Tag Archives: radiation

Cosmic radiation during spaceflight could increase risk of erectile dysfunction in astronauts – Space.com

  1. Cosmic radiation during spaceflight could increase risk of erectile dysfunction in astronauts Space.com
  2. Astronauts may suffer from erectile dysfunction after trips to space, study finds Yahoo! Voices
  3. Cosmic-ray exposure on space missions could cause erectile dysfunction, liquid channels in ice boost frost damage – Physics World physicsworld.com
  4. Erectile Dysfunction a Side-Effect Future Space Travellers Must Brace For, Study Finds! | Weather.com The Weather Channel
  5. Scientists Have Bad News for Astronauts’ Genitals Yahoo! Voices
  6. View Full Coverage on Google News

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Mysterious radiation bursts could be coming from ‘starquakes’ on neutron stars – Space.com

  1. Mysterious radiation bursts could be coming from ‘starquakes’ on neutron stars Space.com
  2. Source of ‘alien’ radio signals may have been discovered by scientists studying the pulses that travel at the Daily Mail
  3. Fast radio bursts from distant neutron stars resemble earthquakes rather than solar flares Phys.org
  4. Mysterious Energy Bursts From Deep Space Have Baffled Scientists For Years. “Starquakes” Could Be the Solution. The Debrief
  5. Mysterious fast radio bursts might be caused by “starquakes,” study finds Ars Technica
  6. View Full Coverage on Google News

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UV radiation pulse played a role in a mass extinction event, fossilized pollen reveals

A lethal pulse of ultraviolet (UV) radiation may have played a role in Earth’s biggest mass extinction event, fossilized pollen grains reveal. 

Pollen that dates to the time of the Permian-Triassic mass extinction event, roughly 250 million years ago, produced “sunscreen” compounds that shielded against harmful UV-B radiation, the analysis found. At that time, approximately 80% of all marine and terrestrial species died off. 

For the study, which was published Jan. 6 in the journal Science Advances (opens in new tab), a team of international scientists developed a new method of using a laser beam to examine the miniscule grains, which measure about half the width of a human hair and were found embedded onto rocks unearthed in southern Tibet, according to a statement.

Plants rely on photosynthesis to convert sunlight into energy, but they also need a mechanism to block out harmful UV-B radiation.

“As UV-B is bad for us, it’s equally as bad for plants,” Barry Lomax (opens in new tab), the study’s co-author and a professor in plant paleobiology at the University of Nottingham in the U.K., told Live Science. “Instead of going to [the pharmacy], plants can alter their chemistry and make their own equivalent version of sunscreen compounds. Their chemical structure acts to dissipate the high-energy wavelengths of UV-B light and stops it from getting within the preserved tissues of the pollen grains.”

Related: 3.5 billion-year-old rock structures are one of the oldest signs of life on Earth

In this case, the radiation spike didn’t “kill the plants outright, but rather it slowed them down by lessening their ability to photosynthesize, which caused them to become sterile over time,” Lomax said. “You then wind up with extinction driven by a lack of sexual reproduction rather than the UV-B frying the plants instantly.”

Experts have long theorized that the Permian-Triassic extinction, classified as one of the five major extinction events on Earth, was in response to a “paleoclimate emergency” caused by the Siberian Traps eruption, a large volcanic event in what is now modern-day Siberia. The catastrophic incident forced plumes of carbon buried deep within the Earth’s interior up into the stratosphere, resulting in a global warming event that “led to a collapse in the Earth’s ozone layer,” according to the researchers. 

The pollen grain used in the work. It measures about half the width of a human hair. (Image credit: Liu Feng/Nanjing Institute of Geology and Paleontology )

“And when you thin out the ozone layer, that’s when you end up with more UV-Bs,” Lomax said.

In their research, the scientists also discovered a link between the burst of UV-B radiation and how it changed the chemistry of plants’ tissues, which led to “a loss of insect diversity,” Lomax said.

“In this case, plant tissues became less palatable to herbivores and less digestible,” Lomax said. 

Because plant leaves had less nitrogen, they were not nutritious enough for the insects that ate them. That may explain why insect populations plummeted during this extinction event.

“Often insects come out unscathed during mass extinction events, but that wasn’t the case here,” Lomax said. 

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NASA Earth Radiation Budget Satellite To Reenter Atmosphere Today

NASA’s Earth Radiation Budget Satellite is expected to burn up in the atmosphere. Here we see the ATV Jules Verne spacecraft on destructive reentry in 2008 taken from the DC-8 aircraft which observed the reentry over the Pacific Ocean. Credit: ESA

In early January

NASA expects most of the satellite to burn up as it travels through the atmosphere, but some components are expected to survive the reentry. The risk of harm coming to anyone on Earth is very low – approximately 1 in 9,400. 

NASA’s Earth Radiation Budget Satellite (ERBS) was designed to examine how energy from the Sun is absorbed and re-emitted by the Earth. By understanding this process, researchers can learn more about patterns in Earth’s weather. ERBS was launched on October 5, 1984, on the Space Shuttle Challenger and retired on October 14, 2005, making it one of the longest-running spacecraft missions. Although the spacecraft was only expected to operate for two years, it actually provided scientists with data on the Earth’s ozone layer for over 20 years. Credit: NASA

Launched from the Space Shuttle Challenger on October 5, 1984, the ERBS spacecraft was part of NASA’s three-satellite Earth Radiation Budget Experiment (ERBE) mission. It carried three instruments, two to measure the Earth’s radiative energy budget, and one to measure stratospheric constituents, including ozone.  

The energy budget, the balance between the amount of energy from the Sun that Earth absorbs or radiates, is an important indicator of climate health, and understanding it can also help reveal weather patterns. Ozone concentrations in the stratosphere play an important role in protecting life on Earth from damaging ultraviolet radiation. 

ERBS far exceeded its expected two-year service life, operating until its retirement in 2005. Its observations helped researchers measure the effects of human activities on Earth’s radiation balance. NASA has continued to build on the success of the ERBE mission with projects including the current Clouds and the Earth’s Radiant Energy System (CERES) suite of satellite instruments.  

The Stratospheric Aerosol and Gas Experiment II (SAGE II) on the ERBS made stratospheric measurements. SAGE II collected important data that confirmed the ozone layer was declining on a global scale. That data helped shape the international Montreal Protocol Agreement, resulting in a dramatic decrease around the globe in the use of ozone-destroying chlorofluorocarbons. Today, SAGE III on the International Space Station collects data on the health of the ozone layer. 



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We now know why black hole jets make high-energy radiation

Enlarge / The jets of material ejected from around black holes can be enormous.

Active galactic nuclei, powered by the supermassive black holes they contain, are the brightest objects in the Universe. The light originates from jets of material hurled out at nearly the speed of light by the environment around the black hole. In most cases, these active galactic nuclei are called quasars. But, in rare instances where one of the jets is oriented directly toward Earth, they’re called a blazar and appear brighter.

While the general outline of how a blazar operates has been worked out, several details remain poorly understood, including how the fast-moving material generates so much light. Now, researchers have turned a new space-based observatory called the Imaging X-ray Polarimetry Explorer (IXPE) toward one of the brightest blazars in the sky. The data from it and other observations combined indicate that light is produced when the black hole jets slam into slower-moving materials.

Jets and light

The IXPE specializes in detecting the polarization of high-energy photons—the orientation of the wiggles in the light’s electric field. Polarization information can tell us something about the processes that created the photons. For example, photons that originate in a turbulent environment will have an essentially random polarization, while a more structured environment will tend to produce photons with a limited range of polarizations. Light that passes through material or magnetic fields can also have its polarization altered.

This turns out to be useful for studying blazars. The high-energy photons these objects emit are generated by charged particles in the jets. When these objects change course or decelerate, they have to give up energy in the form of photons. Since they’re moving at close to the speed of light, they have a lot of energy to give up, allowing blazars to emit across the entire spectrum from radio waves to gamma rays—some of the latter remaining at those energies despite billions of years of redshifting.

So, the question then becomes what causes these particles to decelerate. There are two leading ideas. One of those is that the environment in the jets is turbulent, with chaotic pile-ups of materials and magnetic fields. This decelerates the particles, and the messy environment would mean that the polarization becomes largely randomized.

The alternative idea involves a shockwave, where material from the jets slams into slower-moving material, and decelerates itself. This is a relatively orderly process, and it produces a polarization that’s relatively limited in range and gets more pronounced at higher energies.

Enter IXPE

The new set of observations is a coordinated campaign to record the blazar Markarian 501 using a variety of telescopes capturing polarization at longer wavelengths, with IXPE handling the highest energy photons. In addition, the researchers searched the archives of several observatories to obtain earlier observations of Markarian 501, allowing them to determine if the polarization is stable over time.

Overall, across the entire spectrum from radio waves to gamma rays, the measured polarizations were within a few degrees of each other. It was also stable over time, and its alignment increased at higher photon energies.

There’s still a bit of variation in the polarization, which suggests there’s some relatively minor disorder at the site of the collision, which isn’t really a surprise. But it’s far less disordered than you’d expect from a turbulent material with complicated magnetic fields.

While these results provide a better understanding of how black holes produce light, that process ultimately relies on the production of jets, which takes place much closer to the black hole. How these jets form is still not really understood, so people studying black hole astrophysics still have a reason to go back to work after the holiday weekend.

Nature, 2022. DOI: 10.1038/s41586-022-05338-0  (About DOIs).

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Tree Rings Offer Insight Into Mysterious, Devastating Radiation Storms

A composite image showing a tree ring and flames – UQ researchers used tree ring data to model the global carbon cycle to challenge the common theory about Miyake Events. Credit: The University of Queensland

New light has been shed on a mysterious, unpredictable, and potentially devastating kind of astrophysical event, thanks to a University of Queensland (UQ) study.

A team of researchers, led by Dr. Benjamin Pope from UQ’s School of Mathematics and Physics, applied cutting-edge statistics to data from millennia-old trees, to find out more about radiation ‘storms’.

“These huge bursts of cosmic radiation, known as Miyake Events, have occurred approximately once every thousand years but what causes them is unclear,” Dr. Pope said.

“The leading theory is that they are huge solar flares. We need to know more, because if one of these happened today, it would destroy technology including satellites, internet cables, long-distance power lines, and transformers.

“The effect on global infrastructure would be unimaginable.”

“Rather than a single instantaneous explosion or flare, what we may be looking at is a kind of astrophysical ‘storm’ or outburst.” — Qingyuan Zhang

Enter the humble tree ring.

First author Qingyuan Zhang, a UQ undergraduate mathematics student, developed software to analyze every available piece of data on tree rings.

“Because you can count a tree’s rings to identify its age, you can also observe historical cosmic events going back thousands of years,” Mr Zhang said.

“When radiation strikes the atmosphere it produces radioactive carbon-14, which filters through the air, oceans, plants, and animals, and produces an annual record of radiation in tree rings.

“We modeled the global carbon cycle to reconstruct the process over a 10,000-year period, to gain insight into the scale and nature of the Miyake Events.”

The common theory until now has been that Miyake Events are giant solar flares.

“But our results challenge this,” Mr. Zhang said. “We’ve shown they’re not correlated with sunspot activity, and some actually last one or two years.

“Rather than a single instantaneous explosion or flare, what we may be looking at is a kind of astrophysical ‘storm’ or outburst.”

“The effect on global infrastructure would be unimaginable.” — Dr. Benjamin Pope

Dr. Pope said the fact scientists don’t know exactly what Miyake Events are, or how to predict their occurrence is very disturbing.

“Based on available data, there’s roughly a one percent chance of seeing another one within the next decade. But we don’t know how to predict it or what harms it may cause.

“These odds are quite alarming, and lay the foundation for further research.”

The research is published in Proceedings of the Royal Society A.

Reference: “Modelling cosmic radiation events in the tree-ring radiocarbon record” by Qingyuan Zhang, Utkarsh Sharma, Jordan A. Dennis, Andrea Scifo, Margot Kuitems, Ulf Büntgen, Mathew J. Owens, Michael W. Dee and Benjamin J. S. Pope , Proceedings of the Royal Society A Mathematical Physical and Engineering Sciences.
DOI: 10.1098/rspa.2022.0497

The study was also completed with undergraduate maths and physics students Utkarsh Sharma and Jordan Dennis.

The work was supported by a philanthropic donation to UQ from the Big Questions Institut.



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Gigantic radiation storms have been pummeling Earth for at least 10,000 years and could strike again, tree ring analysis reveals

A series of sudden and colossal spikes in radiation levels across Earth’s history could have come from a series of unknown, unpredictable and potentially catastrophic cosmic events, a new study has revealed. 

Named Miyake events after the lead author of the first study to describe them, the spikes occur roughly once every 1,000 years or so and are recorded as sudden increases in the radiocarbon levels of ancient tree rings.

The exact cause of the sudden deluges of radiation, which periodically transform an extra chunk of the atmosphere’s nitrogen into carbon sucked up by trees, remains unknown. The leading theory among scientists is that Miyake events are solar flares that are 80 times more powerful than the strongest flare ever recorded. But a new study, published Oct. 26 in the journal Proceedings of the Royal Society A: Mathematical, Physical, and Engineering Sciences, suggests that the origin of the radiation bursts could be even more mysterious than first thought.

Related: Strange new type of solar wave defies physics

“These huge bursts of cosmic radiation, known as Miyake Events, have occurred approximately once every thousand years but what causes them is unclear,” lead author Benjamin Pope, an astrophysicist at the University of Queensland, Australia, said in a statement. “We need to know more, because if one of these happened today, it would destroy technology including satellites, internet cables, long-distance power lines and transformers. The effect on global infrastructure would be unimaginable.”

Each year, temperate tree species develop a new concentric ring around their trunks that, added up, indicates their age. Because trees suck up carbon from the atmosphere, scientists can study the amount of radiation in the atmosphere during Earth’s recent history by measuring tree rings for quantities of the radioactive isotope carbon-14 — produced when energetic cosmic rays collide with atmospheric nitrogen.

Scientists have spotted six Miyake events in tree rings so far, indicated by sudden, single-year leaps in the concentrations of carbon-14 and other isotopes; these occurred in the years 7176 B.C., 5410 B.C., 5259 B.C., 660 B.C., A.D. 774 and A.D. 993; alongside a number of other, smaller events spotted at other times.

To investigate if the sudden carbon-14 spikes were caused by incredibly powerful solar flares, the researchers created a simplified model of the global carbon cycle; inputting the tree ring data to demonstrate how carbon was produced by solar radiation and absorbed into Earth’s atmosphere, oceans, land and organisms. By comparing their timeline of atmospheric carbon with the known 11-year solar cycle, the researchers expected to find that the years of the Miyake events corresponded to moments of peak solar activity.

But instead they discovered that the Miyake events did not line up with peak solar activity, and some of the events, unlike the brief flashes we recognize as solar flares, lasted for one or two years.

“Rather than a single, instantaneous explosion or flare, what we may be looking at is a kind of astrophysical ‘storm’ or outburst,” first author Qingyuan Zhang, a mathematician  at the University of Queensland, said in the statement. 

The intensity of these unexplained cosmic barrages is hard to understate. The largest solar storm ever recorded is the 1859 Carrington Event, which, after slamming into Earth, sent powerful streams of solar particles that fried telegraph systems all over the world and caused auroras brighter than the light of the full moon to appear as far south as the Caribbean. The storm released roughly the same energy as 10 billion 1-megaton atomic bombs. If an equally powerful flare were to hit Earth now, it would cause an ‘internet apocalypse,’ blackouts, and trillions of dollars’ worth of damage, according to scientists. But the Carrington Event was 80 times less powerful than the A.D. 774 Miyake event.

Having cast doubt on the spikes coming from conventionally understood solar flares, the researchers considered whether the Miyake events were generated by supernovas or a type of solar superflare. But these alternate theories have holes too: Supernovas sometimes produce radiocarbon spikes in Earth’s atmosphere, but sometimes they don’t; and stars like ours are not known to produce solar flares energetic enough to cause the Miyake events. Evidence for a solar superflare is also missing in recovered ice core nitrate records for the events in A.D. 774 AD and A.D. 993.

Venturing into the historical records brought up only two tantalizing references. One made in the Anglo-Saxon Chronicle (a ninth century collection of annals recounting Anglo-Saxon history) refers to a possible aurora in the form of a “red crucifix, after sunset” being spotted in the sky in A.D. 774, but the researchers think it may also have been an optical illusion known as a moon ring. Another account, made in A.D. 775 in the Chinese chronicle Jiutangshu, describes what also could have been an aurora, but its existence is so far not backed up by other records.

The researchers’ next step is to gather more tree ring and ice core data to further pin down the timing of the events and the mixtures of isotopes produced by them. But the scientists’ uncertainty as to what the events are, or how to predict when they occur, is “very disturbing,” Pope said.

“Based on available data, there’s roughly a one percent chance of seeing another one within the next decade. But we don’t know how to predict it or what harms it may cause,” Pope added. “These odds are quite alarming, and lay the foundation for further research.”

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Tree rings reveal devastating radiation storms – HeritageDaily

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Tree rings offer insight into devastating radiation storms

A composite image showing a tree ring and flames – UQ researchers used tree ring data to model the global carbon cycle to challenge the common theory about Miyake Events. Credit: The University of Queensland

A University of Queensland study has shed new light on a mysterious, unpredictable and potentially devastating kind of astrophysical event.

A team led by Dr. Benjamin Pope from UQ’s School of Mathematics and Physics applied cutting edge statistics to data from millennia-old trees, to find out more about radiation “storms.”

“These huge bursts of cosmic radiation, known as Miyake Events, have occurred approximately once every thousand years, but what causes them is unclear,” Dr. Pope said.

“The leading theory is that they are huge solar flares. We need to know more, because if one of these happened today, it would destroy technology including satellites, internet cables, long-distance power lines and transformers. The effect on global infrastructure would be unimaginable.”

Enter the humble tree ring.

First author Qingyuan Zhang, a UQ undergraduate math student, developed software to analyze every available piece of data on tree rings.

“Because you can count a tree’s rings to identify its age, you can also observe historical cosmic events going back thousands of years,” Mr. Zhang said. “When radiation strikes the atmosphere, it produces radioactive carbon-14, which filters through the air, oceans, plants, and animals, and produces an annual record of radiation in tree rings. We modeled the global carbon cycle to reconstruct the process over a 10,000-year period, to gain insight into the scale and nature of the Miyake Events.”

The common theory until now has been that Miyake Events are giant solar flares.

“But our results challenge this,” Mr. Zhang said. “We’ve shown they’re not correlated with sunspot activity, and some actually last one or two years. Rather than a single instantaneous explosion or flare, what we may be looking at is a kind of astrophysical ‘storm’ or outburst.”

Dr. Pope said the fact scientists don’t know exactly what Miyake Events are, or how to predict their occurrence, is very disturbing.

“Based on available data, there’s roughly a one percent chance of seeing another one within the next decade. But we don’t know how to predict it or what harms it may cause. These odds are quite alarming, and lay the foundation for further research,” he concluded.

The research is published in Proceedings of the Royal Society A, and was completed with help from undergraduate math and physics students Utkarsh Sharma and Jordan Dennis.


Analysis of tree rings reveals highly abnormal solar activity in the mid-holocene


More information:
Modelling Cosmic Radiation Events in the Tree-ring Radiocarbon Record, Proceedings of the Royal Society A: Mathematical and Physical Sciences (2022). DOI: 10.1098/rspa.2022.0497. royalsocietypublishing.org/doi … .1098/rspa.2022.0497
Provided by
University of Queensland

Citation:
Tree rings offer insight into devastating radiation storms (2022, October 25)
retrieved 26 October 2022
from https://phys.org/news/2022-10-tree-insight-devastating-storms.html

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Strange Long-Lasting Pulse of High-Energy Radiation Swept Over Earth

Astronomers think GRB 221009A represents the birth of a new black hole formed within the heart of a collapsing star. In this illustration, the black hole drives powerful jets of particles traveling near the speed of light. The jets pierce through the star, emitting X-rays and gamma rays as they stream into space. Credit: NASA/Swift/Cruz deWilde

NASA’s Swift and Fermi Missions Detect Exceptional Cosmic Blast

An unusually bright and long-lasting pulse of high-energy radiation swept over Earth Sunday, October 9, captivating astronomers around the world. The intense emission came from a gamma-ray burst (GRB) – the most powerful class of explosions in the universe – that ranks among the most luminous events known.

A week ago, on Sunday morning Eastern time, a wave of X-rays and gamma rays passed through the solar system. It triggered detectors aboard

Swift’s X-Ray Telescope captured the afterglow of GRB 221009A about an hour after it was first detected. The bright rings form as a result of X-rays scattered from otherwise unobservable dust layers within our galaxy that lie in the direction of the burst. Credit: Credit: NASA/Swift/A. Beardmore (University of Leicester)

Called GRB 221009A, the explosion provided an unexpectedly exciting start to the 10th Fermi Symposium, a gathering of gamma-ray astronomers now underway in Johannesburg, South Africa. “It’s safe to say this meeting really kicked off with a bang – everyone’s talking about this,” said Judy Racusin, a Fermi deputy project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, who is attending the conference.


Astronomers think GRB 221009A represents the birth of a new

Originating from the direction of the constellation Sagitta, the signal traveled an estimated 1.9 billion years to reach Earth. Many astronomers believe it represents the birth cry of a new black hole, one that formed in the heart of a massive star collapsing under its own weight. In these circumstances, a developing black hole drives powerful jets of particles traveling near the speed of light. The energetic jets pierce through the star, emitting X-rays and gamma rays as they stream into space.

This sequence constructed from Fermi Large Area Telescope data reveals the sky in gamma rays centered on the location of GRB 221009A. Each frame shows gamma rays with energies greater than 100 million electron volts (MeV), where brighter colors indicate a stronger gamma-ray signal. In total, they represent more than 10 hours of observations. The glow from the midplane of our Milky Way galaxy appears as a wide diagonal band. The image is about 20 degrees across. Credit: NASA/DOE/Fermi LAT Collaboration

The burst also provided a long-awaited inaugural observing opportunity for a link between two experiments on the International Space Station (ISS) – NASA’s NICER X-ray telescope and a Japanese detector called the Monitor of All-sky X-ray Image (MAXI). Activated in April, the connection is dubbed the Orbiting High-energy Monitor Alert Network (OHMAN). It allows NICER to rapidly turn to outbursts detected by MAXI, actions that previously required intervention by scientists on the ground.

“OHMAN provided an automated alert that enabled NICER to follow up within three hours, as soon as the source became visible to the telescope,” said Zaven Arzoumanian, the NICER science lead at Goddard. “Future opportunities could result in response times of a few minutes.”

Images taken in visible light by Swift’s Ultraviolet/Optical Telescope show how the afterglow of GRB 221009A (circled) faded over the course of about 10 hours. The explosion appeared in the constellation Sagitta and occurred 1.9 billion years ago. The image is about 4 arcminutes across. Credit: NASA/Swift/B. Cenko

The light from this ancient explosion brings with it valuable new insights into stellar collapse, the birth of a black hole, the behavior and interaction of matter near the speed of light, the conditions in a distant galaxy – and much more. Astronomers may not detect another GRB this bright for decades.

Fermi’s Large Area Telescope (LAT) detected the burst for more than 10 hours, according to a preliminary analysis. One reason for the burst’s exceptional brightness and longevity is that, for a GRB, it lies relatively close to us.

“This burst is much closer than typical GRBs, which is exciting because it allows us to detect many details that otherwise would be too faint to see,” said Roberta Pillera, a Fermi LAT Collaboration member who led initial communications about the burst and a doctoral student at the Polytechnic University of Bari, Italy. “But it’s also among the most energetic and luminous bursts ever seen regardless of distance, making it doubly exciting.”



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