Tag Archives: exploding

Obesity is ‘exploding,’ with more than 12% of people classified as obese worldwide, study finds: ‘Big trouble’ – New York Post

  1. Obesity is ‘exploding,’ with more than 12% of people classified as obese worldwide, study finds: ‘Big trouble’ New York Post
  2. Worldwide trends in underweight and obesity from 1990 to 2022: a pooled analysis of 3663 population-representative studies with 222 million children, adolescents, and adults The Lancet
  3. Obesity has become the most common form of malnutrition in the majority of countries EL PAÍS USA
  4. More than a billion people worldwide are obese, WHO study finds Reuters
  5. More than 1 billion people worldwide are now estimated to have obesity Science News Magazine

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Stephen Colbert’s Crowd Goes Wild For His Wife Over Her Role In Exploding Appendix Story – HuffPost

  1. Stephen Colbert’s Crowd Goes Wild For His Wife Over Her Role In Exploding Appendix Story HuffPost
  2. Stephen Colbert returns after health scare, plus George Clooney, Mark Wahlberg and Dua Lipa show up during a star-studded night for the late shows Yahoo Entertainment
  3. Stephen Colbert Details Hospitalization, Recovery for Ruptured Appendix: “I Was Not Aware of the Amount of Trouble I Was In” Hollywood Reporter
  4. Is The Late Show with Stephen Colbert new tonight, December 11? Last Night On
  5. Stephen Colbert Returns to ‘Late Show’ Following Ruptured Appendix TheWrap

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‘Grandfather’ who shot down a Russian exploding drone with his Kalashnikov rifle receives bravery medal, says Ukraine military – Yahoo News

  1. ‘Grandfather’ who shot down a Russian exploding drone with his Kalashnikov rifle receives bravery medal, says Ukraine military Yahoo News
  2. Video shows Russians appearing to flee Ukrainian attack near Bakhmut CNN
  3. Ukraine releases special forces helmet-camera footage from battle for Bakhmut Euronews
  4. Russian forces eliminate over 1600 Ukrainian troops in 24 hours with heavy assault on frontline Hindustan Times
  5. Ukraine war latest: Russia rages at UK over ‘serious escalation’ of long-range missiles to Kyiv; Kremlin ‘seriously disturbed’ by Wagner chief’s attacks Sky News
  6. View Full Coverage on Google News

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Exploding grenade launcher a gift from Ukraine, Polish police chief says

WARSAW (Reuters) – Poland’s top policeman said that an explosion in his office was caused by a grenade launcher, telling private broadcaster RMF FM that he had received two of the weapons as a gift from Ukraine.

Poland’s interior ministry and prosecutor’s office had not previously confirmed media reports that the explosion on Wednesday, at police headquarters in Warsaw, was caused by a grenade launcher.

Prosecutors said they were investigating the blast, which resulted in Police Commander in Chief Jaroslaw Szymczyk being taken to hospital.

“When I was moving the used grenade launchers, which were gifts from the Ukrainians, there was an explosion,” Szymczyk told RMF FM.

He said he was moving the launchers into an upright position at the time.

RMF cited a source from a Polish delegation that visited Ukraine as saying Szymczyk had received two launchers from officials as presents during visits to the police and the State Emergency Service of Ukraine.

The officials had assured the Polish delegation that the launchers were not loaded, and the delegation took them back to Warsaw by car before leaving them in the back room of Szymczyk’s office, the source told RMF.

Reuters was unable to independently confirm this version of events. Ukrainian police and the State Emergency Service of Ukraine did not immediately respond to requests for comment. A Polish police spokesman could not immediately be reached for comment.

Szymczyk has been criticised over the incident, with commentators with backgrounds in the security services cited by Polish media as saying that military equipment should not have been taken into Poland from outside the European Union or taken into an office.

(Reporting by Alan Charlish and Dan Peleschuk in Kyiv; Editing by Nick Macfie)

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Florida population is ‘exploding’ in area hardest hit by Hurricane Ian



CNN
 — 

Hurricane Ian last week slammed into one of the fastest-growing areas of the country, putting hundreds of thousands of people in harm’s way — many of whom had never experienced a hurricane.

Florida has added nearly 3 million people since 2010. And the Fort Myers area, which was ravaged by Ian’s deadly storm surge, was recently named the sixth fastest-growing city in the country by the US Census Bureau. The population in the Fort Myers-Cape Coral metro area was around 444,000 in 2000, according to Census Bureau data. By 2021 it had ballooned to more than 787,000.

Southwest Florida’s population has “exploded in part because it’s the cheapest part of the state to live,” according to Jesse Keenan, a professor of sustainable real estate at Tulane University’s School of Architecture, who told CNN that “there has been a huge amount of growth in the past several decades.”

Florida, which has a reputation for attracting retirees, has recently drawn new residents from parts of the country that historically don’t have much experience with hurricanes. In 2019, Florida saw the most migration from Northeast states including New York, New Jersey and Pennsylvania, according to the Census Bureau, in addition to states in the Midwest.

The influx comes as scientists warn that hurricanes are becoming more destructive, with larger storm surges due to sea level rise and a new propensity for strong storms to rapidly intensify.

Those trends combined with the region’s growing population, housing and infrastructure have made the coast even more vulnerable to strong storms.

But little has been done to dissuade people from moving into the danger zone, experts told CNN.

Southwest Florida is attractive in large part because it has a good quality of life – it’s sunny, warm and relatively cheap.

But something else is at play: In 2011, Florida’s Republican-controlled state legislature loosened decades-old state regulations meant to keep development in high-risk areas at a reasonable pace, or to discourage developers from building on low-lying wetlands, Keenan said.

Around the same time, former Gov. Rick Scott and Republican lawmakers approved a state budget that got rid of the Department of Community Affairs, a state office regulating growth and development.

“That opened the door for unrestrained development in ways that put people at a lot of risk, particularly flood risks,” Keenan said.

The weakening of those regulations was cheered by Florida’s business community and real estate sector, which framed the move as supercharging economic growth. But that growth started happening in riskier areas that are more vulnerable to storms.

“The bottom line is the state backed out and the counties were left to their own devices without any adult supervision,” said Keenan. “You build where the land’s cheap, and you sell that housing at a comparatively lower price. It was a race, and storms like this really force everybody to take a water break and reevaluate their lives in many ways.”

Jeremy Porter, senior research fellow for the climate risk nonprofit First Street Foundation, also noted that hard-hit Cape Coral was built on a floodplain.

“There’s a tremendous amount of risk,” Porter said.

But that risk isn’t necessarily obvious to newcomers, and there is no central resource to help homeowners understand the threat.

The Federal Emergency Management Agency’s flood maps – which are used to determine insurance requirements policy premiums – were not designed to serve as a general risk-assessment tool for individuals. They also only consider risk based on previous floods, rather than the increasing threat as rainfall rates get higher, sea level rises and storms get stronger.

A recent report from First Street Foundation found that as of 2020, around 8.7 million properties were listed in FEMA’s Special Flood Hazard Areas — but as many as 14.6 million properties are actually at risk of significant flooding.

And that risk grows even higher in the group’s future projections. First Street’s analysis showed that by 2050, Cape Coral will be among the cities with the greatest proportion of properties with substantial flood risk.

“None of the current standards built into public-facing maps, especially federal maps, take into account that change in climate in the future,” Porter said.

As the focus in Southwest Florida turns to rebuilding, the question now is whether state and county officials will discourage growth in these vulnerable areas. They could push residents to build more resilient homes – or give them “carte blanche” to rebuild to status quo, said Larry Larson, director emeritus and senior policy adviser for the Association of State Floodplain Managers and a longtime flood hazard expert.

“The challenge now for Florida will be you’ve got a lot of destroyed buildings, houses and so on,” Larson told CNN. “What are you going to do when you let them rebuild?”

There are a few ways some governments and the private sector can discourage people from buying homes in flood-prone areas. In some instances, the federal or local governments can buy frequently flooded properties and relocate families that live there.

Another way is to show home buyers the information up front. First Street, for example, has partnered with real estate giant Redfin to show prospective buyers how flood-prone a property is. Those estimates take the climate crisis into account.

Porter said Redfin and First Street have seen home buyers steering away from the most high-risk houses on the market.

“We’re seeing people are starting to interact with that data,” Porter said. “They’re looking explicitly at the flood risk scores.”

But it’s not fool-proof. Porter noted that people aren’t necessarily saying no to flood-prone neighborhoods just yet. Instead, they’re looking at lower-risk houses in the same area.

“It doesn’t mean people are moving outside their housing market when they see that level of risk,” Porter said.

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Exploding package that injured Northeastern University worker had note criticizing Zuckerberg and academia’s relationship with virtual reality developers, sources say



CNN
 — 

Authorities in Boston have launched an investigation after a package sent to Northeastern University exploded and injured a staff member Tuesday evening, officials said.

The package contained a rambling note that criticized Facebook founder Mark Zuckerberg and the relationship between academic institutions and the developers of virtual reality, several federal law enforcement sources told CNN.

The 45-year-old man who opened the package suffered minor hand injuries, according to university and law enforcement officials. Investigators have not said how the package arrived on the campus, stressing the investigation is ongoing.

The campus is expected to fully reopen Wednesday, the university said.

The package was sent to the university’s virtual reality center and was opened by someone who works there, the sources said.

CNN has reached out to Facebook for comment.

The note was in a hard plastic container that detonated as the victim opened the latches and lifted the lid, the sources said.

While the employee was not seriously hurt, the explosion caused hand injuries including lacerations, the sources added.

The package was delivered to Holmes Hall, where the institution’s virtual reality center is located, university spokeperson Shannon Nargi told CNN .

Police were called to the scene around 7:18 p.m., Boston Police Superintendent Felipe Colon said during a news conference Tuesday night.

About a minute after the initial call, a Northeastern University police officer arrived at Homes Hall, said Michael Davis, chief of the university police department.

University police announced the scene was “contained” just before 10 p.m.

“It’s very important to note, our campus is secure,” Davis said during the news conference.

Boston Mayor Michelle Wu praised law enforcement’s response.

“We want to make sure to emphasize that this is of the utmost priority, the safety and well-being of all our young people here,” Wu said during the news conference.

The FBI Boston Division coordinated with the Boston Police Department, FBI spokesperson Kristen Setera told CNN.

The FBI offered the full resources of the Joint Terrorism Task Force, its evidence response team and special agent bomb technicians to assist in the investigation, said Jason Cromartie, assistant special agent in charge.

The university serves more than 16,000 undergraduate students, according to last year’s enrollment report.



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First look at No. 1 pick Travon Walker’s fit with Jags; plus, an exploding NFL trend and a legit QB battle

JACKSONVILLE, Fla. — The biggest challenge for NFL evaluators is determining whether a prospect is an ideal fit for the team’s scheme. For a media scout, the lack of information and insight from each organization can make it difficult to play the mock draft game when attempting to match top prospects with pro franchises.

In the 2022 NFL Draft, the surprising rise of Travon Walker to No. 1 overall created quite a stir in media circles, with many observers obsessing over the Georgia product’s sack production instead of focusing on his intriguing traits as a super-sized defensive playmaker with positional flexibility.

With the Jacksonville Jaguars’ pass-rush need, the pre-draft debate between Walker and Michigan’s Aidan Hutchinson dominated discussion in the days leading up to the top selection, as analysts weighed each prospect’s pros and cons.

After Jacksonville turned in the card for Walker, questions ensued about the 6-foot-5, 272-pounder’s relative lack of college production and how the Jaguars planned to maximize his skill set. What was the thinking behind spending the draft’s No. 1 overall pick on a raw prospect?

“For us, it was just the potential, the upside,” Pederson said last month on The Rich Eisen Show. “As coaches, we’re privy to a lot of film and a lot of conversations that a lot of people don’t get, and a lot of information. And part of our job is to gain that information. And we just felt at the time, and even sitting here today, that the best for our organization was Travon Walker.

“When you look at his body of work at Georgia, from Day 1, the day he got there, they moved him all up and down that defensive front. He’s a very versatile player. There’s a lot of unique things that he can do along the defensive front. And for us, we feel like he’s going to be a good outside edge rusher with Josh Allen and KC, K’Lavon Chaisson, and these guys that we have, and Jordan Smith. He just adds to that room. And it’s a position that we addressed in the draft and we’re happy and we’re excited and we can’t wait to get him in here.”

After spending a few days in Jacksonville this week watching the team conduct OTAs, I understand why Walker was the Jaguars’ choice at No. 1. The massive edge defender is an intimidating presence as a stand-up player in a 3-4 defense. Moreover, he is an explosive athlete with heavy hands and a non-stop motor. Walker’s pass-rushing tools are unrefined, partly because, in UGA’s defense, he wasn’t routinely asked to just pin back his ears and hunt quarterbacks. As Pederson noted, though, the 21-year-old’s rare natural gifts offer immense upside.

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Strange ‘reverse shock wave’ supernova is exploding in the wrong direction

A colorized image of Cassiopeia A based on data from the Hubble, Spitzer and Chandra space telescopes. (Image credit: NASA/JPL-Caltech)

A powerful shock wave traveling through a cloud of gas left behind by the explosive death of a star has a bizarre quirk: Part of it is traveling in the wrong direction, a new study reveals. 

In the study, researchers found that the shock wave is accelerating at different rates, with one section collapsing back toward the origin of the stellar explosion, or supernova, in what the study authors call a “reverse shock.”  

Cassiopeia A is a nebula, or gas cloud, left behind by a supernova in the constellation Cassiopeia, around 11,000 light-years from Earth, making it one of the closest supernova remnants. The nebula, which is around 16 light-years wide, is made of gas (mainly hydrogen) that was expelled both before and during the explosion that ripped apart the original star. A shock wave from that explosion is still rippling through the gas, and theoretical models show that this shock wave should be expanding evenly, like a perfectly rounded balloon that’s constantly being inflated. 

But the researchers found that this wasn’t the case.

“For a long time, we suspected something weird was going on inside Cassiopeia A,” lead author Jacco Vink, an astronomer at the University of Amsterdam in the Netherlands, told Live Science. Previous studies had shown that the internal motions within the nebula were “rather chaotic” and highlighted that the western region of the shock wave moving through the gas cloud might even be going in the wrong direction, he added.

Related: 11 fascinating facts about our Milky Way galaxy 

In the new study, the researchers analyzed the movement of the shock wave, using X-ray images collected by NASA’s Chandra X-ray Observatory, a telescope that orbits Earth. The data, collected over 19 years, confirmed that part of the western region of the shock wave was, in fact, retreating in the opposite direction in a reverse shock. 

But they also discovered something even more surprising: Parts of the same region were still accelerating away from the supernova’s epicenter, like the rest of the shock wave.

Uneven expansion 

The current average speed of the expanding gas in Cassiopeia A is around 13.4 million mph (21.6 million km/h), which makes it one of the fastest shock waves ever seen in a supernova remnant, Vink said. This is mainly because the remnant is so young; light from Cassiopeia A reached Earth in 1970. But over time, shock waves lose their momentum to their surroundings and slow down. 

Cassiopeia A consists of two main expanding bands of gas: an inner shell and an outer shell. These two shells are two halves of the same shock wave, and across most of the nebula, the inner and outer shells are traveling at the same speed and in the same direction. But in the western region, the two shells are going in opposite directions: The outer shell is still expanding outward, but the inner shell is moving back toward where the exploding star would have been. 

An image of Cassiopeia A showing the shock wave move through the inner and outer shells of gas. The blue arrows show the western section of the inner shell moving back towards the center of the nebula. (Image credit: J.Vink/astronomie.nl)

The reverse shock is retreating at around 4.3 million mph (6.9 million km/h), which is about a third of the average expansion speed of the rest of the nebula. However, what really puzzled the researchers was how fast the outer shell was expanding compared with the retreating inner shell in this region. The researchers had expected the outer shell to be expanding at a decreased rate compared with the rest of the shock wave, but they found that it was actually accelerating faster than some other regions of the shock wave. “That was a total surprise,” Vink said.

Cosmic collision 

The unusual expansion within Cassiopeia A’s western region does not match up with theoretical supernova models and suggests that something happened to the shock wave in the aftermath of the stellar explosion, Vink said. 

The researchers said the most likely explanation is that the shock wave collided with another shell of gas that was likely ejected by the star before it exploded. As the shock wave hit this gas, it may have slowed down and created a pressure buildup that pushed the inner shell back toward the center. However, the outer shell still may have been forced through this blockage and begun to accelerate again on the other side, Vink said. “This explains both the inward movement of the inner shell but also predicts that the outer shell should be accelerating, as indeed we measured,” he added. 

The researchers also think the unique way the original star died could explain the uneven shock wave. Cassiopeia A is the result of a Type IIb supernova, in which a massive star exploded after it  had almost completely shed its outer layers, Vink said.

An image of  Cassiopeia A combining X-ray data collected by NASA’s Imaging X-ray Polarimetry Explorer, shown in magenta, and NASA’s Chandra X-Ray Observatory, in blue. (Image credit: NASA/CXC/SAO/IXPE)

“X-ray estimates suggest that the star was around four to six times the mass of the sun during the explosion,” Vink said, but the star most likely had a mass of around 18 times the sun when it was born. This means the star lost around two-thirds of its mass, most of which would have been hydrogen, before it exploded; The shock wave may have later collided with this gas, Vink said.

There are several theories as to why Cassiopeia A lost so much of its mass before it exploded. In September 2020, another team of researchers proposed that the original star was part of a binary star system, where two stars orbit each other. That research team said this companion star also could have gone supernova before Cassiopeia A and blasted off the star’s hydrogen “skin” in the process, Live Science previously reported

However, the authors of the new study are unconvinced by this theory. “The only problem is that we have not yet found the remains of the other star,” Vink said. “So, at this stage, it remains speculative.”

So for now, no one knows exactly what is fueling Cassiopeia A’s uneven shock wave.

The study was published online Jan. 21 in the preprint server arXiv and has been accepted for future publication in The Astrophysical Journal.

Originally published on Live Science.

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NASA’s New X-Ray Space Telescope Snaps First Image: an Exploding Star

NASA’s new X-ray space telescope captured its first image, and it shows the vibrant electromagnetic afterglow of a supernova explosion.

The Imaging X-Ray Polarimetry Explorer (IXPE) launched into orbit aboard a SpaceX Falcon 9 rocket on December 9, then spent a month calibrating its instruments and adjusting to the space environment. When it was finally ready to collect data, mission controllers pointed its mirrors at a supernova called Cassiopeia A — the vibrant, gas-cloud remains of a star that exploded in the 17th century.

The first image was released on Monday. The gas cloud is about 10 light-years wide. In visible light, it doesn’t actually glow the stunning purple color depicted above. That’s just the color NASA researchers chose to represent how powerful the X-ray light is in different parts of the cloud.

In the image below, they used a wider range of colors to show the variation in X-rays.

The IXPE image of Cassiopeia A, January 11-18, 2022, shows the increasing intensity of X-rays in colors ranging from cool purple and blue to red and hot white.

NASA



When the star exploded, its shock waves superheated gas in its vicinity and accelerated nearby particles, causing it to glow bright in X-ray light. Somewhere in the center of those gas clouds, there’s a super-dense object that formed when the former star’s core collapsed. It could be a black hole or a neutron star.

IXPE is set to spend at least two years studying the most extreme and mysterious objects in the universe — nebulae, supernovas, neutron stars, and black holes. It’s NASA’s first major X-ray space telescope since the Chandra X-ray Observatory launched into orbit in 1999. That telescope’s first image also captured Cassiopeia A.

“The IXPE image of Cassiopeia A is as historic as the Chandra image of the same supernova remnant,” Martin C. Weisskopf, who leads the IXPE team at NASA, said in a press release. “It demonstrates IXPE’s potential to gain new, never-before-seen information about Cassiopeia A, which is under analysis right now.”



An illustration of NASA’s Imaging X-ray Polarimetry Explorer.

NASA



Unlike Chandra, IXPE focuses on polarization — the direction that waves of X-ray light are pointed as they travel through space. That information can tell scientists a lot about how the X-rays are produced and allow them to see how radiation varies across the object they’re studying. In this case, it could offer new peeks at what’s happening inside those gas clouds and explain why they emit such powerful X-rays.

“The IXPE image of Cassiopeia A is bellissima, and we look forward to analyzing the polarimetry data to learn even more about this supernova remnant,” Paolo Soffitta, the Italian IXPE team leader at the National Institute of Astrophysics (INAF) in Rome, said in the press release.

Now the IXPE team is working on using the telescope’s data to build a map of polarized X-rays across the supernova cloud.

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Astronomers Capture Red Supergiant Star Exploding in Massive Supernova – For the Very First Time

An artist’s impression of a red supergiant star in the final year of its life emitting a tumultuous cloud of gas. This suggests at least some of these stars undergo significant internal changes before going supernova. Credit: W.M. Keck Observatory/Adam Makarenko

Astronomers Capture Red Supergiant’s Death Throes

“For the first time, we watched a red supergiant star explode,” researcher says.

For the first time ever, astronomers have imaged in real time the dramatic end to a red supergiant’s life — watching the massive star’s rapid self-destruction and final death throes before collapsing into a type II supernova.

Led by researchers at
An artist’s rendition of a red supergiant star transitioning into a Type II supernova, emitting a violent eruption of radiation and gas on its dying breath before collapsing and exploding. Credit: W. M. Keck Observatory/Adam Makarenko

Although the work was conducted at Northwestern, where Jacobson-Galán was a National Science Foundation (NSF) Graduate Research Fellow, he has since moved to UC Berkeley. Northwestern co-authors include Deanne Coppejans, Charlie Kilpatrick, Giacomo Terreran, Peter Blanchard and Lindsay DeMarchi, who are all members of Northwestern’s Center for Interdisciplinary and Exploratory Research in Astrophysics (CIERA).

‘We’ve never confirmed such violent activity’

The University of Hawaiʻi Institute for AstronomyPan-STARRS on Haleakala, Maui, first detected the doomed massive star in summer 2020 via the huge amount of light radiating from the red supergiant. A few months later, in fall of 2020, a supernova lit the sky.

The team quickly captured the powerful flash and obtained the very first spectrum of the energetic explosion, named supernova 2020tlf (SN 2020tlf) using the W.M. Keck Observatory’s Low Resolution Imaging Spectrometer on Maunakea, Hawaiʻi. The data showed direct evidence of dense circumstellar material surrounding the star at the time of explosion, likely the same gas that Pan-STARRS had imaged the red supergiant star violently ejecting earlier in the summer.

“It’s like watching a ticking time bomb,” said Raffaella Margutti, an adjunct associate professor at CIERA and the paper’s senior author. “We’ve never confirmed such violent activity in a dying red supergiant star where we see it produce such a luminous emission, then collapse and combust, until now.”

The team continued to monitor SN 2020tlf after the explosion. Based on data obtained from Keck Observatory’s Deep Imaging and Multi-Object Spectrograph and Near Infrared Echellette Spectrograph, the researchers determined SN 2020tlf’s progenitor red supergiant star — located in the NGC 5731 galaxy about 120 million light-years away from Earth — was 10 times more massive than the sun.

Remote possibilities

Margutti and Jacobson-Galán conducted most of the study during their time at Northwestern, with Margutti serving as an associate professor of physics and astronomy and member of CIERA, and Jacobson-Galán as a graduate student in Margutti’s research group. Margutti is now an associate professor of astronomy and astrophysics at UC Berkeley.

Northwestern’s remote access to Keck Observatory’s telescopes was integral to their research. From the University’s Evanston campus, astronomers can connect with an on-site telescope operator in Hawaiʻi and choose where to position the telescope. By bypassing long-distance travel to Hawaiʻi, astronomers save precious observing time — often catching transient events like supernovas, which can quickly flare up and then swiftly vanish.

“This significant discovery of a red supergiant supernova is yet one more strong indication of the importance of Northwestern’s investment in access to top private telescope facilities, including the Keck Observatory,” said Vicky Kalogera, the Daniel I. Linzer Distinguished University Professor of Physics and Astronomy at Northwestern’s Weinberg College of Arts and Sciences and director of CIERA. “The Keck telescopes, currently the best on our planet, uniquely enable scientific advances of this caliber as CIERA researchers have shown since our Keck partnership started just a few years ago.”

Margutti, Jacobson-Galán and their Northwestern co-authors are members of the Young Supernova Experiment, which uses the Pan-STARRS telescope to catch supernovae right after they explode.

“I am most excited by all of the new ‘unknowns’ that have been unlocked by this discovery,” Jacobson-Galán said. “Detecting more events like SN 2020tlf will dramatically impact how we define the final months of stellar evolution, uniting observers and theorists in the quest to solve the mystery on how massive stars spend the final moments of their lives.”

Reference: “Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf” by W. V. Jacobson-Galán, L. Dessart, D. O. Jones, R. Margutti, D. L. Coppejans, G. Dimitriadis, R. J. Foley, C. D. Kilpatrick, D. J. Matthews, S. Rest, G. Terreran, P. D. Aleo, K. Auchettl, P. K. Blanchard, D. A. Coulter, K. W. Davis, T. J. L. de Boer, L. DeMarchi, M. R. Drout, N. Earl, A. Gagliano, C. Gall, J. Hjorth, M. E. Huber, A. L. Ibik, D. Milisavljevic, Y.-C. Pan, A. Rest, R. Ridden-Harper, C. Rojas-Bravo, M. R. Siebert, K. W. Smith, K. Taggart, S. Tinyanont, Q. Wang and Y. Zenati, 6 January 2022, The Astrophysical Journal.
DOI: 10.3847/1538-4357/ac3f3a

The study, “Final Moments I: Precursor emission, envelope inflation and enhanced mass loss preceding the luminous type II supernova 2020tlf,” was supported by (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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