Elon Musk has become the first person in history to surpass $400,000,000,000 net worth

Elon Musk has become the first person in history to surpass $400,000,000,000 net worth

Elon Musk has become the first person in history to surpass $400,000,000,000 net worth

According to Bloomberg, Elon Musk has seen a recent surge in wealth for one big reason

With Elon Musk owning SpaceX, Tesla and Twitter to name just a few, he’s got countless sources of income and there’s no wonder the entrepreneur has surpassed $400,000,000,000 net worth.

The billionaire reached the historic wealth marker this week, making him the first person in history to ever have a net worth so high.

According to the Bloomberg Billionaires Index, the 53-year-old is now worth an incredible $447 billion as of December 11, which is $198 billion more than the second richest person in the world Jeff Bezos at $249 billion.

Although if we go off Forbes’ rich list, he is only worth a mere $379.4 billion – pathetic.

What is almost unbelievable though, is that just three weeks ago we published how he was worth $315.7 billion meaning that he’s incurred $63.7 billion… again, according to Forbes.

Elon Musk has become the first person in history to amass more than $400 billion, according to Bloomberg (Anna Moneymaker/Getty Images)

Elon Musk has become the first person in history to amass more than $400 billion, according to Bloomberg (Anna Moneymaker/Getty Images)

Meanwhile, Bloomberg’s records state that since Election Day, dominated by President-elect Donald Trump, Musk has become roughly $136 billion richer.

And he even has a role in the White House.

“I am pleased to announce that the Great Elon Musk, working in conjunction with American Patriot Vivek Ramaswamy, will lead the Department of Government Efficiency (‘DOGE’),” Trump wrote at the time.

The President-Elect went on to explain that the pair would ‘pave the way for my Administration to dismantle Government Bureaucracy, slash excess regulations, cut wasteful expenditures, and restructure Federal Agencies – Essential to the ‘Save America’ Movement’.

As well as Tesla, SpaceX and Twitter, Musk also owns artificial intelligence company xAI, American infrastructure business The Boring Company as well as tech-company Neuralink.

Musk has incurred $136 billion since President-elect Donald Trump beat Vice-President Kamala Harris at the poles (Brandon Bell/Getty Images)

Musk has incurred $136 billion since President-elect Donald Trump beat Vice-President Kamala Harris at the poles (Brandon Bell/Getty Images)

In its own words, Neuralink states: “We are currently focused on giving people with quadriplegia the ability to control their computers and mobile devices with their thoughts.”

Musk also owns a healthy share of cryptocurrency including Dogecoin, designed initially to make a joke of the crypto system using a popular internet meme of a dog.

His upcoming role as the US’ head of the new Department of Government Efficiency (DOGE) is actually named after the memecoin.

Last week, Musk’s record-breaking $56bn payout was denied for a second time, with a judge ruling against the richest man in the world.

Musk was set to receive the $56bn in pay from Tesla under a historic compensation package struck in 2018. It was described in court documents as the largest ever seen in public markets.

However, Judge Kathleen McCormick called Tesla’s legal argument ‘fatally flawed’ and at times ‘indefensible’ as she denied the motion in a 101-page opinion.
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New Research Shows Southern Ocean as a Powerful Influence on Climate Change

New Research Shows Southern Ocean as a Powerful Influence on Climate Change

model reveals the Southern Ocean as a powerful influence on climate change
The Southern Ocean, the vast belt of water circling Antarctica, is a turbulent part of the ocean conveyor, where vast reservoirs of heat and carbon may rise to the surface, interacting with the atmosphere. The region, researchers say, plays a critical role in climate change. Credit: Google Earth

Researchers at MIT and Florida State University found evidence that the missing piece in the model of world’s oceans circulation of heat, water and carbon around the planet may lie in the Southern Ocean. Their research has lead them to draw up a new schematic for ocean circulation and according to their observations and models, the Southern Ocean is a site where strong winds dredge waters that play a role in climate change.

The world’s oceans act as a massive conveyor, circulating heat, water and carbon around the planet. This global system plays a key role in climate change, storing and releasing heat throughout the world. To study how this system affects climate, scientists have largely focused on the North Atlantic, a major basin where water sinks, burying carbon and heat deep in the ocean’s interior.

But what goes down must come back up, and it’s been a mystery where, and how, deep waters circulate back to the surface. Filling in this missing piece of the circulation, and developing theories and models that capture it, may help researchers understand and predict the ocean’s role in climate and climate change.

Recently, scientists have found evidence that the missing piece may lie in the Southern Ocean — the vast ribbon of water encircling Antarctica. The Southern Ocean, according to observations and models, is a site where strong winds blowing along the Antarctic Circumpolar Current dredge waters up from the depths.

“There’s a lot of carbon and heat in the interior ocean,” says John Marshall, the Cecil and Ida Green Professor of Oceanography at MIT. “The Southern Ocean is the window by which the interior of the ocean connects to the atmosphere above.”

Marshall and Kevin Speer, a professor of physical oceanography at Florida State University, have published a paper in Nature Geoscience in which they review past work, examine the Southern Ocean’s influence on climate and draw up a new schematic for ocean circulation.

A revised conveyor

For decades, a “conveyor belt” model, developed by paleoclimatologist Wallace Broecker, has served as a simple cartoon of ocean circulation. The diagram depicts warm water moving northward, plunging deep into the North Atlantic; then coursing south as cold water toward Antarctica; then back north again, where waters rise and warm in the North Pacific.

However, evidence has shown that waters rise to the surface not so much in the North Pacific, but in the Southern Ocean — a distinction that Marshall and Speer illustrate in their updated diagram.

schematic emphasizes the role of the Southern Ocean in the world’s ocean circulation
A new schematic emphasizes the role of the Southern Ocean in the world’s ocean circulation. The upper regions of ocean circulation are fed predominantly by broad upwelling across surfaces at mid-depth over the main ocean basins (rising blue-green-yellow arrows). Upwelling to the ocean surface occurs mainly around Antarctica in the Southern Ocean (rising yellow-red arrows) with wind and eddies playing a central role. Credit: John Marshall and Kevin Speer

Marshall says winds and eddies along the Southern Ocean drag deep waters — and any buried carbon — to the surface around Antarctica. He and Speer write that the updated diagram “brings the Southern Ocean to the forefront” of the global circulation system, highlighting its role as a powerful climate mediator.

Indeed, Marshall and Speer review evidence that the Southern Ocean may have had a part in thawing the planet out of the last Ice Age. While it’s unclear what caused Earth to warm initially, this warming may have driven surface wind patterns poleward, pulling up deep water and carbon — which would have been released into the atmosphere, further warming the climate.

Shifting winds

In a cooling world, it appears that winds shift slightly closer to the Equator, and are buffeted by the continents. In a warming world, winds shift toward the poles; in the Southern Ocean, unimpeded winds whip up deep waters. The researchers note that two manmade atmospheric trends — ozone depletion and greenhouse gas emissions from fossil fuels — have a large effect on winds over the Southern Ocean: As the ozone hole recovers, greenhouse gases rise and the planet warms, winds over the Southern Ocean are likely to shift, affecting the delicate balance at play. In the future, if the Southern Ocean experiences stronger winds displaced slightly south of their current position, Antarctica’s ice shelves may be more vulnerable to melting — a phenomenon that may also have contributed to the end of the Ice Age.

“There are huge reservoirs of carbon in the interior of the ocean,” Marshall says. “If the climate changes and makes it easier for that carbon to get into the atmosphere, then there will be an additional warming effect.”

Jorge Sarmiento, a professor of atmospheric and oceanic sciences at Princeton University, says the Southern Ocean has been a difficult area to study. To fully understand the Southern Ocean’s dynamics requires models with high resolution — a significant challenge, given the ocean’s size.

“Because it’s so hard to observe the Southern Ocean, we’re still in the process of learning things,” says Sarmiento, who was not involved with this research. “So I think this is a very nice snapshot of our current understanding, based on models and observations, and it will sort of be a touchstone for future developments in the field.”

Marshall and Speer are now working with a multi-institution team led by MIT’s collaborator, the Woods Hole Oceanographic Institution, to measure how waters upwell in the Southern Ocean. The researchers are studying the flow driven by eddies in the Antarctic Circumpolar Current, and have deployed tracers and deep drifters to measure its effects; temperature, salinity and oxygen content in the water also help tell them how eddies behave, and how quickly or slowly warm water rises to the surface.

“Any perturbation that is made to the atmosphere, whether it’s due to glacial cycles or ozone or greenhouse forcing, can change the balance over the Southern Ocean,” Marshall says. “We have to understand how the Southern Ocean works in the climate system and take that into account.”

Reference: “Closure of the meridional overturning circulation through Southern Ocean upwelling” by John Marshall and Kevin Speer, 26 February 2012, Nature Geoscience.
DOI: 10.1038/ngeo1391

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Jim Carrey says he will only play The Grinch again under one condition

Jim Carrey says he will only play The Grinch again under one condition

Jim Carrey says he will only play The Grinch again under one condition

The actor shared his thoughts on returning to the beloved character almost 25 years later

Jim Carrey has revealed he’s open to returning to his infamous and beloved role of The Grinch, but he does have one condition that would have to be met first.

It’s now nearing 25 years since Carrey appeared as the grumpy, green Grinch in the 2000 adaptation of How the Grinch Stole Christmas, but every year millions of people across the globe return to hit play on the movie, feeling like it’s not Christmas without it.

Almost 20 years after the movie’s release, one fan wrote on Twitter: “The Jim Carrey version of the Grinch is a top-tier Christmas movie and I’m not saying you’re wrong if you disagree, but you definitely aren’t right.”

Carrey played the Grinch in 2000 (Universal Pictures)

Carrey played the Grinch in 2000 (Universal Pictures)

Carrey has taken on a huge range of roles since then, appearing in movies like Bruce Almighty, Eternal Sunshine of the Spotless Mind and Kick-Ass 2.

Most recently he’s taken on the eccentric role of Dr. Robotnik in the Sonic the Hedgehog movies, but Carrey has now admitted that he would be up for returning to the Grinch, even after so many years have passed.

The actor made the revelation in an interview with Comicbook.com, in which he was asked which of his characters he’d like to play again.

Carrey volunteered the idea of the Grinch, however, he admitted there was one aspect of the role that he wasn’t a fan of.

He said: “Oh, gosh, you know, if we could figure out the Grinch. The thing about it is, on the day, I do that with a ton of makeup and can hardly breathe. It was an extremely excruciating process. The children were in my mind all the time. ‘It’s for the kids. It’s for the kids. It’s for the kids.'”

Carrey most recently appears in the Sonic the Hedgehog movies (Joe Maher/Getty Images)

Carrey most recently appears in the Sonic the Hedgehog movies (Joe Maher/Getty Images)

While he’s clearly not keen to rush back to the makeup chair, Carrey pointed out that advancements in technology might make it easier for him to return to the role without the more ‘excruciating’ aspects of it.

Sharing the conditions under which he’d happily return, he continued: “And now, with motion capture and things like that, I could be free to do other things. Anything is possible in this world.”

Carrey’s comments came around the same time he spoke to the Associated Press about the idea of retiring; something he has previously floated.

When asked why he’s still working on big projects, Carrey jokingly: “I bought a lot of stuff and I need the money, frankly.”

News of Carrey’s potential return to the Grinch has understandably sparked excitement among fans, with one person writing: “I speak for everyone when I say F***ING YES! Jim Carrey was iconic as the Grinch & the best live screen adaptation of Dr Seuss!”

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Hypersonic Reentry: How OSIRIS-REx Transformed Space Science

Hypersonic Reentry: How OSIRIS-REx Transformed Space Science

OSIRIS-REx Sample Return Capsule Maximum Heating in Earth’s Atmosphere
The OSIRIS-REx mission achieved a significant milestone by returning the first U.S. asteroid sample, accompanied by groundbreaking research. A large-scale observation campaign, involving over 80 collaborators and 400 sensors, provided invaluable data about the entry of a meter-sized object into Earth’s atmosphere. Credit: NASA’s Goddard Space Flight Center/CI Lab

The OSIRIS-REx mission returned asteroid samples, enabling a vast observation campaign that provided new insights into atmospheric entry using innovative distributed acoustic sensing technology.

This success prepares the spacecraft, now OSIRIS-APEX, for its 2029 mission to asteroid Apophis.

The OSIRIS-REx mission achieved a historic milestone last year as the first U.S. mission to return an asteroid sample to Earth, bringing with it a wealth of groundbreaking data. An international team, led by Sandia National Laboratories and including researchers from Los Alamos National Laboratory, has now shared preliminary findings from the capsule’s atmospheric reentry.

Unprecedented Geophysical Campaign

The capsule’s return marked the largest geophysical observation effort of its kind. “This project was a unique opportunity for us to observe the geophysical signals produced by a meter-sized object traveling at hypersonic speeds,” said Chris Carr, lead researcher at Los Alamos National Laboratory. “There are few chances for scientists to be prepared to collect this type of data that we need to propel scientific inquiry for years to come.”

The campaign involved over 400 sensors, many of which were stationed near Eureka, NV along the “loneliest road in America.” Given the size of the project, there were many objectives among the more than 80 collaborators. One team of Los Alamos scientists focused on distributed acoustic sensing (DAS), and the paper as a whole encompasses many methods to obtain data during the capsule’s return.

OSIRIS-REx Sample Return Landing
The sample return capsule from NASA’s OSIRIS-REx mission is seen shortly after touching down in the desert on September 24, 2023, at the Department of Defense’s Utah Test and Training Range. The sample was collected from the asteroid Bennu in October 2020 by NASA’s OSIRIS-REx spacecraft. Credit: NASA/Keegan Barber

Breakthrough in Space Matter Observation

Though space matter does pass through Earth’s atmosphere, it is difficult to determine where and when the object will make its entry. Even when it is possible to determine those factors, the financial and logistic constraints will almost certainly render it a non-starter. This results in very limited real-time observational data about the behavior of foreign objects entering the atmosphere. The OSIRIS-REx sample return capsule gave researchers a unique opportunity to collect this data.

“For our DAS sub-team, it was the fact that we recorded the signal using a surface-laid cable,” Carr said. “This was the first time such a signal was recorded by DAS, and going into the fieldwork, we weren’t sure if we’d be successful. We were very excited to see the first plots of our data and see that we recorded it.”

OSIRIS REx Spacecraft Leaving Bennu Surface
NASA’s OSIRIS-REx spacecraft leaving the surface of asteroid Bennu after collecting a sample. Credit: NASA’s Goddard Space Flight Center/CI Lab/SVS

Enhancing Future Space Research

The preliminary findings of the campaign show implications for future projects in space and on the ground; specifically, aiding the development of entry and propagation models. This paper documents the process used to detect and record the entry of the capsule, and it shows that the methods are capable of handling the kind of observation needed in this large of a campaign. It has substantially increased knowledge of entry detection for space objects and will allow researchers to better understand how objects enter the Earth’s atmosphere.

OSIRIS-APEX Asteroid Apophis
OSIRIS-APEX carries out its extended mission to near-Earth asteroid Apophis. Credit: NASA’s Goddard Space Flight Center/CI Lab
Preparing for the Next Mission

Now that the capsule has touched down and the data is ready for release, OSIRIS-REx is being made ready for its next mission. NASA renamed the spacecraft OSIRIS-APEX as it is prepared for a 2029 arrival to the asteroid Apophis.

Reference: “Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry” by Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama and Cleat Zeiler, 30 September 2024, The Planetary Science Journal.
DOI: 10.3847/PSJ/ad5b5e
Funding: Center for Space and Earth Science and LDRD award 20220188DR

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MIT Unveils Breakthrough in Detecting Tiny Asteroids, Boosting Planetary Defense

MIT Unveils Breakthrough in Detecting Tiny Asteroids, Boosting Planetary Defense

James Webb Space Telescope Revealing Small Asteroids
An artist’s illustration of NASA’s James Webb Space Telescope revealing, in the infrared, a population of small main-belt asteroids. Credit: Ella Maru and Julien de Wit

Researchers at MIT have developed a method to detect small asteroids in the main asteroid belt, significantly improving our ability to spot objects as little as 10 meters across.

This new technique, which identified 138 space rocks ranging from bus- to stadium-sized, allows for earlier detection and better tracking of potential near-Earth objects, enhancing planetary defense. The approach, using data from telescopes initially aimed at exoplanets, has uncovered over a hundred new asteroids, with implications for understanding asteroid origins and collision processes.

Advancements in Asteroid Detection

The asteroid that wiped out the dinosaurs is estimated to have been about 10 kilometers (6 miles) wide — roughly the width of Brooklyn, New York. Fortunately, impacts from such massive objects are extremely rare, occurring only once every 100 million to 500 million years.

In comparison, much smaller asteroids, about the size of a bus, hit Earth far more often — approximately every few years. These “decameter” asteroids, measuring 10 to 100 meters (30 to 330 feet) across, are more likely to break free from the main asteroid belt and become near-Earth objects. When they do collide with Earth, they can cause significant damage, as seen in the 1908 Tunguska event in Siberia and the 2013 Chelyabinsk explosion over Russia. Studying decameter-sized asteroids in the main belt could help scientists better understand the origins of meteorites and the processes that shape our solar system.

Now, an international team led by physicists at MIT have found a way to spot the smallest decameter asteroids within the main asteroid belt — a rubble field between Mars and Jupiter where millions of asteroids orbit. Until now, the smallest asteroids that scientists were able to discern there were about a kilometer in diameter. With the team’s new approach, scientists can now spot asteroids in the main belt as small as 10 meters across.

In a paper published on December 9 in the journal Nature, the researchers report that they have used their approach to detect more than 100 new decameter asteroids in the main asteroid belt. The space rocks range from the size of a bus to several stadiums wide, and are the smallest asteroids within the main belt that have been detected to date.

The researchers envision that the approach can be used to identify and track asteroids that are likely to approach Earth.

“We have been able to detect near-Earth objects down to 10 meters in size when they are really close to Earth,” says the study’s lead author, Artem Burdanov, a research scientist in MIT’s Department of Earth, Atmospheric and Planetary Sciences. “We now have a way of spotting these small asteroids when they are much farther away, so we can do more precise orbital tracking, which is key for planetary defense.”

The study’s co-authors include MIT professors of planetary science Julien de Wit and Richard Binzel, along with collaborators from multiple other institutions, including the University of Liege in Belgium, Charles University in the Czech Republic, the European Space Agency, and institutions in Germany including Max Planck Institute for Extraterrestrial Physics, and the University of Oldenburg.

TRAPPIST La Silla Observatory
One of the observing domes of La Silla Observatory, the TRAPPIST. Credit: ESO
Integrating Exoplanet and Asteroid Research

De Wit and his team are primarily focused on searches and studies of exoplanets — worlds outside the solar system that may be habitable. The researchers are part of the group that in 2016 discovered a planetary system around TRAPPIST-1, a star that’s about 40 light years from Earth. Using the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) in Chile, the team confirmed that the star hosts rocky, Earth-sized planets, several of which are in the habitable zone.

Scientists have since trained many telescopes, focused at various wavelengths, on the TRAPPIST-1 system to further characterize the planets and look for signs of life. With these searches, astronomers have had to pick through the “noise” in telescope images, such as any gas, dust, and planetary objects between Earth and the star, to more clearly decipher the TRAPPIST-1 planets. Often, the noise they discard includes passing asteroids.

“For most astronomers, asteroids are sort of seen as the vermin of the sky, in the sense that they just cross your field of view and affect your data,” de Wit says.

De Wit and Burdanov wondered whether the same data used to search for exoplanets could be recycled and mined for asteroids in our own solar system. To do so, they looked to “shift and stack,” an image processing technique that was first developed in the 1990s. The method involves shifting multiple images of the same field of view and stacking the images to see whether an otherwise faint object can outshine the noise.

Breakthroughs in Asteroid Imaging

Applying this method to search for unknown asteroids in images that are originally focused on far-off stars would require significant computational resources, as it would involve testing a huge number of scenarios for where an asteroid might be. The researchers would then have to shift thousands of images for each scenario to see whether an asteroid is indeed where it was predicted to be.

Several years ago, Burdanov, de Wit, and MIT graduate student Samantha Hasler found they could do that using state-of-the-art graphics processing units that can process an enormous amount of imaging data at high speeds.

They initially tried their approach on data from the SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) survey — a system of ground-based telescopes that takes many images of a star over time. This effort, along with a second application using data from a telescope in Antarctica, showed that researchers could indeed spot a vast amount of new asteroids in the main belt.

Webb Telescope in Space
James Webb Space Telescope artist concept. Credit: NASA
“An Unexplored Space”

For the new study, the researchers looked for more asteroids, down to smaller sizes, using data from the world’s most powerful observatory — NASA’s James Webb Space Telescope (JWST), which is particularly sensitive to infrared rather than visible light. As it happens, asteroids that orbit in the main asteroid belt are much brighter at infrared wavelengths than at visible wavelengths, and thus are far easier to detect with JWST’s infrared capabilities.

The team applied their approach to JWST images of TRAPPIST-1. The data comprised more than 10,000 images of the star, which were originally obtained to search for signs of atmospheres around the system’s inner planets. After processing the images, the researchers were able to spot eight known asteroids in the main belt. They then looked further and discovered 138 new asteroids around the main belt, all within tens of meters in diameter — the smallest main belt asteroids detected to date. They suspect a few asteroids are on their way to becoming near-Earth objects, while one is likely a Trojan — an asteroid that trails Jupiter.

“We thought we would just detect a few new objects, but we detected so many more than expected, especially small ones,” de Wit says. “It is a sign that we are probing a new population regime, where many more small objects are formed through cascades of collisions that are very efficient at breaking down asteroids below roughly 100 meters.”

“Statistics of these decameter main belt asteroids are critical for modeling,” adds Miroslav Broz, co-author from the Prague Charles University in Czech Republic, and a specialist of the various asteroid populations in the solar system. “In fact, this is the debris ejected during collisions of bigger, kilometers-sized asteroids, which are observable and often exhibit similar orbits about the Sun, so that we group them into ‘families’ of asteroids.”

“This is a totally new, unexplored space we are entering, thanks to modern technologies,” Burdanov says. “It’s a good example of what we can do as a field when we look at the data differently. Sometimes there’s a big payoff, and this is one of them.”

Reference: “JWST sighting of decameter main-belt asteroids and view on meteorite sources” by Artem Y. Burdanov, Julien de Wit, Miroslav Brož, Thomas G. Müller, Tobias Hoffmann, Marin Ferrais, Marco Micheli, Emmanuel Jehin, Daniel Parrott, Samantha N. Hasler, Richard P. Binzel, Elsa Ducrot, Laura Kreidberg, Michaël Gillon, Thomas P. Greene, Will M. Grundy, Theodore Kareta, Pierre-Olivier Lagage, Nicholas Moskovitz, Audrey Thirouin, Cristina A. Thomas and Sebastian Zieba, 9 December 2024, Nature.

DOI: 10.1038/s41586-024-08480-z

This work was supported, in part, by the Heising-Simons Foundation, the Czech Science Foundation, and the NVIDIA Academic Hardware Grant Program.

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Illuminating the Abyss: Photon Rings and the Future of Black Hole Imaging

Illuminating the Abyss: Photon Rings and the Future of Black Hole Imaging

Black Hole Photon Ring Art Concept
Using a global array of radio telescopes, astronomers captured the first-ever image of a black hole. Future plans involve moving part of the telescope into space and using advanced laser data transmission to improve image quality and test theories of gravity. Credit: SciTechDaily.com

TBIRD, a laser communications system developed by Lincoln Laboratory, transmits data at unprecedented speeds, enabling scientists to capture black holes’ elusive photon rings.

The Event Horizon Telescope network captured groundbreaking images of a black hole in 2019 and 2021. Plans to enhance these observations include placing telescopes in space and employing advanced laser communication technology from MIT’s Lincoln Laboratory. This will enable detailed tests of gravitational theories through high-resolution imaging of black holes.

First Image of a Black Hole

In April 2019, astronomers from around the world made history by capturing the first-ever image of a black hole — a gravitational giant so powerful that not even light can escape its pull. This groundbreaking image revealed the glowing gas surrounding the supermassive black hole at the center of the galaxy Messier 87 (M87). Two years later, in March 2021, the same team released another remarkable image showing polarized light near the black hole, offering the first glimpse of its magnetic field.

The instrument behind these stunning images is the Event Horizon Telescope (EHT), a global network of radio telescopes that work together to form a virtual Earth-sized observatory. By combining data from telescopes around the globe, the EHT can create incredibly detailed images of distant black holes. Now, scientists are planning to extend the EHT into space to achieve even sharper views of M87’s black hole. However, transmitting the enormous amounts of data collected by space-based telescopes back to Earth is a major technical challenge. To solve this, researchers at MIT Lincoln Laboratory have developed a cutting-edge laser communications (lasercom) system capable of transmitting data at the extremely high speeds required for this ambitious mission.

Black Hole M87 Photon Ring
Astronomers imaged the black hole at the center of galaxy M87 in 2019 (left) and its magnetic field in 2021 (center). A major goal is to image its photon ring (simulated at right).
Credit: Event Horizon Telescope; Science Advances, vol. 6, no. 12
Expanding Imaging Techniques into Space

The EHT created the two existing images of M87’s black hole via interferometry — specifically, very long-baseline interferometry. Interferometry works by collecting light in the form of radio waves simultaneously with multiple telescopes in separate places on the globe and then comparing the phase difference of the radio waves at the various locations in order to pinpoint the direction of the source. By taking measurements with different combinations of the telescopes around the planet, the EHT collaboration — which included staff members at the Harvard-Smithsonian Center for Astrophysics (CfA) and MIT Haystack Observatory — essentially created an Earth-sized telescope in order to image the incredibly faint black hole 55 million light-years away from Earth.

With interferometry, the bigger the telescope, the better the resolution of the image. Therefore, in order to focus in on even finer characteristics of these black holes, a bigger instrument is needed. Details that astronomers hope to resolve include the turbulence of the gas falling into a black hole (which drives the accumulation of matter onto the black hole through a process called accretion) and a black hole’s shadow (which could be used to help pin down where the jet coming from M87 is drawing its energy from). The ultimate goal is to observe a photon ring (the place where light orbits closest before escaping) around the black hole. Capturing an image of the photon ring would enable scientists to put Albert Einstein’s general theory of relativity to the test.

TBIRD Communications Payload
The TBIRD communications payload is approximately the size of a tissue box. Credit: Lincoln Laboratory

Advantages of Space-Based Observatories

With Earth-based telescopes, the farthest that two telescopes could be from one another is on opposite sides of the Earth, or about 13,000 kilometers apart. In addition to this maximum baseline distance, Earth-based instruments are limited by the atmosphere, which makes observing shorter wavelengths difficult. Earth’s atmospheric limitations can be overcome by extending the EHT’s baselines and putting at least one of the telescopes in space, which is exactly what the proposed CfA-led Black Hole Explorer (BHEX) mission aims to do.

One of the most significant challenges that comes with this space-based concept is transfer of information. The dataset to produce the first EHT image was so massive (totaling 4 petabytes) that the data had to be put on disks and shipped to a facility for processing. Gathering information from a telescope in orbit would be even more difficult; the team would need a system that can downlink data from the space telescope to Earth at approximately 100 gigabits per second (Gbps) in order to image the desired aspects of the black hole.

Breakthroughs in Data Transfer Technologies

Here is where Lincoln Laboratory comes in. In May 2023, the laboratory’s TeraByte InfraRed Delivery (TBIRD) lasercom payload achieved the fastest data transfer from space, transmitting at a rate of 200 Gbps — which is 1,000 times faster than typical satellite communication systems — from low Earth orbit (LEO).

“We developed a novel technology for high-volume data transport from space to ground,” says Jade Wang, assistant leader of the laboratory’s Optical and Quantum Communications Group. “In the process of developing that technology, we looked for collaborations and other potential follow-on missions that could leverage this unprecedented data capability. The BHEX is one such mission. These high data rates will enable scientists to image the photon ring structure of a black hole for the first time.”

A lasercom team led by Wang, in partnership with the CfA, is developing the long-distance, high-rate downlink needed for the BHEX mission in middle Earth orbit (MEO).

Future Prospects and Technology Development

“Laser communications is completely upending our expectations for what astrophysical discoveries are possible from space,” says CfA astrophysicist Michael Johnson, principal investigator for the BHEX mission. “In the next decade, this incredible new technology will bring us to the edge of a black hole, creating a window into the region where our current understanding of physics breaks down.”

Though TBIRD is incredibly powerful, the technology needs some modifications to support the higher orbit that BHEX requires for its science mission. The small TBIRD payload (CubeSat) will be upgraded to a larger aperture size and higher transmit power. In addition, the TBIRD automatic request protocol — the error-control mechanism for ensuring data make it to Earth without loss due to atmospheric effects — will be adjusted to account for the longer round-trip times that come with a mission in MEO. Finally, the TBIRD LEO “buffer and burst” architecture for data delivery will shift to a streaming approach.

“With TBIRD and other lasercom missions, we have demonstrated that the lasercom technology for such an impactful science mission is available today,” Wang says. “Having the opportunity to contribute to an area of really interesting scientific discovery is an exciting prospect.”

References:

“High Data Rate Laser Communications for the Black Hole Explorer” by Jade Wang, Bryan Bilyeu, Don Boroson, Dave Caplan, Kat Riesing, Bryan Robinson, Curt Schieler, Michael D. Johnson, Lindy Blackburn, Kari Haworth, Janice Houston, Sara Issaoun, Daniel Palumbo, Elliot Richards, Ranjani Srinivasan, Jonathan Weintroub and Dan Marrone, 13 June 2024, Astrophysics > Instrumentation and Methods for Astrophysics.
arXiv:2406.09572

“The Black Hole Explorer: Motivation and Vision” by Michael D. Johnson, Kazunori Akiyama, Rebecca Baturin, Bryan Bilyeu, Lindy Blackburn, Don Boroson, Alejandro Cardenas-Avendano, Andrew Chael, Chi-kwan Chan, Dominic Chang, Peter Cheimets, Cathy Chou, Sheperd S. Doeleman, Joseph Farah, Peter Galison, Ronald Gamble, Charles F. Gammie, Zachary Gelles, Jose L. Gomez, Samuel E. Gralla, Paul Grimes, Leonid I. Gurvits, Shahar Hadar, Kari Haworth, Kazuhiro Hada, Michael H. Hecht, Mareki Honma, Janice Houston, Ben Hudson, Sara Issaoun, He Jia, Svetlana Jorstad, Jens Kauffmann, Yuri Y. Kovalev, Peter Kurczynski, Robert Lafon, Alexandru Lupsasca, Robert Lehmensiek, Chung-Pei Ma, Daniel P. Marrone, Alan P. Marscher, Gary J. Melnick, Ramesh Narayan, Kotaro Niinuma, Scott C. Noble, Eric J. Palmer, Daniel C. M. Palumbo, Lenny Paritsky, Eliad Peretz, Dominic Pesce, Alexander Plavin, Eliot Quataert, Hannah Rana, Angelo Ricarte, Freek Roelofs, Katia Shtyrkova, Laura C. Sinclair, Jeffrey Small, Sridharan Tirupati Kumara, Ranjani Srinivasan, Andrew Strominger, Paul Tiede, Edward Tong, Jade Wang, Jonathan Weintroub, Maciek Wielgus, George Wong and Xinyue Alice Zhang, 13 June 2024, Astrophysics > Instrumentation and Methods for Astrophysics.
arXiv:2406.12917

The BHEX mission concept has been in development since 2019. Technical and concept studies for BHEX have been supported by the Smithsonian Astrophysical Observatory, the Internal Research and Development program at NASA Goddard Space Flight Center, the University of Arizona, and the ULVAC-Hayashi Seed Fund from the MIT-Japan Program at MIT International Science and Technology Initiatives. BHEX studies of lasercom have been supported by Fred Ehrsam and the Gordon and Betty Moore Foundation.
Illuminating the Abyss: Photon Rings and the Future of Black Hole Imaging Read More
China has a $943,000,000 'megaconstellation' plan with 13,000 satellites that will rival Elon Musk's Starlink

China has a $943,000,000 ‘megaconstellation’ plan with 13,000 satellites that will rival Elon Musk’s Starlink

China has a $943,000,000 'megaconstellation' plan with 13,000 satellites that will rival Elon Musk's Starlink

The plan is set to plug some gaps in Starlink’s coverage

China is launching its own satellite ‘megaconstellation’, which is set to rival Elon Musk’s Starlink.

Despite our modern-day technology, will still sometimes have to deal with slow internet connection. First-world problems, I know…

Musk’s SpaceX was the first space tech company to launch low Earth orbit (LEO) satellites in an attempt to solve this problem.

A handful of Starlink satellites were first launched in 2019, positioned just 340 miles above our planet’s surface level. In comparison, geostationary satellites favored by traditional internet providers are only operational at an altitude of around 22,236 miles.

There will one day be more than 40,000 Starlinks in the sky (John Keeble/Getty Images)

There will one day be more than 40,000 Starlinks in the sky (John Keeble/Getty Images)

That’s a staggering difference, and its LEO’s proximity to Earth that gives us more reliable network coverage.

It allows Starlink to improve internet speed and reduce latency levels, while covering larger areas.

Now, China are launching their own so-called megaconstellations, with Shanghai Spacecom Satellite Technology (SSST) raising $943 million (6.7 billion yuan) for a new initiative.

The satellite project in question is dubbed G60 and, like Starlink, uses LEO to beam data back down to us.

Some 12,000 satellites were projected to be launched in 2024, with a total of 12,000 set to be live in total.

The light blue countries have access to Starlink, while dark blue means it's rolling out soon and brown means the service isn't currently available (Starlink/SpaceX)

The light blue countries have access to Starlink, while dark blue means it’s rolling out soon and brown means the service isn’t currently available (Starlink/SpaceX)

Meanwhile, satellite network group China SatNet is also reportedly set to launch its own system, called Guowang, meaning ‘national network.’

Like G60 and Starlink, it aims to provide global broadband internet coverage and support the country’s growing digital economy.

If they really do want to rival Musk, though, then they’re a bit behind.

Starlink already has more than 6,000 satellites in orbit, serving some four million customers across the globe.

There are currently more than 6,000 of their satellites in orbit, accessible in 100 different countries. And SpaceX plans to launch as many as 42,000 Starlinks in the future.

Although China’s new projects can most definitely plug a gap in Starlink’s coverage.

A group of Starlink satellites spotted over Uruguay (MARIANA SUAREZ/AFP via Getty Images)

A group of Starlink satellites spotted over Uruguay (MARIANA SUAREZ/AFP via Getty Images)

Starlink has no operating licence in China, while a number of other countries – like South Africa, Cameroon, and Brazil – has moved to block the service provider.

Last month, Chinese state media said SpaceSail, the company behind the G60 constellation, agreed with Brazilian state-owned group Telebrás to provide satellite communications and broadband internet services over the country.

As the technology battle between the US and China expands, so too do tensions surrounding trade materials.

China just cost the US $34 million a decade after banning rare earth minerals used in EV batteries last month. The shipping of gallium, germanium, antimony and superhard materials will be stopped.

China has a $943,000,000 ‘megaconstellation’ plan with 13,000 satellites that will rival Elon Musk’s Starlink Read More
Yellowstone star makes brutal dig at Kevin Costner following his exit from beloved show

Yellowstone star makes brutal dig at Kevin Costner following his exit from beloved show

Yellowstone star makes brutal dig at Kevin Costner following his exit from beloved show

Luke Grimes starred in Yellowstone alongside Costner from the very beginning of the show

Yellowstone actor Luke Grimes made a bold claim about his former co-star Kevin Costner after he made his exit from the popular Paramount series.

Grimes spoke out about the series as it prepares to launch into its final episodes, bringing the stories of the characters that fans have followed for the last six years to their end.

The actor has been involved with the series since the very beginning, initially starring alongside Costner before news of an alleged conflict between Costner and series creator Taylor Sheridan emerged.

Coster played John Dutton in Yellowstone (Paramount)

Coster played John Dutton in Yellowstone (Paramount)

Yellowstone ended up being placed on hiatus last year as conversations took place behind the scenes, and Costner ultimately announced his departure from the series earlier this year.

Addressing fans in an Instagram post back in June, Costner, who played John Dutton, said: “I want to reach out and let you know that after this long year and a half of working on Horizon and doing all the things that’s required, and thinking about Yellowstone, that beloved series that I love, that I know you love, I just realized that I’m not going to be able to continue season 5B or into the future.

“It was something that really changed me,” he continued. “I loved it. And I know you loved it. And I just wanted to let you know that I won’t be returning, and I love the relationship we’ve been able to develop and I’ll see you at the movies.”

Many fans were left disappointed at the idea of the show without Costner, but now Grimes has shared a different point a view and expressed a hope that everyone would ‘see that it was time’ for Costner’s departure.

Grimes claimed the final episodes were among the 'easiest' to film (Paramount)

Grimes claimed the final episodes were among the ‘easiest’ to film (Paramount)

In an interview with Esquire, he then suggested life was slightly easier on set without the actor, saying: “To be really honest, there was a part of Kevin being gone that meant some of the conflict was gone. Obviously, it didn’t make it super fun to be around. Not pointing any fingers, but it was actually the easiest season we’ve filmed.”

Costner’s departure for the show also meant the end of his character, who was ultimately killed off in the opening episode of season 5 part 2.

The death was revealed to be part of a murder-for-hire plot from Sarah Atwood (Dawn Olivieri), the girlfriend of John’s estranged brother (Wes Bentley), who staged the scene to make it look like John took his own death.

Commenting on the storyline, Yellowstone executive producer Christina Voros told The Hollywood Reporter the death was an ‘incredibly brave’ move by Sheridan.

“I think it is testament to his faith in the characters and the actors who embody them to go, ‘Let’s not make this about the incident. Let’s make this about how these human beings exist in the aftermath.’ That was more interesting to [Taylor] than the incident itself,” she said.

Yellowstone star makes brutal dig at Kevin Costner following his exit from beloved show Read More
Grandmother dies after 'getting trapped by mechanical bed for two days'

Grandmother dies after ‘getting trapped by mechanical bed for two days’

Grandmother dies after 'getting trapped by mechanical bed for two days'

Rosalind Walker passed away on April 3, 2023 at her home in Illinois

On April 3, 2023, Rosalind ‘Roz’ Walker passed away at her home in Illinois, US, surrounded by her family.

And a wrongful death lawsuit – filed in St Louis County – has since claimed her passing resulted from the grandmother allegedly becoming trapped inside her malfunctioning bed.

The lawsuit

The lawsuit – filed by Walker’s daughter Angela Moan – is against retail company Sleep Number which provides ‘innovative mattresses, pillows, and smart beds,’ as per its website and the bed’s manufacturer Leggett & Platt Inc.

Walker is reported by The Post as having purchased a bed from the manufacturer 10 years prior to her passing, the bed allegedly coming with a 25-year warranty.

The lawsuit alleges on March 1 last year, the grandmother’s mattress ‘suddenly lowered itself without warning’ and trapped her against the wall where she remained for a reported two whole days until emergency services visited her home, discovered her and took her to hospital.

The filing states Walker suffered unspecified injuries and after being treated in hospital was moved to a rehabilitation center before returning home, but with hospice care.

It claims Sleep Number and Leggett & Platt Inc ‘did not have adequate instructions or cautionary language in the instructions or on the bed alerting Mrs. Walker not to go between the bed and the wall as she could be trapped’.

The lawsuit is seeking an unspecified amount for medical bills and the suffering Walker’s death has caused loved ones and Walker’s family have paid tribute to her online.

Rosalind Walker passed away at the age of 80 (Elias, Kallal & Schaaf)

Rosalind Walker passed away at the age of 80 (Elias, Kallal & Schaaf)

Commemorating Rosalind Walker

Elias, Kallal and Schaff funeral homes, crematory and cemeteries website states Walker was born on October 29, 1942 in Chicago.

She married her partner on March 24, 1963, however, he sadly passed away in 2009.

“Roz was a Charter member of Resurrection Lutheran Church of Godfrey, IL and a member of Chapter GG of PEO sisterhood. She loved working in her yard, traveling, and playing cards. Roz was very active within the community and was a fierce and loyal friend and will be missed by many,” the site continues.

Walker is survived by her daughter and two grandchildren.

And a spokesperson from Sleep Number has since responded to news of the lawsuit.

The lawsuit claims Walker got trapped by the bed (Getty Stock Images)

The lawsuit claims Walker got trapped by the bed (Getty Stock Images)

Sleep Number’s response

A spokesperson for Sleep Number told The Post: “The suit alleges that a malfunctioning adjustable base purchased in 2014 was a contributing factor in the death of Rosalind Walker.

“We understand that this incident is alleged to have occurred in March 2023; we were notified of the alleged incident after the lawsuit was filed yesterday, December 10.”

“We extend our sincere condolences to the family of Ms Walker for their tragic loss.”

Grandmother dies after ‘getting trapped by mechanical bed for two days’ Read More
Pentagon reveals 'truth' behind mysterious drones above New Jersey believed to be from a 'mothership'

Pentagon reveals ‘truth’ behind mysterious drones above New Jersey believed to be from a ‘mothership’

Pentagon reveals 'truth' behind mysterious drones above New Jersey believed to be from a 'mothership'

The Pentagon has spoken out on the drones that have been spotted in parts of the East Coast

The Pentagon has been forced to deny a congressman’s outlandish claims about the origin of the mysterious drones that have been spotted in New Jersey.

There has been dozens of drone sightings on the East Coast in recent weeks, leaving many people wondering what the aircrafts are doing and where they came from.

With people’s questions in mind, New Jersey Representative, Jeff Van Drew, took it upon himself to give an apparent explanation, insisting that the information was given to him from ‘reliable sources’.

Sharing the so-called ‘real deal’, the lawmaker told Fox News: “I’m on the Transportation Committee, on the Aviation Subcommittee, and I’ve gotten to know people. And from very high sources, very qualified sources, very responsible sources.”

Van Drew went on: “I’m going to tell you… Iran launched a mothership probably about a month ago that contains these drones. That mothership is off the east coast of the United States of America.”

He also said that the drones ‘should be shot down’.

“We are not getting the full deal and the military is on alert with this,” the lawmaker added.

But the Pentagon has now denied that there’s a ‘mothership’ linked to the mysterious drones.

Jeff Van Drew made the outlandish claims to Fox News (Drew Angerer/Getty Images)

Jeff Van Drew made the outlandish claims to Fox News (Drew Angerer/Getty Images)

Speaking on Wednesday (December 11), Pentagon spokesperson Sabrina Singh said in a briefing that there was ‘no evidence these are coming from a foreign entity or the work of an adversary’.

“We’re going to continue to monitor what is happening. But, you know, at no point were our installations threatened when this activity was occurring.” she continued.

Addressing Van Drew’s claims directly, Singh added there’s ‘no truth’ to his allegations.

“There is no Iranian ship off the coast of the United States, and there’s no so-called mothership launching drones towards the United States.” she continued.

Reuters reports that the FBI and New Jersey State police had asked the public to report any information regarding the possible sightings, with the FBI saying: “Witnesses have spotted the cluster of what look to be drones and a possible fixed-wing aircraft.

“We have reports from the public and law enforcement dating back several weeks.”

The Pentagon’s initial assessment had also shown the ‘drones’ weren’t from another country and that US military didn’t take them down because they weren’t deemed to be a threat.

Sabrina Singh said there's no evidence that the drones are from a a foreign entity (Celal Gunes/Anadolu via Getty Images)

Sabrina Singh said there’s no evidence that the drones are from a a foreign entity (Celal Gunes/Anadolu via Getty Images)

The Pentagon’s statement comes just weeks after mysterious drones were spotted near three British airbases – RAF Lakenheath, RAF Mildenhall, and RAF Feltwell – all of which are used by the United States Air Force (USAF).

At the time of the reports in November, the USAF said that it was unsure if the drones were hostile or not, reported BBC News.

Addressing the matter, a spokesperson for USAF in Europe said: “We can confirm that small unmanned aerial systems [UASs] were spotted in the vicinity of and over RAF Lakenheath, RAF Mildenhall and RAF Feltwell.

“The number of UASs fluctuated and they ranged in size/configuration. The UASs were actively monitored and installation leaders determined that none of the incursions impacted base residents or critical infrastructure.

“To protect operational security, we do not discuss our specific force protection measures but retain the right to protect the installation.”

They went on to say that they would ‘continue to monitor our airspace’ and were working with host-national authorities and mission partners to ensure those at the base and its assets were safe.
Pentagon reveals ‘truth’ behind mysterious drones above New Jersey believed to be from a ‘mothership’ Read More