Uncovering the Universe: Why We Just Recently Realized It’s Dark Instead of Bright

Adobe Stock Photo/Phoebe Watts

Set against the vastness of space, our blue planet emerges above the desolate lunar landscape. This iconic photograph, “Earthrise,” was captured by Apollo 8 astronaut Bill Anders on Christmas Eve 1968.

Nearly six decades later, we regard this image as part of our narrative. Yet, envision a different earthrise where space is not a dark backdrop, but a vivid blue, akin to a sunny sky. Odd as it may appear, this was the vision held by many Europeans for centuries.

Our comprehension of the cosmos has evolved significantly over time, influencing how we perceive our place within it. The shift from an earth-centered to a sun-centered universe, along with the transition from a finite to an infinite cosmos, prompted a profound reevaluation of humanity’s role in the grand scheme. The change from a vibrant to a dim universe is equally crucial, yet it remains largely overlooked in our historical narratives.

Recently, through my scholarly work in literary and scientific history, I have sought to trace the timeline of this transformation. At what point did our universe metaphorically turn dark? What did this shift imply for humanity?

Earthrise—a photograph from the moon’s surface in 1968 showcasing the notion that space is dark.

NASA

Reflect on the account given by Domingo González, the hero of Francis Godwin’s 1638 science fiction novel, The Man in the Moone. González travels to the moon in a swan-powered vehicle and notes a scarcity of stars. Even those he does see are dim. He observes, “It was always daytime for some reason, yet the stars appeared faint, similar to the moon’s glow in daylight.” Why are there fewer stars in his experience? Why do they appear washed out? Because, in his narrative, space is akin to the daytime sky, where the sun drowns out the luminosity of stars.

From our viewpoint, González’s reality seems inverted. In his portrayal, daytime reveals our true nature, while night conceals us within Earth’s shadow. Yet, ascending to space at midnight, we would eventually emerge from darkness into eternal daylight.

In Francis Godwin’s The Man in the Moone, protagonist Domingo González embarks for the moon in a swan-powered craft.

Houghton Library

While González omits mention of a shadow, we glimpse it in another early space narrative by John Milton, Paradise Lost. As Milton’s Satan nears Earth, he remarks upon “a whirling canopy / a spreading shadow of the night.” If you visualize pre-modern eras, adding this shadow to your image of earthrise transforms it. A dark cone emerges from the jagged globe, plunging into the azure sky and vanishing beneath the lunar horizon.

Additional authors elucidate why the Universe is imagined as not merely bright, but blue-hued. The prevalent rationale is that the “firmament” was envisioned as blue. Walter Charlton, a contemporary of Milton, remarked this notion was widely shared “by many transcendental thinkers, as well as the average populace.” Observing the daytime sky, they believed they were witnessing the universe’s limit.

The Path to Earthrise

This luminescent universe also manifests in visual art. A comparison with Apollo 8 is particularly pertinent. Hours after capturing earthrise, the crew transmitted radio messages from lunar orbit to Earth. Commander Frank Bowman extended Christmas wishes and recited the biblical creation tale. For the first time, humanity achieved a god-like vantage point of the radiant blue planet glistening against the abyss. In contrast, when pre-modern artists portrayed these scripture moments, they often rendered a dim planet against a bright celestial expanse. To reimagine earthrise, picture one of these shadowed Earths ascending above the lunar surface instead of the iconic “blue marble.”

It was not just poets and artists who envisioned such a realm. Philosophers and scientists also entertained the concept. Aristotle remarked on “the shadow of the earth (termed night).” Two millennia later, Copernicus similarly wrote, “While the rest of the universe is illuminated and radiant, the night signifies nothing but the shadow of the Earth, extending in a cone and culminating at a point.”

This perspective was not unreasonable; early European scholars lacked compelling evidence to argue otherwise, particularly concerning the light-refracting properties of the universe and Earth’s atmosphere. Without such evidence, why suspect that night predominates and day a rarity? What led pre-modern Christians to diverge from millennia of tradition and perceive heaven—not as eternal brightness, but infinite darkness?

A 13th-century manuscript depicting a gray Earth casting a black shadow against a blue universe (left) and a 15th-century manuscript showcasing the newly created Earth as a black marble surrounded by blue cosmos (right).

Heritage Image Partnership Ltd/Alamy; National Library of France

This does not imply that luminous spaces were universally accepted in pre-modern thought. For instance, scholars within the Islamic tradition favored the concept of dark spaces starting in the 9th century, yet this perspective seems to have been less influential in the West. In any case, the notion of a dark universe had to be re-established among 17th-century European thinkers.

During this period, significant advancements in atmospheric science emerged. Notably, the term “atmosphere” was coined in the 17th century, with Walter Charlton among the first to utilize it in English. His view of the universe acts as a transitional development in this narrative: a universe that oscillates between brightness and darkness based on an observer’s orientation towards the sun. Although Charlton described a dark universe, he noted that it was “not nearly as deep blue as many presume,” and filled with countless tiny particles or “atoms,” which he speculated could impact visibility. In contrast, Otto von Guericke, who endorsed the infinite universe and conducted pioneering vacuum experiments, postulated that in an “unblemished” and “void” space, devoid of illuminated objects, we would perceive “nothing but shadows.”

Thereafter, dark space gained traction among European scientists and thinkers informed by these scientific advancements. However, this marks only part of the narrative, as visions of bright spaces lingered in cultural imaginations for centuries.

Fast forward to 1858, when astronomer James Gall envisioned his foray into the void for a Victorian audience, exclaiming, “As I look around me, how peculiar! The heavens are pitch black.” While Gall acknowledged the darkness of space, he doubted the audience’s awareness of this fact. It wasn’t a naive child or uninformed individual believing in a “giant blue sphere,” but the renowned literary historian David Masson in 1880 who clung to this isolated imagery, which persisted well into the 1920s, right at the brink of the Space Age.

Thus, we confront a dual narrative of a decline in our cosmic imagination alongside the unexpected evolution of these ideas. Some of the most striking evidence is found in literature, especially in space travel narratives, which were initially recognized by literary scholars such as C.S. Lewis and more recently John Leonard. Nevertheless, this aspect has yet to receive thorough investigation, and its cultural ramifications remain largely unexamined.

The implications are significant, often concealed in plain sight. Prominent images such as earthrise have reshaped our perceptions of our planet and its environmental context. The view of Earth as “perfect” and “blue” has also rendered it “fragile,” symbolizing the perils of nuclear conflict and climate change, as well as underscoring the call for political unity and ecological stewardship. What is less acknowledged, however, is that this transformation arose not only from a fresh perspective on Earth, but importantly on the vastness surrounding it.

For millennia, the entirety of Earth has been envisioned, represented, and contemplated. Yet, much of it was depicted within brilliant space, eliciting markedly different responses. Hence, the influence of earthrise was indeed more profound than commonly appreciated. The mass circulation of such imagery has obliterated even the faintest remnants of a once-bright universe and firmly imprinted its inversion into collective consciousness. The Earth stands not merely as “blue” or “fragile.” While it may appear thus against the cold, dark expanse surrounding it, it has transitioned into both a scientific reality and a cultural perception.

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Source: www.newscientist.com

This Year, for Better or Worse, the Comet Blazed Bright.

Comet Lemon photographed from northern Italy on October 26, 2025

Marcel Clemens/Alamy

Although no one has officially stated it, 2025 has certainly been an exceptional year for comets. There’s Comet Lemon, discovered in January and making headlines for nine months. Each time I encountered that striking long tail formed by the comet’s solar heat, I was captivated.

In September, C/2025 R2 (SWAN) was discovered, radiantly bright even when near the moon on Halloween, making it easily visible. Then came Comet 3I/Atlas, which gained notoriety after a Harvard astronomer—primarily a cosmologist—identified it as an alien probe.

As a cosmologist who recognizes my limited expertise in comet studies, I fully trust the specialists asserting that Comet 3I/Atlas is not some extraterrestrial object. This isn’t a regret; this comet is still scientifically intriguing. Unlike lemons and SWANs, it hails from beyond our solar system, categorizing Comet 3I/Atlas as an interstellar comet.

Its entry into our solar system offers a thrilling opportunity. While pinpointing its exact trajectory may be unattainable, its composition can reveal a wealth of information about its parent star. Essentially, we can learn about the makeup of an enigmatic star even when its identity remains unknown.

Our expedition with this year’s comet reflects a long historical pattern of human fascination with enigmatic celestial phenomena. Most notably, Halley’s Comet’s passage in 1066 was illustrated in the Bayeux Tapestry, symbolizing the onset of the Norman invasion of England. Nowadays, we understand that humanity is not the universe’s focal point, and the universe lacks a center—but it’s easy to entertain the notion that the comet of 2025 could be conveying a message.

Reflecting on this year, filled with distressing and unfortunate occurrences, it’s tempting to ponder whether these comets hint at an impending apocalypse. The state of science in the United States faces turmoil, as the current administration cuts funding and initiatives (see page 20). Moreover, anti-immigrant sentiments have gained a mainstream foothold in both the United States and the United Kingdom.

As a Black and Jewish queer scientist, and an immigrant’s child, maintaining an open heart daily is a struggle. I recognize that there are those who wish to silence me. Contrary to my previous scientific education, I could interpret the comet as a sign to surrender. Yet, alternative paths exist. As a scientist, I perceive comets as sources of hope. They are breathtaking visual havens. The quest to observe them has fostered community. My astrophotography group eagerly anticipates sharing our experiences. While it’s frustrating to encounter rampant misinformation in various media concerning questions like “Are they aliens?”, I feel grateful that attention is being drawn to these phenomena.

For 2026, my aspirations are immense. Scientifically, I yearn for groundbreaking observations of dark matter. Socially, I aim to ensure that all children have access to essential resources—food, shelter, education, and healthcare—in environments that affirm their identities. While these are monumental dreams, they likely won’t manifest by year’s end. Nevertheless, comets remind us of the vast universe, brimming with marvelous surprises. Just as we strive to discover comets, we must also endeavor to create the better world we desire.

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Source: www.newscientist.com

The AI Bubble is Popping, but AI’s Future Remains Bright

Growing concerns of an AI bubble

CFOTO/Sipa USA/Alamy

Substantial investments in AI are suggesting a global financial bubble that may soon burst, exposing companies and investors to the risk of unmanageable debts unable to be serviced by the scant revenues from current AI applications. But what implications does this have for the future of the technology fueling this financial madness?

Recent warnings have emerged globally about the danger of an AI bubble. The Bank of England, the CEO of JP Morgan Chase, and even OpenAI’s Sam Altman have all cautioned against the current trends. “This isn’t merely a stock market bubble; it encompasses investment and public policy bubbles,” asserts David Edgerton from King’s College London.

The interconnected nature of deals among leading AI firms has raised concerns. Take Nvidia, for instance, which manufactures the GPU chips propelling the AI surge; it recently poured up to $100 billion into OpenAI, while maintaining its own data centers filled with Nvidia chips. Ironically, OpenAI also holds a stake in Nvidia’s competitor, AMD.

According to Morgan Stanley Wealth Management, an estimated $400 billion is spent yearly on data centers, leading to increasing worries about the impending burst of the AI bubble. In the second quarter of this year, the US GDP saw a 3.8% increase, but as Harvard’s Jason Furman points out, excluding data center investment, the actual growth was merely 0.1% in the first half of the year.

Carl Benedikt Frey, a professor at Oxford University, notes that such frenetic deal-making isn’t uncommon in the technology sector’s history. “Overbuilding tends to happen; it unfolded during the railroad boom and again during the dot-com bubble,” he explains.

The concern is whether the fallout from the AI bubble will impact only the companies involved or whether it could ripple through the economy. Frey indicates that many data centers being constructed “off-balance sheet” entail creating new companies to bear the associated risks and potential rewards, usually supported by external investors or banks.

This opacity leaves many unsure about who might be negatively affected. The funding for data centers could be rooted in investments from influential tech billionaires or major banks, and substantial losses might trigger a banking crisis, adding turbulence to the economy. “While a financial crisis isn’t immediately on the horizon, the uncertainties breed potential risks,” Frey comments.

Benjamin Arold, a professor at Cambridge University, states that the crucial factor is the profit-to-company valuation ratio, revealing the disconnect between public perception and the actual financial performance of companies. Such metrics are, he warns, red flags for contemporary tech firms.

“We haven’t seen price levels like this in 25 years; it’s reminiscent of the dot-com bubble,” Arold warns. “It may work out in the end, but investing in it feels risky.”

James Poskett from the University of Warwick argues that the AI sector may face a downturn that could lead to many companies going out of business. However, he believes this doesn’t spell the end for the technology itself. “It’s essential not to conflate that with the notion that the technology itself is flawed or redundant,” Poskett emphasizes. “AI could falter, yet it won’t vanish.”

Poskett suggests we may end up with valuable technology, much like how the collapse of various railroad companies in the past left the legacy of a robust rail system, or how the dot-com bust concluded with an extensive fiber-optic infrastructure.

For consumers, the fallout from the AI bubble could translate to fewer choices, potentially higher costs, and a slower rate of technological advancements. Utilizing an expensive tool like GPT-5 for tasks such as email creation resembles using a sledgehammer to crack a nut and may reveal the concealed costs associated with its use, obscured by the present AI race. “There’s currently a lot of ‘free lunch,’ but eventually, these companies will need to start turning a profit,” Poskett notes.

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Source: www.newscientist.com

Bright Seifert Galaxy’s Ultra-Massive Black Hole Exhibits Signs of “Overeating”

In a new research paper published in Monthly Notices of the Royal Astronomical Society, astronomers from the University of Leicester explain for the first time how the “excessive diet” of fresh material in black holes has led to emissions reaching nearly a third of the speed of light.



This image illustrates Seyfert Galaxy PG1211+143. Image credits: Centre Donna Astromyk destrasbourg/Sinbad/SDSS.

The intense outflow of ionized gases has raised significant concerns at the ESA’s XMM-Newton X-ray observatory since its initial detection by University of Leicester astronomers in 2001, now recognized as a distinctive trait of the luminous active galactic nuclei (AGNs).

Professor Ken Pound and Dr. Kim Page from Leicester remarked:

“The black hole’s size increases with its mass, with a solar mass black hole having a radius of about 3 km.”

“Stellar mass black holes are prevalent across galaxies, often forming from the dramatic collapse of massive stars; however, ultra-massive black holes can be found in the nuclei of almost all galaxies except the smallest external ones.”

In 2014, astronomers undertook a five-week investigation of an ultra-massive black hole in the distant Seyfert Galaxy PG1211+143, located approximately 1.2 billion light-years from the constellation Coma Berenices.

Utilizing ESA’s XMM-Newton Observatory, they observed counter-inflows, accumulating at least 10 Earth masses near the black hole.

In their latest study, they detected a powerful new outflow traveling at 0.27 times the speed of light, initiated shortly thereafter. The gravitational energy released as material is drawn into the black hole is heated to millions of degrees, producing an overwhelming radiant pressure.

“Establishing a direct causal relationship between significant, temporary inflows and the resulting outflows offers an exciting perspective for observing the growth of supermassive black holes through continuous monitoring of the hot relativistic winds linked with new material accretion,” stated Professor Pound.

“PG1211+143 has been the focus of University of Leicester X-ray astronomers using ESA’s XMM-Newton Observatory since its launch in December 1999.”

“Initial findings surprisingly revealed a counterflow of rapid movements, reaching 15% of the speed of light (0.15c), affecting stellar formation (and consequently the growth) of the host galaxy.”

“Subsequent observations have shown that such winds are a common characteristic of bright AGNs.”

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Ken Pounds & Kim Page. 2025. Observations of the Eddington-style outflow from the bright Seyfert Galaxy PG1211+143. mnras 540(3): 2530-2534; doi: 10.1093/mnras/staf637

Source: www.sci.news

Earth becomes visible to the naked eye, shining as bright as Venus

Comet C/2024 G3 (ATLAS) captured on December 31, 2024 using the telescope at Rio Hurtado, Chile

lionel magic

A comet that has surprised astronomers could shine as brightly as Venus in the night sky as it passes Earth in the coming days.

Comet C/2024 G3 (ATLAS) was discovered by NASA’s Asteroid Earth Impact Last Alert System more than 600 million kilometers from Earth in April last year. Astronomers initially thought that the comet would not be able to survive in an orbit so close to the Sun, but subsequent observations showed that the comet was following a different path that would allow it to survive, possibly reaching Earth. It has been suggested that it may even be possible to remain unharmed until the approach of

This new orbit, which takes 160,000 years to complete, will mean the comet will snake its way through the solar system, making it visible to stargazers in the Southern Hemisphere. But for the last part of its journey around the sun, people in the northern hemisphere should also be mostly visible through binoculars.

Observations since the new orbit was proposed have shown the comet to be brighter than expected, which could mean it is breaking up as it approaches the sun. However, the latest observations show that the brightness persists and even increases, which would not be the case if the comet disintegrated.

If C/2024 G3 survives, it could appear very bright in the night sky, with some astronomers predicting its brightness could rival that of Venus, making it one of the brightest comets in decades. I’m doing it.

However, the comet’s exact brightness is unknown. It may be far enough away that it reflects the sunlight and is clearly visible, or it may be washed away by the sunlight and become invisible.

Astronomers have also suggested a phenomenon called forward scatter, where dust from the comet makes it appear brighter than normal, but meteorologist Joe Rao said that’s unlikely. space dot com.

If a comet shines brightly, it will probably reach its maximum level around the time of its closest approach to the Sun. The Central Astronomical Telegraph Office, which aggregates observations from astronomers around the world, predicts that this will occur on January 13 at 10:17 a.m. GMT, with the comet’s closest approach to Earth occurring several hours later. are.

This equates to an approximately three-day viewing period from January 12 to 14 for people in the Northern Hemisphere hoping to catch a glimpse of the comet if it’s bright enough. For people in areas such as the United States and Europe, the best time to see the comet is about 30 minutes before sunrise on January 12, when it should be visible through binoculars about 5 degrees from the sun or directly above the horizon. You should get a second chance around 30 minutes after sunset on January 14th.

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Source: www.newscientist.com

Astronomers Analyze Gas Flow in Uncommonly Bright Infrared Galaxy

Ultraluminous infrared galaxies are the rarest and most extreme star-forming systems and are found only in the distant universe.

Radiative distribution of stars, cold gas, and ionized gas in the unusual HyLIRG Einstein ring PJ0116-24. Image courtesy of Liu others., doi:10.1038/s41550-024-02296-7.

“Ultraluminous Infrared Galaxies (HyLIRGs) are incredibly luminous galaxies illuminated by extremely rapid star formation within their interiors,” said Dr Daizhong Liu from the Max Planck Institute for Extraterrestrial Physics and his colleagues.

“Previous studies had suggested that such extreme galaxies must have arisen through galactic mergers.”

“The collisions of these galaxies are thought to create regions of dense gas that trigger rapid star formation.”

“However, isolated galaxies could also become HyLIRGs through internal processes alone if star-forming gas flows rapidly toward the galaxy's center.”

In the new study, the astronomers focused on a gravitationally lensed HyLIRG galaxy known as PJ0116-24.

“PJ0116-24 is so distant that it took its light about 10 billion years to reach Earth,” the researchers said.

“By chance, the foreground galaxy acts as a gravitational lens, bending and magnifying the light from the background galaxy, PJ0116-24, and directing it towards the Einstein ring.”

“This precise configuration of space allows us to magnify very distant objects and see them with a level of detail that is very difficult to achieve any other way.

The researchers used ESO's Very Large Telescope (VLT) and the Atacama Large Millimeter/submillimeter Array (ALMA) to study the motion of gas within PJ0116-24.

“ALMA tracks the cold gas which appears blue here, while the VLT with its new High Resolution Imaging Spectrograph (ERIS) tracks the warm gas which appears red,” the researchers say.

“Thanks to these detailed observations, we now know that the gas in this extreme galaxy rotates in an organized manner, rather than the chaotic state expected after a galaxy collision. A stunning result!”

“This convincingly shows that a merger is not necessarily required for a galaxy to become a HyLIRG.”

Team paper Published in the journal Natural Astronomy.

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D. Liu othersA detailed study of a rare, ultra-luminous rotating disk in a 10 billion year old Einstein ring. Nat AstronPublished online July 15, 2024; doi: 10.1038/s41550-024-02296-7

Source: www.sci.news

Indie Developers Shine Bright: Summer Game Fest Showcases Innovation Beyond AAA titles | Games

IThere's been a lot of speculation regarding the outlook for the games industry in 2024. Following a surge of investment during the pandemic, the industry experienced a temporary boost in growth as people sought entertainment and social interaction while adhering to safety measures at home. However, this year has seen a correction, with studios and companies that expanded too rapidly now scaling back, leading to layoffs and studio closures. Job opportunities for developers have decreased, and games that faced delays due to the pandemic are taking longer to release, resulting in fewer titles compared to the previous year.

The Summer Game Fest, which has taken the place of E3 in Los Angeles, reflects this industry slowdown. What was once a grand trade show is now a more modest event held in smaller venues away from the main convention center. The shift from elaborate press conferences to online livestreams signifies a change in the industry landscape. However, amidst this decline, there is a bright spot in the success of indie games.

Indie games like Palworld, Helldivers 2, and Hades II have emerged as top sellers on platforms like Steam, showcasing the creativity and innovation present in the indie gaming scene. In contrast, big-budget blockbusters from major publishers are facing challenges, with titles like Redfall and Suicide Squad receiving mixed reactions. The industry’s focus on franchised games and live service models is leading to a lack of fresh ideas and risks being taken.

UFO 50, a collection of 50 games. Photo: Mossmouth

However, the indie gaming scene is thriving, with a multitude of creative and unique games being showcased at events like the Summer Game Fest. Titles like UFO 50, Tales of the Shire, and Fear the Spotlight offer players fresh experiences and showcase the diversity of the indie game market. As the industry shifts towards more indie success stories, there is hope for a resurgence of innovative and original content.

While the gaming industry’s major players continue to rely on established franchises and blockbuster titles, it is the indie developers who are driving forward with new ideas and creative approaches. With initiatives like Outersloth supporting indie developers and new entrants like Blumhouse entering the gaming space, there is a sense of revitalization and excitement surrounding indie games.

As the industry evolves, it is clear that the future of gaming lies beyond the traditional giants. With a global community of players and creators, the possibilities for innovation and growth are endless. While the big names may dominate headlines, it is the indie scene that is truly pushing boundaries and shaping the future of gaming.

What to Play

Star Wars: Hunters. Photo: LucasFilm Games/Zynga

For a fresh gaming experience, try out Star Wars: Hunters on platforms like the Nintendo Switch and smartphones. This team-based arena shooter offers diverse characters from the Star Wars universe and engaging gameplay mechanics. With a focus on intuitive controls and immersive visuals, this game is a must-try for Star Wars fans and gamers alike.

Available on: Nintendo Switch, iPhone, Android
Estimated play time: 20+ hours

What to Read

No guns in sight… Catto's Post Office is one of the cosy titles featured on Wholesome Direct. Photo: Inn Shambles Studios

What to click on

Question Block

Elden Ring…can't swim. Photo: Bandai Namco

This week's Question Block explores the dilemma of how video games handle water-related challenges and the consequences of immersion versus gameplay mechanics. The debate over drowning animations and failure states in games highlights the complexities of creating authentic yet engaging gaming experiences.

Whether a game opts for realism or streamlined gameplay, the approach to water mechanics can shape the player’s experience and immersion in the virtual world. As the industry evolves, designers face the challenge of balancing authenticity with player engagement to deliver memorable and enjoyable gaming experiences.

For more insights into game design and industry trends, stay tuned to Question Block and other engaging content related to the evolving world of video games.

Source: www.theguardian.com

Hubble Observes Bright Blue Compact Galaxy

Dazzling new photos from the NASA/ESA Hubble Space Telescope show the brilliant blue compact galaxy ESO 185-IG013 in the constellation Telescope.

This Hubble image shows ESO 185-IG013, a brilliant blue compact galaxy located approximately 260 million light-years away in the constellation Telescopium. Image credit: NASA / ESA / R. Chandar, University of Toledo / Gladys Kober, NASA and Catholic University of America.

ESO 185-IG013 is located about 260 million light-years away in the small constellation Telescopium in the south.

Also known as LEDA 63618, this galaxy is classified as a luminescent blue compact galaxy (BCG).

All stars in ESO 185-IG013 have a combined mass of more than 7 billion solar masses.

“BCG is a nearby galaxy that exhibits intense bursts of star formation,” Hubble astronomers said in a statement.

“It is unusually blue in visible light, distinguishing it from other high starburst galaxies that emit more infrared light.”

“We study BCG because it provides a relatively close equivalent to galaxies in the early universe.”

“This means BCG can help us learn about the formation and evolution of galaxies as they may have occurred billions of years ago.”

Astronomers imaged ESO 185-IG013 at ultraviolet, visible, and infrared wavelengths, revealing details about its past.

“There are hundreds of young star clusters in our galaxy, many of which are younger than 100 million years,” the astronomers said.

“Many star clusters are only 3.5 million years old – relatively infants compared to the time scale of our universe.”

“Scientists predict that many of these youngest clusters will not survive because young clusters often outgas so much that they can disappear.”

“The large number of young star clusters indicates that ESO 185-IG013 was part of a recent galaxy collision and merger.”

“Disturbances in the galaxy's structure, likely caused by intense interactions between gas and dust during the collision, are another sign.”

“This merger provided the system with large amounts of fuel for star formation, which continues today.”

“ESO 185-IG013 also contains a tidal shell, and the diffuse light surrounding its bright center is a common signal of galaxy mergers,” the researchers said.

“We think that in galaxy mergers, the smaller of the two interacting galaxies is blocked by the larger galaxy and loses most of its material.”

“This causes matter to be ejected and then pulled back in by the gravity of the larger galaxy.”

“The dense region where material rearranges is called a shell, and it contains many star clusters. In addition to the shell, ESO 185-IG013 boasts a tail of gas to the northeast.”

Source: www.sci.news