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Black Holes

A Thread of Hot Gas: Unveiling the Hidden Matter of the Cosmos

Astronomers have uncovered a colossal, searing-hot filament of gas linking four galaxy clusters in the Shapley Supercluster a discovery that could finally solve the mystery of the Universe s missing matter. This giant thread, 10 times the mass of the Milky Way and stretching 23 million light-years, is one of the best confirmations yet of what cosmological simulations have long predicted: that vast, faint filaments connect the Universe s largest structures in a cosmic web.

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The discovery of a massive thread of hot gas connecting four galaxy clusters has sent shockwaves throughout the scientific community. This filament, which clocks in at over 10 million degrees, is a staggering 10 times the mass of the Milky Way and stretches diagonally away from us through the Shapley Supercluster for an astonishing 23 million light-years.

Astronomers have long searched for this elusive matter, which makes up over one-third of the “normal” matter in the local Universe. This missing material has been hiding in plain sight, woven into a vast network of filaments that underpin the structure of everything we see around us – the cosmic web.

The European Space Agency’s XMM-Newton and JAXA’s Suzaku X-ray space telescopes have made this groundbreaking discovery possible by combining their unique capabilities. XMM-Newton pinpointed contaminating sources of X-rays, while Suzaku mapped the filament’s faint light over a wide region of space.

“This finding is a game-changer for our understanding of the cosmos,” says lead researcher Konstantinos Migkas of Leiden Observatory in the Netherlands. “For the first time, our results closely match what we see in our leading model of the cosmos – something that’s not happened before. It seems that the simulations were right all along.”

The filament is a crucial piece in the puzzle of the cosmic web, and its discovery has significant implications for our understanding of the Universe. As well as revealing a huge and previously unseen thread of matter running through the nearby cosmos, this finding shows how some of the densest and most extreme structures in the Universe – galaxy clusters – are connected over colossal distances.

“This research is a great example of collaboration between telescopes, and creates a new benchmark for how to spot the light coming from the faint filaments of the cosmic web,” adds Norbert Schartel, ESA XMM-Newton Project Scientist. “More fundamentally, it reinforces our standard model of the cosmos and validates decades of simulations: it seems that the ‘missing’ matter may truly be lurking in hard-to-see threads woven across the Universe.”

The study of the cosmic web is an ongoing effort, with ESA’s Euclid mission launched in 2023 to explore its structure and history. The mission is also digging deep into the nature of dark matter and energy – neither of which have ever been observed, despite accounting for a whopping 95% of the Universe – and working with other dark Universe detectives to solve some of the biggest and longest-standing cosmic mysteries.

Astrophysics

Harnessing the Power of Black Holes: A Tiny Spacecraft’s Quest to Rewrite Physics

A visionary plan proposes sending a paperclip-sized spacecraft, powered by Earth-based lasers, to a nearby black hole within a century. Led by astrophysicist Cosimo Bambi, the mission would test the limits of general relativity and explore the mysteries of event horizons. While current technology can t yet achieve it, advancements in nanocraft design, laser propulsion, and black hole detection could make the journey possible within decades, potentially rewriting the laws of physics as we know them.

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The possibility of sending a tiny spacecraft to a nearby black hole has sparked excitement among astrophysicists. Cosimo Bambi, an expert on black holes, has outlined the blueprint for such a mission in the journal iScience. If successful, this century-long journey could revolutionize our understanding of physics and the laws governing space and time.

Bambi believes that with advancements in technology, it’s not entirely impossible to achieve this feat. The first challenge lies in finding a black hole close enough to target. Previous knowledge suggests there might be one lurking 20-25 light-years from Earth, but detecting it won’t be easy due to their invisible nature. Instead, scientists study them by observing the effects they have on nearby stars or distortions in light.

New techniques for discovering black holes may lead to finding a nearby one within the next decade. Once identified, the next hurdle is getting there with a spacecraft that can withstand the journey. Bambi proposes using nanocrafts – gram-scale probes consisting of a microchip and light sail – accelerated by Earth-based lasers to a third of the speed of light.

At this pace, the craft could reach a black hole 20-25 light-years away in about 70 years, with data gathering taking another two decades to get back to Earth. This would make the total mission duration around 80-100 years. Upon reaching the black hole, researchers can run experiments to answer pressing questions like: does it truly have an event horizon? Do the rules of physics change near a black hole? And does Einstein’s theory of general relativity hold under extreme conditions?

Bambi acknowledges that creating such a spacecraft is currently beyond our capabilities and would require significant advancements in technology. However, with advancements in funding and technological progress over the next 30 years, he believes it may be possible to make this vision a reality.

As Bambi notes, people once thought detecting gravitational waves or observing black hole shadows was impossible, but we achieved those milestones within a century. This work highlights the power of human ingenuity and our relentless pursuit of understanding the universe’s secrets.

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Astrophysics

A Star’s Second Act: Uncovering the Secrets of Black Hole Encounters

This is the first confirmed case of a star that survived an encounter with a supermassive black hole and came back for more. This discovery upends conventional wisdom about such tidal disruption events and suggests that these spectacular flares may be just the opening act in a longer, more complex story.

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The discovery of a star that survived an encounter with a supermassive black hole and came back for more has left astronomers stunned. For decades, scientists have observed spectacular flares caused by stars falling onto these cosmic monsters, only to be destroyed in the process. However, a team of researchers from Tel Aviv University has made a groundbreaking finding: one such flare, named AT 2022dbl, was repeated nearly two years after its initial occurrence, suggesting that at least part of the star survived.

Led by Dr. Lydia Makrygianni and Prof. Iair Arcavi, the study published in the Astrophysical Journal Letters reveals that this flare might not have been a full stellar disruption as previously thought. Instead, it could be a result of the partial destruction of the star, with much of its material surviving to come back for a second, nearly identical passage.

The implications of this finding are significant. If future flares from the same location occur at regular intervals, it would suggest that these events might not be one-off occurrences but rather part of a more complex and dynamic process. “This discovery upends conventional wisdom about such tidal disruption events,” says Prof. Arcavi. “We’ll have to re-write our interpretation of these flares and what they can teach us about the monsters lying in the centers of galaxies.”

The study’s findings also challenge long-held assumptions about black holes, which are notoriously difficult to study due to their complete darkness. By observing the aftermath of a star’s encounter with a supermassive black hole, scientists have gained valuable insights into these enigmatic objects.

As researchers continue to investigate this phenomenon, they may uncover even more secrets about the complex interactions between stars and supermassive black holes. The question now is: will we see a third flare after two more years, in early 2026?

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Black Holes

Radar on NASA’s Europa Clipper Mission Successfully Conducts First Big Test

NASA’s Europa Clipper spacecraft just aced a key radar test while flying past Mars, proving its ability to detect structures beneath planetary surfaces—something that couldn’t be tested on Earth. The radar, known as REASON, will eventually be used to explore Europa, an icy moon of Jupiter believed to harbor a subsurface ocean.

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The NASA Europa Clipper mission has achieved a significant milestone by successfully testing its Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) instrument during a flyby of Mars in March. The test, which was impossible to conduct on Earth due to the scale and complexity of the radar system, aimed to determine the radar’s readiness for the mission at Jupiter’s moon Europa.

The REASON instrument, which will “see” into Europa’s icy shell, may have pockets of water inside, uses two pairs of slender antennas that jut out from the solar arrays, spanning a distance of about 58 feet (17.6 meters). This unusual radar setup for an interplanetary spacecraft was designed to catch as much light as possible at Europa, which receives only about 1/25th the sunlight as Earth.

During the Mars flyby, REASON sent and received radio waves for about 40 minutes, collecting a wealth of data that will help scientists understand how the ice may capture materials from the ocean and transfer them to the surface of the moon. The instrument’s performance was deemed successful, with engineers able to collect 60 gigabytes of rich data.

The Europa Clipper mission’s primary goal is to determine the thickness of the ice shell on Europa and its interactions with the ocean below. The REASON radar will play a crucial role in achieving this objective, providing scientists with valuable insights into the moon’s composition and geology. With the success of the REASON test, the mission is now one step closer to unlocking the secrets of Jupiter’s icy moon and potentially discovering habitable worlds beyond our planet.

The Europa Clipper spacecraft is currently on its journey to reach Europa, which will take approximately 1.8 billion miles (2.9 billion kilometers) and include a gravity assist using Earth in 2026. The mission is managed by Caltech, led by NASA’s Jet Propulsion Laboratory, and includes partners such as the Johns Hopkins Applied Physics Laboratory and NASA’s Science Mission Directorate.

As scientists continue to analyze the data from the REASON test, they are exercising their skills and preparing for the detailed exploration of Europa that will take place in the future. The mission has the potential to revolutionize our understanding of the solar system and provide new insights into the astrobiological potential of habitable worlds beyond Earth.

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