Nuclear energy is uniquely positioned to provide power to crypto mining companies and other major energy users who have committed to a carbon-free future,” John Kotek, senior vice president of policy development and government affairs at Nuclear Energy Institute, said in an email.

The nuclear industry views the crypto craze not as a crutch but as a launching pad for expansion. “U.S. nuclear power plants are ready and able to supply miners with abundant, reliable carbon-free power while also providing new business pathways for the nuclear developers and utilities, increasing their operating profits, and potentially accelerating the deployment of the next generation of reactors,” Kotek said.


Nuclear producers aren’t the only power generators getting in on the trend. Stronghold Digital Mining, a bitcoin miner that registered last month for a $100 million initial stock offering, plans to build its bitcoin mining operation in northwestern Pennsylvania, powered from Venango County waste coal. While its bitcoin would not be zero-carbon, it would reduce environmentally harmful piles of waste coal.

Energy and cryptocurrency experts say several trends are shifting the market in favor of U.S. nuclear power producers.

In May, Chinese regulators announced new measures to limit bitcoin mining in several regions that failed to meet Beijing’s energy-use targets. Bitcoin production levels have fallen since then, forcing bitcoin producers to relocate to places with low operating costs and cool climates to reduce the costs of cooling the bitcoin data centers. The state of Washington, which has lots of inexpensive hydroelectric power, has undergone a huge boom in bitcoin mining.

How mining is done

Bitcoin is a peer-to-peer virtual currency, operating without a central authority, and which can be exchanged for traditional currency such as the U.S. dollar. It is the most successful of hundreds of attempts to create virtual money through the use of cryptography, the science of making and breaking codes — hence, they are called cryptocurrency.

Bitcoin mining is built around blockchain technology, and it involves generating a string of code that decrypts a collection of previously executed bitcoin transactions. Successful decryption is rewarded with a new bitcoin. The supply of bitcoins is limited to 21 million — nearly 90% have already been mined. So the remaining bitcoins become increasingly scarce and more difficult to extract.

Data centers operated by bitcoin miners randomly generate code strings, called “hashes,” to solve the puzzle and earn new coins. Worldwide, miners on the bitcoin network generate more than 100 quintillion hashes per second — that’s 100,000,000,000,000,000,000 guesses per second, according to Blockchain.com. The first phase of the Nautilus project in Pennsylvania would generate five quintillion hashes per second.

Such guesswork requires muscular computing power, robust internet connections, and lots of electricity. Smaller bitcoin miners have teamed up in consortiums to pool their computing power. Bigger players have built huge data centers devoted exclusively to producing lines of random code.
An electrician checks cryptocurrency computer mining rigs in Hennepin, Ill., where Sangha Systems is converting the bitcoin mining facility to solar power to address growing concerns about the industry's carbon footprint. The owner of a Pennsylvania nuclear power plant announced that it would form a partnership with a cryptocurrency mining operation to produce and market "zero carbon" bitcoin produced from nuclear energy.
Antonio Perez / MCT

“Mining cryptocurrency is an international, profitable, and energy-intensive business,” ScottMadden a management consulting firm, said in a paper it published last year. Bitcoin mining consumes an estimated 0.5% of the electricity produced worldwide or about as much as the country of Greece.

Some lawmakers have called for greater regulation of cryptocurrency, citing the enormous amount of resources required to produce it. “There are computers all over the world right now spitting out random numbers around the clock, in a competition to try to solve a useless puzzle and win the bitcoin reward,” Sen. Elizabeth Warren (D., Mass.) said in June, calling for a crackdown on “environmentally wasteful cryptocurrencies.”

Why possible numbers look good


But as a business proposition, bitcoin has appeal. ScottMadden, the consulting firm, suggested last year that nuclear operators in some states were in a unique position to profit from cryptocurrency ventures.

Diverting 1 megawatt of power to an efficient mining operation could conservatively generate top-line revenue of $900,000 a year and profits of $650,000, not accounting for cooling, repairs, or technicians, according to ScottMadden. Its analysis predicts that a project could break even in about 15 months.

The consulting firm’s conceptual project was based upon a bitcoin price of $9,275. The price of a bitcoin last week varied between $38,000 and $42,000.

Such numbers no doubt got the attention of Talen Energy, which plans to divert about 180 MW to the first phase of the Nautilus Cryptomine, which would be producing bitcoin at the Susquehanna plant in Luzerne County.

”I think it’s a great opportunity for our plant,” said Dustin Wertheimer, vice president and divisional chief financial officer of Talen Energy. He is based in Allentown, home to Talen’s previous owner, PPL Corp. Talen is now based in the Woodlands, Texas.

Unlike other crypto projects in which the power generator is an arms-length electricity supplier, the Nautilus Cryptomine is a 50-50 venture between Talen and TeraWulf. The project would be directly connected to the Susquehanna plant — “behind the meter,” in industry parlance — and would avoid any transmission costs from the grid.
Bitcoin tokens. The price of a bitcoin traded for about $40,000 last week.
Dan Kitwood / MCT

The direct connection also guarantees that the operation is sourced exclusively with carbon-free energy, Wertheimer said.

“You’ve seen some of the press and the negative publicity that bitcoin has received recently and the impact of fossil fuel,” Wertheimer said. “So that’s a great thing for us to have a direct connection into a carbon-free power source.”

The cryptomine would be located inside a 200,000-square-foot building — about four football fields. The mining operation would be built on a data center campus that Talen is developing next to the Susquehanna plant. The data center would generate about 1,000 construction jobs, Wertheimer said. The cryptomine would employ about 50 people to operate.

The first phase of the project would cost about $350 million to $400 million. The Nautilus venture is negotiating with fiber-optic providers to bring in super-charged internet connections required to transmit and receive the huge amounts of code it generates, Wertheimer said.

“As you look across the United States, and you look at kind of the challenges that are facing nuclear plants, I think this is a great opportunity to prolong the life of a lot of plants,” he said.



The Inquirer explores what work will look like in the pandemic and beyond.
The Future of Work is produced with support from the William Penn Foundation and the Lenfest Institute for Journalism. Editorial content is created independently of the project’s donors.

Published
Aug. 6, 2021

Andrew Maykuth
I cover how we produce and use energy, as well as its impact on the economy and the environment.
China Says It's Closing in on Thorium Nuclear Reactor

With prototype reportedly firing up in September, country teases commercial thorium power by 2030

PRACHI PATEL
04 AUG 2021



Thorium on the periodic table of elements.
KLAUDIA KILMAN/ALAMY


There is no denying the need for nuclear power in a world that hungers for clean, carbon-free energy. At the same time, there's a need for safer technologies that bear less proliferation risk. Molten salt nuclear reactors (MSRs) fit the bill—and, according to at least one source, China may be well on their way to developing MSR technology.

Government researchers there unveiled a design for a commercial molten salt reactor (MSR) that uses thorium as fuel, the South China Morning Post reported recently. A prototype reactor, the paper said, should be ready this month for tests starting in September. Construction of the first commercial reactor being built in the Gansu province should be complete, they noted, by 2030.

If all goes well with the prototype, says a report in Live Science, the Chinese government plans to build several large MSRs. According to the World Nuclear Association, the country is eyeing thorium MSRs as a source of energy especially for the northwestern portion of the country, which has lower population density and an arid climate.

MSRs are attractive for arid regions because instead of the water used by conventional uranium reactors, MSRs use molten fluoride salts to cool their cores. Uranium or thorium fuel can be mixed into the coolant salt. Thorium MSRs have the advantage of being more abundant and cheaper.

China's experimental reactor won't be the world's first. Researchers at Oak Ridge National Laboratory (ORNL) pioneered thorium-based MSRs in the 1950s for nuclear aircraft propulsion as part of the Manhattan Project. A 7.4 MWth experimental reactor operated at the laboratory over a period of four years—although only a portion of its fuel was derived from uranium-233 bred from thorium in other reactors. This MSR technology was eventually shelved because the Pentagon favored the uranium fast breeder reactor, says Charles Forsberg, Principal Research Scientist at MIT's department of Nuclear Science and Engineering and former nuclear researcher at ORNL.

Scientists in China are now building on the same basic MSR technology developed at ORNL. The Chinese government had a small, short-lived knowledge exchange program with ORNL. But most of the thorium reactor-related intellectual property from ORNL is in the public domain, and China appears to have made some use of it. "The real data mine is the thousands of published reports in 1960s and '70s that are found in the open literature," Forsberg says.

Plus, recent technology developments have made it more feasible to build MSRs, he adds. This includes modern instrumentation that can unveil exactly what goes on in the reactor—but also includes equipment that finds parallel use, such as high-temperature salt pumps used in today's concentrated solar power plants that store heat via molten salts.

The real data mine is the thousands of published reports in 1960s and '70s that are found in the open literature.

"So now if you want to build a salt pump for a MSR you go talk to your local friendly CSP pump suppliers for a slightly different salt composition," Forsberg says. "That makes a tremendous difference in your development program. You have fifty years' worth of new technology to tap into."

But even though France, India, Japan, Norway, and the U.S. are all reportedly working on thorium nuclear reactors, none of these countries have outlined plans for commercial reactors yet. A handful of private sector developers are working hard to deploy MSRs within the next decade. The closest is probably Alameda, Calif.-based Kairos Power, which plans to have a 50 MW demonstration reactor operational in Oak Ridge, Tenn. by 2026.

Yet China leads global MSR research, according to the World Nuclear Association, and it's no surprise that the country is forging ahead faster, Forsberg says. The country's talent pool in nuclear engineering, he says, is quite substantial. "You put a lot of talented people on a project, and it works," he says. "They'll be successful even if it takes them a while."


Prachi Patel
is a freelance journalist based in Pittsburgh. She writes about energy, biotechnology, materials science, nanotechnology, and computing.


 

China Starts Constructing $17-Billion Nuclear Power Plant



China started this week construction work on a new US$17-billion nuclear power plant project, for which it will install Russian nuclear reactors at the Xudabao project in northeastern China, World Nuclear News reports.

The Xudabao 3 unit is the first of four units at the plant to see the beginning of construction. Russia’s Rosatom will design the nuclear island and will provide equipment. The Russian firm will also provide commissioning services for the equipment it will have supplied. The Russians will also provide the construction and equipment for the Xudabao 4 unit, whose construction is expected to begin in 2022.

The two units are currently expected to be commissioned in 2027 or 2028.

Construction for the Xudabao units 1 and 2 has yet to begin, according to World Nuclear News.

Last month, China had to close down a nuclear power plant in the province of Guangdong in the south because it was damaged. The operator, however, insisted that the Taishan nuclear plant does not have any major safety issue.  

A month before that, French company Framatome, a subsidiary of French energy giant EDF, issued a statement related to Taishan’s reactor number 1, saying that it “is supporting resolution of a performance issue with the Taishan Nuclear Power Plant.”

The Taishan nuclear plant could turn into an “imminent radiological threat,” the part owner of the facility, the French company has told the United States, CNN reported in the middle of June, citing U.S. officials and a letter of the French firm it had obtained.

A week before the Chinese operator of the plant announced it would shut down for maintenance, France’s EDF, which holds 30 percent in the TNPJVC joint venture operating Taishan, had said in a statement that it would have shut the plant if it were in France.

“EDF's operating procedures for the French nuclear fleet would lead EDF, in France, to shut down the reactor in order to accurately assess the situation in progress and stop its development. In Taishan, the corresponding decisions belong to TNPJVC,” the French company said.

By Tsvetana Paraskova for Oilprice.com