Hubble Captures Stunning Images of Star-Forming Clouds in Nearby Dwarf Galaxy

Explore the stunning new image captured by the NASA/ESA Hubble Space Telescope, showcasing a section of the N159 star-forming complex located in the Large Magellanic Cloud, a dwarf galaxy approximately 160,000 light-years away from Earth.



This breathtaking Hubble image portrays N159, a vibrant star-forming complex in the Large Magellanic Cloud. Image credit: NASA / ESA / Hubble / R. Indebetouw.

N159 stands as one of the most colossal molecular clouds within the Large Magellanic Cloud, making it a noteworthy member of our cosmic neighborhood – the Milky Way galaxy.

Positioned at the southwestern edge of the renowned Tarantula Nebula, N159 spans over 150 light-years across.

The newly released Hubble image captures only a fraction of the expansive N159 complex.

“A dense cloud of cold hydrogen gas predominates the scene, creating a complex array of ridges, cavities, and luminescent filaments,” stated Hubble astronomers.

“Within these thick clouds, newly formed stars begin to blaze, their intense radiation illuminating the surrounding hydrogen in a striking crimson hue.”

“The brightest zones signify the presence of hot, massive young stars whose vigorous stellar winds and energetic light reshape the surrounding space.”

“These powerful forces carve out bubble-like formations and hollow cavities within the gas, clearly illustrating the effects of stellar feedback.”

“Dark clouds in the foreground glow thanks to a new star shining from behind.”

“The illuminated clouds and intricate bubbles reveal the dynamic interplay between star formation and the primordial matter from which stars arise, capturing the perpetual cycles of creation and transformation within this neighboring galaxy.”

Source: www.sci.news

Bolivian Fossil Site Captures Thousands of Cretaceous Dinosaur Footprints, Tail Marks, and Swim Trails

The Carreras Pampas archaeological site within Bolivia’s Toro Toro National Park has documented 1,321 tracks and 289 isolated footprints, totaling 16,600 theropod dinosaur footprints. Additionally, 280 swim tracks have been identified, amounting to 1,378 swim tracks in total. Some of the tracks include tail traces.



Dinosaur footprints at the Carreras Pampas Stadium in Bolivia’s Toro Toro National Park. Image credit: Esperante et al., doi: 10.1371/journal.pone.0335973.

Bolivia boasts one of the most comprehensive and diverse records of dinosaur footprints globally, covering the Triassic, Jurassic, and Cretaceous periods.

Despite the abundance of track sites, there has been limited scientific research published.

A recent study led by paleontologist Raul Esperante from the Institute of Geosciences, along with his colleagues, has documented an extraordinary variety of dinosaur footprints at the Carreras Pampas site in Toro Toro National Park.

In nine different study areas, the research team uncovered 16,600 footprints left by three-toed theropod dinosaurs from the late Cretaceous.

These footprints vary in size from small (less than 10 cm) to large (over 30 cm) and capture a range of dinosaur behaviors, including running, swimming, tail dragging, and abrupt turns.

“The waist height of most (80%) of the trackmakers was between 65 cm and 1.15 meters, with a significant portion measuring between 75 cm and 1.05 meters,” stated the paleontologist.

“Interestingly, very few trackmakers exceeded 1.25 meters in height.”

The majority of these footprints are oriented approximately northwest to southeast, and the sediments retain ripple marks, indicating that these dinosaurs traversed ancient shorelines.

“The Carreras Pampas track set a new world record for the number of individual dinosaur footprints, continuous tracks, tail marks, and swimming marks,” the researchers noted.

“This exceptional frequency suggests it was a heavily trafficked area, and the parallel alignment of some footprints may imply groups of dinosaurs traveled together.”

“Numerous more footprints at this site and other locations in Bolivia remain to be studied,” they added.

“This site offers a remarkable glimpse into the region’s past. It reveals not only how many dinosaurs inhabited the area but also their behaviors during migration.”

“It’s truly incredible to work here, as the ground is covered with dinosaur footprints wherever you look.”

The team’s findings were published in the online journal PLoS ONE.

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R. Esperante et al. 2025. Morphology, preservation, and taphonomy of dinosaur footprints, tail prints, and swim tracks in the world’s largest athletic arena: Carreras Pampas, Toro Toro National Park, Bolivia (Upper Cretaceous). PLoS One 20 (12): e0335973; doi: 10.1371/journal.pone.0335973

Source: www.sci.news

Psyche Captures Sight of Interstellar Comet 3I/ATLAS

NASA’s Psyche spacecraft has obtained fresh images of 3I/ATLAS, marking it as the third astronomical object and the second comet observed from outside our solar system.



Psyche secured four observations of 3I/ATLAS over an 8-hour period on September 8 and 9, 2025. Image credit: NASA/JPL-Caltech/ASU.

3I/ATLAS was found on July 1, 2025, by the ATLAS survey telescope located in Rio Hurtado, Chile.

The orbits of interstellar comets represent the most dynamically extreme pathways of any astronomical object recorded within our solar system.

Known also as C/2025 N1 (ATLAS) and A11pl3Z, 3I/ATLAS reached its closest point to the Sun on October 30, 2025.

The latest images of the comet were captured during an eight-hour window on September 8 and 9, 2025, when 3I/ATLAS was roughly 53 million kilometers (33 million miles) away from NASA’s Psyche spacecraft.

“The observations collected by the mission’s multispectral imager will assist in refining the trajectory of 3I/ATLAS,” stated members of the Psyche team.

“Psyche’s multispectral imager consists of a pair of identical cameras fitted with filters and telephoto lenses to photograph the surface of the metal-rich asteroid Psyche across various wavelengths of light.”

“During these observations, Comet 3I/ATLAS was moving away from the spacecraft, but the imager’s sensitivity to the comet’s reflected sunlight allowed for accurate tracking of the object.”

The recent observations further illuminate the faint coma—a cloud of gas and dust—surrounding 3I/ATLAS’ core, which is a frozen mixture of ice and rock.

“Psyche will collaborate with numerous other NASA missions to track the positions of comets over time, aiding astronomers in comprehending the movement of such objects within our solar system,” researchers stated.

“Though comets do not pose a direct threat to Earth, NASA’s space missions contribute to ongoing efforts to discover, monitor, and better understand objects in our Solar System.”

Source: www.sci.news

Mars Reconnaissance Orbiter Captures Close-Up Image of Interstellar Comet 3I/ATLAS

Exciting new images from High-Resolution Image Science Experiment onboard NASA’s Mars Reconnaissance Orbiter will enable astronomers to refine their estimates regarding the size of 3I/ATLAS, the third known interstellar object that has passed through our solar system.



This image of 3I/ATLAS was captured by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter on October 2, 2025. Credit: NASA / JPL-Caltech / University of Arizona.

On October 2, 2025, the Mars Reconnaissance Orbiter (MRO) observed 3I/ATLAS from approximately 30 million km (19 million miles) away.

The MRO team utilized the High-Resolution Imaging Science Experiment (HiRISE), which typically focuses on the Martian surface.

By maneuvering, the spacecraft can direct its camera toward other celestial objects. This method was previously employed in 2014 when HiRISE collaborated with MAVEN to examine the comet Siding Spring.

“Observations of interstellar objects are still infrequent, so each time we learn something new,” noted Dr. Shane Byrne, HiRISE principal investigator and researcher at the University of Arizona.

“We were fortunate that 3I/ATLAS came close to Mars.”

Captured at a resolution of about 30 km (19 miles) per pixel, 3I/ATLAS appears as a pixelated white sphere in the HiRISE images.

“This sphere is a cloud of dust and ice, referred to as a coma, that the comet emits as it travels past Mars,” the researchers added.

Further analysis of HiRISE images could assist scientists in establishing an upper limit on the size of a comet’s core, composed of ice and dust.

The images might also uncover properties of particles known as comas within the comet’s atmosphere.

Ongoing scrutiny of the images may reveal nuclear fragments and gas jets expelled as comets disintegrate over time.

“One of MRO’s greatest contributions to NASA’s Mars research is its ability to observe surface phenomena that only HiRISE can detect,” explained Dr. Leslie Tampali, MRO’s project scientist and a research scientist at NASA’s Jet Propulsion Laboratory.

“This opportunity allows us to study passing space objects.”

“Thanks to NASA’s versatile fleet of spacecraft throughout our solar system, we can continue to observe this dynamic entity from unique perspectives,” stated Georgia Tech researcher Professor James Ray, a HiRISE co-investigator.

“All three prior interstellar objects exhibit significant differences from one another and from typical Solar System comets, making every new observation incredibly valuable.”

“Being able to observe a visitor from another star system is extraordinary in itself,” remarked Dr. Tomás Díaz de la Rubia, senior vice president for research and partnerships at the University of Arizona.

“Doing so from a University of Arizona-led instrument orbiting Mars adds to its remarkable nature.”

“This moment highlights the ingenuity of our scientists and the lasting impact of this university’s leadership in space exploration.”

“HiRISE exemplifies how discovery tools can benefit both science and the public interest.”

Source: www.sci.news

Hubble Captures Bizarre Spiral Galaxy: NGC 1511

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured a remarkable image of the barred spiral galaxy NGC 1511.



This Hubble image features the barred spiral galaxy NGC 1511, located approximately 50 million light-years away in the constellation Hydra. Image credit: NASA / ESA / Hubble / D. Tilker.

NGC1511 resides in the constellation Hydra, about 50 million light-years from our planet.

This spiral galaxy was discovered by British astronomer John Herschel on November 2, 1834.

NGC 1511, also known as ESO 55-4, IRAS 03594-6746, or LEDA 14236, is a principal member of a small galaxy group known as the NGC 1511 Group.

“Like many galaxies, NGC 1511 doesn’t navigate through space alone,” stated Hubble astronomers.

“Instead, it exists alongside a pair of smaller galactic companions known as NGC 1511A and NGC 1511B. Both companions lie outside the scope of this Hubble image.”

“NGC 1511B is the nearest neighbor to NGC 1511, and the two galaxies have likely collided in the past,” researchers remarked.

“A thin filament of hydrogen gas links them, and NGC 1511B is elongated and warped due to this collision.”

Astronomers have also discovered signs indicating that NGC 1511 once had another small companion galaxy that has since been completely annihilated.

“These disruptions have impacted NGC 1511 as well,” the researchers added.

“This galaxy has undergone explosive star formation, and its disk displays unusual loops and plumes that may suggest previous interactions with nearby galaxies.”

“We are utilizing Hubble’s precise observations of NGC 1511 to analyze star clusters nestled within its dusty gas, aiming to comprehend how material circulates from interstellar clouds to stars and back.”

Source: www.sci.news

Video Captures Orcas Preying on Great White Sharks and Consuming Their Livers

Certain killer whales have a preference for liver, particularly that of great white sharks.

A video captured by Mexican scientists demonstrates how an astute whale targets the apex predator’s fatty organs.

Researchers documented two killer whale hunts in the Gulf of California, one in 2020 and the other in 2022. The footage reveals a group of great white sharks flipping a young shark onto its back, disorienting it, before slicing open its side to extract its liver. The findings from this video study were published on Monday in Frontiers in Marine Science.

In one notable scene, all members of the shark clan feasted on the pink liver fat while the remainder of the shark’s body remained submerged in the ocean depths. A sea lion was seen lurking nearby, seemingly hoping to steal a meal, but orcas released bubbles to ward it off.

Marine biologist and documentarian Eric Higuera Rivas, who filmed the hunt from a nearby boat, initially did not grasp the significance of the footage until he began editing.

“On the monitor, we noticed the shark’s liver hanging out, already dislodged. Moments later, the shark emerged with the liver in its mouth,” recounted Higuera Rivas, a co-author of the study. “I was astonished to learn it was a great white shark. I could hardly believe it.”

Heather Bowlby, a researcher from Fisheries and Oceans Canada not involved in the study, noted that the footage serves as a strong reminder that even apex predators need to stay vigilant.

“We typically view great white sharks as the pinnacle of the food chain,” she stated. “It’s always beneficial to remind them that they can also be prey.”

Higuera Rivas and his team indicated that the hunt appeared to involve members of the same group of killer whales, which they have designated as Moctezuma pods. This pod regularly patrols the Baja California coast, primarily hunting elasmobranchs, including sharks and whales. Higuera Rivas has been monitoring these pods and recording their behaviors for over a decade, noting their adaptations based on the species they target.

Previously, evidence of killer whales preying on great white sharks was limited to South Africa, where they have been known to extract livers and wash the remains ashore.

Alison Towner, a marine biologist at Rhodes University specializing in the South African phenomenon, stated that while behaviors in Mexico and South Africa are similar, they are not identical; Mexican killer whales typically target younger sharks, whereas their South African counterparts focus on adults.

Towner indicated that individual killer whale pods likely learned their hunting strategies independently.

“Observing this behavior in Mexico implies that specific groups of killer whales have developed distinct methods for hunting sharks,” she mentioned via email. “Even though the same organs are the target, the manner in which they are approached varies from what we have documented in South Africa, indicating group-specific learning.”

A new study reveals that Mexican killer whales have discovered a vulnerability in great white sharks.

“When flipped over, a shark enters a state known as tonic immobility,” explained study co-author Francesca Pancaldi, a shark researcher at the National Institute of Marine Sciences. “They become immobilized, akin to a catatonic state. They simply freeze.”

The liver, a nutrient-rich and fatty organ, comprises about a quarter of a shark’s body, delivering “a substantial amount of energy,” he added.

Researchers from both South Africa and Mexico concurred that this hunting behavior is likely not new to killer whales. What has changed for scientists is the advancement of drone technology, which has enhanced the ability to observe and document these hunting events.

“I believe this has been occurring for centuries, but it’s challenging to witness such events,” Pancaldi remarked.

However, she also mentioned that climate changes may have heightened interactions between great white sharks and the octopus pods.

“In fact, we have noticed a growing presence of great white sharks in the Gulf of California over the past decade,” Pancaldi noted, explaining that the species is particularly sensitive to changes in ocean temperatures linked to weather patterns such as El Niño.

According to Towner, scientists in South Africa began observing attacks by killer whales on great white sharks nearly a decade ago. Such predatory behavior has caused great whites to abandon their usual feeding, resting, and breeding spots, referred to as assemblages.

“As a result of repeated predation, great whites have entirely vacated their traditional core gathering sites,” Towner explained. “Many sharks may have relocated offshore or to less monitored regions, which is reshaping coastal ecosystems.”

Following the exodus of the sharks, populations of Cape fur seals and sevengill sharks have surged, leading to conflicts with the primary prey species, such as small fish and smaller sharks, according to the report. This study was published in Frontiers in Marine Science earlier this year.

Mr. Towner noted that only two adult male killer whales, referred to as Port and Starboard, were responsible for the frequent attacks on great white sharks in South Africa. This predation puts pressure on great whites, which have slow growth and reproductive rates, and a similar situation could develop in Mexico if this behavior becomes more prevalent.

Source: www.nbcnews.com

Hubble Space Telescope Captures NGC 3370 Observations

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured new images of the nearly face-on spiral galaxy NGC 3370.



This Hubble image illustrates spiral galaxy NGC 3370, located approximately 90 million light-years away in the constellation Leo. Image credits: NASA / ESA / Hubble / A. Riess / K. Noll.

NGC 3370 is situated in the constellation Leo, roughly 90 million light-years from Earth.

This galaxy, also known as the Silverado Galaxy, IRAS 10444+1732, LEDA 32207, and UGC 5887, is nearly comparable to our Milky Way in both diameter and mass.

Discovered on March 21, 1784, by German-British astronomer William Herschel, NGC 3370 was the first of its kind to be identified.

Together with NGC 3447 and NGC 3455, it forms part of the NGC 3370 galaxy group.

NGC 3370 contains two types of celestial objects that astronomers find valuable for measuring distances to far-off galaxies: Cepheid variable stars and Type Ia supernovae.

“Cepheid variable stars undergo changes in both size and temperature during their pulsations,” Hubble astronomers explained in a statement.

“Consequently, the brightness of these stars fluctuates over timescales of days to months.”

“This variation reveals a key relationship: the brighter a Cepheid variable star, the slower its pulsation.”

“By timing the pulsation cycle of a Cepheid variable star, we can ascertain its true brightness.”

“When combined with observations of its apparent brightness from Earth, this data enables us to calculate the distance to the star and its galaxy.”

“Type Ia supernovae allow for distance measurements through a single explosive event, as opposed to periodic brightness changes.”

“These explosions occur when a star’s dead core reignites due to a sudden surge of nuclear fusion.”

“They reach similar peak brightness levels, akin to those of Cepheid variable stars, and knowing the intrinsic brightness of a supernova allows us to determine its distance.”

“The observation of both Cepheid variable stars and Type Ia supernovae is crucial for accurately gauging how quickly our universe is expanding.”

Source: www.sci.news

Hubble Captures Stunning Image of Dusty Spiral Galaxy NGC 7496

NGC 7496 is a barred spiral galaxy situated roughly 24 million light-years away in the Taurus constellation.



This Hubble image captures barred spiral galaxy NGC 7496 in the constellation Hyuri, located approximately 24 million light-years away. Image credits: NASA / ESA / Hubble / R. Chandar / J. Lee / PHANGS-HST team.

NGC 7496 was discovered by British astronomer John Herschel on September 5, 1834.

The galaxy is also identified as ESO 291-1, LEDA 70588, and IRAS 23069-4341, and spans approximately 70,000 light-years in diameter.

NGC 7496 belongs to the NGC 7582 group, which comprises about 10 large galaxies.

This galaxy is classified as a Type II Seyfert galaxy, notable for a high star formation rate.

At its center lies an active galactic nucleus containing a supermassive black hole primarily consuming gas.

According to Hubble astronomers, “Hubble observed NGC 7496 for the first time as part of the Physics at High Angular Resolution of the Nearby GalaxieS (PHANGS) program.”

“Alongside the NASA/ESA Hubble Space Telescope, this initiative utilizes the capabilities of various powerful observatories, including the Atacama Large Millimeter/Submillimeter Array, ESO’s Very Large Telescope, and the NASA/ESA/CSA James Webb Space Telescope.”

“NGC 7496 was the inaugural galaxy in the PHANGS sample to be observed by Webb.”

“Each of these observatories offers a unique perspective on this extensively studied galaxy.”

“With its exceptional ultraviolet capabilities and high resolution, Hubble’s observations reveal young star clusters emitting high-energy radiation.”

“Hubble’s insights into NGC 7496 will assist in determining the ages and masses of these young stars, as well as the degree to which their light is obscured by dust.”

“Previous Hubble images of NGC 7496 were released in 2022,” they noted.

“Today’s image incorporates fresh data showcasing the galaxy’s star clusters amid glowing red clouds of hydrogen gas.”

Source: www.sci.news

Hubble Space Telescope Captures Stunning Spiral Galaxy: NGC 6000

The Hubble team has unveiled stunning images captured by the NASA/ESA Hubble Space Telescope, showcasing half of the Barred Spiral Galaxy NGC 6000.



This Hubble image reveals NGC 6000, a barred spiral galaxy located around 102 million light years away in the constellation Scorpius. Image credits: NASA/ESA/Hubble/A. Filippenko/MHözsaraç.

NGC 6000 is approximately 102 million light years distant from the constellation Scorpio.

Also known as ESO 450-20, IRAS 15467-2914, or LEDA 56145, this spiral galaxy spans nearly 67,000 light years.

It was first observed by British astronomer John Herschel on May 8, 1834.

Classified as a Seyfert II Galaxy, NGC 6000 is the brightest galaxy in the constellation of Scorpio.

“The NGC 6000 showcases a luminous yellow center surrounded by a sparkling blue region,” stated Hubble astronomers.

“These colors signify variations in the average age, mass, and temperature of the stars within the galaxy.”

“In the galaxy’s core, the stars tend to be older and smaller.”

“Interestingly, fewer giant stars are cooler compared to their larger counterparts; cooler stars appear red, while hotter stars take on a blue hue.”

“Along the spiral arm of NGC 6000, the Brilliant Star cluster is home to a young, massive star that distinctly looks blue.”

Hubble’s instruments gathered data from new images of NGC 6000 while investigating the site of a recent supernova explosion in a nearby galaxy.

“NGC 6000 has witnessed two supernovas: SN 2007CH in 2007 and SN 2010 in 2010,” noted the astronomer.

“We were able to detect the faint glow of the supernova several years post the initial explosion.”

“These observations assist in determining the star mass of supernova progenitor cells and whether they possess stellar companions.”

“If you zoom in on the right side of the galaxy disc in this image, you may notice other yellow and blue formations, which are four thin lines.”

“These represent asteroids from our solar system transit across Hubble’s field of vision while observing NGC 6000.”

“The four streaks arise from varying exposures captured sequentially with brief pauses in between, which we merged to create this final image.”

“The colors appear in this manner: each exposure captures specific red and blue wavelengths, as we used filters to isolate light at very particular wavelengths.”

“Collecting these individual exposures is vital for studying and comparing star colors, though it makes inter-agency intrusions quite apparent.”

Source: www.sci.news

Hubble Captures the Stellar Core of Messier 82

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured a new image of the central region of the Edge-on-Starburst Galaxy Messier 82.



This Hubble image displays Messier 82, a starburst irregular galaxy located 12 million light years away in the Ursa Major constellation. Image credits: NASA/ESA/Hubble/WD Vacca.

Messier 82 is situated roughly 12 million light years from the northern Ursa Major constellation.

Initially identified by German astronomer Johann Erard Bord in 1774, this galaxy spans about 40,000 light years.

Known as the Cigar Galaxy, Messier 82 features an elongated oval shape due to the tilt of its starry disc relative to our view.

This galaxy is renowned for its remarkable pace in star formation, generating stars at a rate ten times faster than that of the Milky Way.

“Messier 82 is home to a stunning star that shines through clouds of gas, dust, and clumps,” remarked the Hubble astronomer.

“It’s not surprising to find that the galaxy is so densely packed with stars.”

“Galaxies that produce stars at a rate ten times faster than the Milky Way are classified as Starburst Galaxies.”

“This vigorous starbursts phase has led to the emergence of superstar clusters at the galaxy’s core.”

“Each of these stellar clusters contains hundreds of thousands of stars, surpassing the brightness of ordinary star clusters.”

Astronomers have employed Hubble to investigate these vast clusters and understand their formation and evolution.

“The image reveals features that were previously unseen in earlier Hubble images of galaxies: data from the Advanced Camera for Surveys (ACS) high-resolution channels,” they noted.

“The high-resolution channel is one of three sub-instruments of the ACS, which was installed in 2002.”

“After five years of operation, the high-resolution channel provided stunning, detailed observations of a dense stellar environment like the heart of the Starburst Galaxy.”

“Unfortunately, an electronic failure in 2007 rendered the high-resolution channel inoperative.”

Source: www.sci.news

Powerful Image Captures the Hidden Struggles of Southeast Asia’s Fishing Industry

Fishermen unload their catch in the Philippines

Nicole Tung

These striking images capture the efforts of photographer Nicole Tung, who dedicated nine months to documenting the human and environmental toll of overfishing in Southeast Asia. Since the 1950s, fishing has rapidly evolved from a traditional craft into a global industry, primarily in developed nations. The rise in overfishing and illegal catch practices is alarming, driven by the increasing demand from a growing population.

Tung emphasizes the significance of the region as a vital part of the global fisheries market. Her project received funding from the €50,000 Kaminyak Photojournalism Award for fieldwork, which shifted her perspective on seafood consumption. Rather than suggesting complete abstention, she advocates for greater awareness and informed choices from consumers.

She expressed her distress over harrowing accounts from Indonesian fishermen, who detailed the violence and dreadful conditions they encounter at sea.

The image above illustrates a fisherman delivering a catch of tuna at General Santos fishport in the Philippines after a month at sea, including Bigger Tuna and Blue Marlin.

Thai dock worker

Nicole Tung

In other scenes, dock workers from Myanmar sort fish species being offloaded in Ranong, Thailand. Below, the indigenous Ulak Roy people and Thai villagers from Koh Lipe gather wood from nearby islands during a festival celebrating the end of the fishing and tourism season. They utilize the materials to construct ceremonial boats as offerings to their ancestors.

Indigenous Urak Lawoi people and Thai villagers sail their boats in Thailand

Nicole Tung

In this concluding image, a family of Filipino fishermen prepares bait for their fishing line in Quezon, Palawan, Philippines.

Family preparing to fish in the Philippines

Nicole Tung

Topics:

Source: www.newscientist.com

Hubble Captures Image of Active Spiral Galaxy NGC 7456

Using the Widefield Camera 3 (WFC3) mounted on the NASA/ESA Hubble Space Telescope, astronomers have captured a breathtaking new image of the Spiral Galaxy NGC 7456.



This Hubble image showcases NGC 7456, a spiral galaxy located 51 million light-years away in the constellation of Grus. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 7456 was discovered by British astronomer John Herschel on September 4, 1834.

This galaxy is approximately 51 million light-years from Earth, in the constellation Grus.

Also referred to as ESO 346-26, IRAS 22594-3950, or LEDA 70304, it spans a diameter of 117,100 light-years.

The NGC 7456 belongs to the LDC 1547 Galaxy Group, which includes 16 large galaxies.

“In Hubble’s image, one can observe the intricate, swirling arms of this galaxy in exquisite detail, complemented by a dark, diffuse mass of dust,” remarked an astronomer from Webb.

“The bright pink regions signify gas-rich areas where new stars are emerging, illuminating the surrounding clouds, as this gas emits transmitted red light.”

“The Hubble program has been gathering these data to study stellar activity, tracking new star-forming clouds, hydrogen, star clusters, and gaining insights into galaxy evolution over time,” they further explained.

“With its capability to capture visible ultraviolet and some infrared light, Hubble isn’t the only observatory focused on NGC 7456.”

“ESA’s XMM-Newton satellite has imaged X-rays from galaxies multiple times and discovered what is known as a hyper-luminous X-ray source.”

“These compact objects emit significantly more powerful X-rays than one would expect for their size.”

“We are still investigating what drives these extreme objects. NGC 7456 contributes several examples to this research.”

“Additionally, the area surrounding the galaxy’s supermassive black hole is incredibly bright and energetic, making NGC 7456 an active galaxy.”

“Whether viewed in visible light or X-rays, there’s always something intriguing about this galaxy, whether focusing on its core or its outer regions.”

Source: www.sci.news

Hubble Space Telescope Captures Stunning Detail of NGC 45’s Outer Arm

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured breathtaking new images of sections of the spiral galaxy known as NGC 45.



This Hubble image depicts the outer arm of the NGC 45, a spiral galaxy approximately 22 million light-years distant in the Cetus constellation. This color image was generated from individual exposures taken in both visible and near-infrared light using Hubble’s Wide Field Camera 3 (WFC3). The colors have been produced by assigning different hues to each monochromatic image captured through various filters. Image credits: NASA/ESA/Hubble/D. Calzetti/R. Chandar/Mhözsaraç.

NGC 45 is located about 22 million light-years away within the constellation of Cetus.

Also referred to as DDO 223, ESO 473-1, or Leda 930, this galaxy spans roughly 81,000 light-years in diameter.

The discovery of NGC 45 dates back to November 11, 1835, by British astronomer John Herschel.

“The data from Hubble utilized to create this portrait of NGC 45 was obtained from two complementary observational programs,” stated Hubble astronomers.

“Initially, we leveraged Hubble’s capability to capture light from ultraviolet to near-infrared ranges to broadly observe galaxies and examine star formation within them.”

“In the second program, we focused on many of the same nearby galaxies as the first, narrowing down to a specific wavelength of red light known as H-alpha.”

“Star-forming nebulae emit strong H-alpha light, and several of these areas can be identified by their bright pink red color throughout NGC 45.”

“These observational programs aim to investigate star formation across galaxies of varying sizes, structures, and separations, making NGC 45 a particularly compelling target.”

Though it may appear to be an ordinary spiral galaxy, NGC 45 is actually a remarkable low surface brightness galaxy.

“Low surface brightness galaxies are more intriguing than the evening sky and are incredibly challenging to detect,” articulated the researchers.

“They possess relatively fewer stars in relation to the amount of gas and dark matter they contain, making them appear unexpectedly faint.”

“Since the accidental discovery of the first low-surface brightness galaxies in 1986, scientists have learned that 30-60% of all galaxies may fall within this category.”

“Investigating these elusive galaxies is crucial for understanding the formation and evolution of galaxies, and Hubble’s sensitive instruments are well-suited for this task.”

Source: www.sci.news

This Adorable Footage Captures a Baby Turtle Responding to Its Mother’s Call

Emerging from the darkness, slimy nails break through the murky barrier, reaching towards the light. Thunder rumbles as the ground cracks.

This is not a scene from a horror film featuring the undead rising from their graves. Rather, it showcases one of nature’s most endearing spectacles, Parent-child relationship: a forthcoming BBC series exploring the struggles of nurturing the next generation of wildlife, specifically the hatching of the magnificent Amazon River Turtle in Guapoi, South Brazil.

https://c02.purpledshub.com/uploads/sites/41/2025/07/Parenthood-turtle-hatchlings.mp4
Giant Amazon River turtles featured in the new BBC series Parent-child relationship

According to Sir David Attenborough’s narration, the tiny turtles await the perfect conditions to break free. When rain falls, it softens the sand enough for them to dig their way out. If there’s insufficient rain, the layer of sand above becomes too baked in the sun. They are numerous, making their survival seem effortless.

“There’s always that anxiety. You never know how it will turn out,” says series producer Elizabeth Orcham to BBC Science Focus. “As we sit with the crew, we hope everything works. The moment it rains or doesn’t rain, the tension rises. Is it too much rain?”

The rain arrived early during the filming, but the turtles managed to emerge just in time. “Seeing most of the turtles succeed and not lose too many is really comforting. It’s just wonderful.”

Despite the challenges posed by the weather, two million turtles hatched successfully, overcoming what seemed like insurmountable odds.

“Sometimes, it’s a wonder how they survive. It’s fascinating to see just how clumsy they can be,” she notes.

This clumsiness, however, is part of a finely tuned process. Scientists have been investigating communication among these turtles for over a decade. A 2014 study found that mothers likely communicate with their hatchlings to guide them into the water. According to Oakham, this is the only turtle species known to exhibit parental care post-hatching.

The female giant Amazon River turtle (Podocnemis Exagna), also known as the Arrau turtle, grows to a remarkable 76cm (30 inches) in shell length and weighs up to 91kg (200 pounds), while the male measures at 48cm (19 inches). The hatchlings are merely 5cm (2 inches) long. – Photo credit: Getty

The team even managed to capture charming moments featuring the hatchlings helping each other dig out.

“We were thrilled to showcase this new research on turtle communication,” Oakham explains. The filmmakers even accessed the nest to record the hatchlings’ emergence.

Childcare challenges

Climate change poses the greatest threat to the otherwise stable lifecycle of the giant Amazon River turtle.

“Warmer air due to climate change retains more moisture, leading to two outcomes,” she elaborates. “Firstly, it makes the environment drier, but when it finally rains, the moisture simply drips off.”

Severe floods that once occurred every 20 years have now happened twice in the last five years, jeopardizing the hatching process during critical seasons.

Before hatching, the turtles must absorb some of their yolk sac. If they haven’t done so before floods arrive, they will not survive. Thus, when mother turtles lay eggs, they risk a significant gamble regarding the weather – a gamble that is increasingly hard to predict.

They typically lay their eggs two to three months before the rainy season, allowing the sand to solidify and form a protective layer. At this time, the mothers leave the river for the sandbanks, coinciding with the largest congregation of freshwater turtles on the planet, and one of the few instances the species ventures onto land.

“Water can be life-sustaining but also perilous,” Oakham states. “With climate change, this duality has become even more pronounced, making the environment more unpredictable for these parents. Navigating this uncertainty while caring for their young is a delicate balance.”

This episode is the fourth in a five-part series on parental life in freshwater habitats, Parent-child relationship. All five episodes will be available on BBC iPlayer from August 3, 2025.

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About our experts

Elizabeth Orcum is a producer and director with a deep commitment to environmental storytelling and natural history. She is widely recognized for her work on the fifth episode of Green Planet, titled “The Human World,” which delivers a compelling narrative on the interconnectedness of plants and humans. She is now eager to share the stories of animal parents worldwide through the BBC series Parent-child relationship.

Source: www.sciencefocus.com

Hubble Captures Stunning Images of NGC 1309

The Hubble team has unveiled a breathtaking new image captured by the NASA/ESA Hubble Space Telescope, showcasing the Facon Spiral Galaxy NGC 1309.



Hubble’s image reveals NGC 1309, a spiral galaxy situated about 100 million light years away in the Eridanus constellation. This color representation is a result of observations from Hubble’s Advanced Camera (ACS) and Wide Field Camera 3 (WFC3), utilizing multiple filters to explore ultraviolet, infrared, and optical wavelengths. Each color corresponds to a specific filter’s monochromatic image. Image credits: NASA/ESA/Hubble/L. Galbany/S. Jha/K. Noll/A. Riess.

NGC 1309 is located about 100 million light years away in the constellation Eridanus.

Commonly referred to as IRAS03197-1534, LEDA 12626, or TC 470, this galaxy has a diameter of 75,000 light years.

NGC 1309 was first discovered on October 3, 1785, by the German-British astronomer William Herschel.

The galaxy is the brightest member of the NGC 1309 group, which also includes MCG -03-09-027 and UGCA 71.

“The mesmerizing Hubble images capture the bluish tones of NGC 1309, alongside dark brown gas clouds and shimmering white centers, interspersed with hundreds of remote background galaxies,” remarked Hubble astronomers.

“Almost every dot, stripe, and cluster of light in this image represents an individual galaxy.”

“The sole exception in this vast extragalactic scenery is a star, identifiable near the top of the frame due to its distinctive diffraction spikes.”

“This star is relatively nearby, merely thousands of light years away within our Milky Way galaxy.”

Significant scientific interest in NGC 1309 arises from two supernovae. SN 2002fk and SN 2012Z, which occurred in 2002 and 2012, respectively.

“The SN 2002fk exemplified the type Ia supernova, occurring when a white dwarf’s core explodes,” the astronomer explained.

“Conversely, SN 2012Z displayed a more unique behavior, classified as a type IAX supernova. Its spectrum resembled that of a type Ia supernova, yet its brightness was unexpectedly dim.”

“Hubble’s observations revealed that the explosion did not fully annihilate the white dwarf, resulting in a ‘zombie star’ that shone even more brightly than before the supernova event.”

“Hubble’s extensive observations of NGC 1309 over several years enabled the identification of supernova progenitor cells within images taken prior to the explosion.”

Source: www.sci.news

Hubble Space Telescope Captures a Mesmerizing Spiral Galaxy Spin

The NASA/ESA Hubble Space Telescope has captured a stunning image of the Barred Spiral Galaxy NGC 3285b.



This Hubble image reveals NGC 3285B, a spiral galaxy approximately 137 million light years away in the Hydra constellation. The color images were generated from separate exposures in the ultraviolet and infrared regions using Hubble’s Wide Field Camera 3 (WFC3), based on data collected through seven filters. Image credits: NASA/ESA/Hubble/RJ Foley, UC Santa Cruz.

NGC 3285b is situated around 137 million light years from the Hydra constellation.

It is also referred to as Leda 31293, ESO 501-18, or IRAS 10322-2723, with a diameter of 100,000 light years.

NGC 3285B boasts a disc and multiple swirling arms, characterized by a large, bright, golden nucleus, while its spiral arms exhibit a light, faint reddish hue.

It is part of the NGC 3312 Galaxy Group (LGG 210) and is a member of the Hydra I Galaxy Cluster.

“NGC 3285B is a component of the Hydra I Cluster, one of the largest galactic clusters in the nearby universe,” stated Hubble astronomers.

“Galactic clusters consist of hundreds to thousands of galaxies held together by gravity.”

“The Hydra I cluster is centered around two massive elliptical galaxies.”

“Each of these galaxies spans about 150,000 light years, roughly 50% larger than our Milky Way.”

NGC 3285B lies on the outskirts of the Hydra I cluster, distanced from the colossal central galaxy.

“This galaxy captured Hubble’s interest as it hosted a Type Ia supernova in 2023,” the astronomer noted.

“Type Ia supernovae produce a condensed star core known as white dwarf explosives, igniting a sudden fusion burst approximately five billion times brighter than the sun.”

The supernova, labeled SN 2023XQM, appears as a blue dot on the far left side of the galaxy’s disc.

“Hubble observed NGC 3285B as part of a campaign focused on Type Ia supernovae.”

“We aim to address the effects of distance and dust by examining each of these supernovae in ultraviolet, optical, and near-infrared light.”

“This initiative will enhance cosmic distance measurements that depend on observations of Type Ia supernovae.”

Source: www.sci.news

Gemini North Telescope Captures Stunning New Images of Interstellar Comet 3I/Atlas

Astronomers utilizing the Gemini North telescope at NSF’s International Gemini Observatory have observed the interstellar comet 3i/Atlas as it passes through our cosmic neighborhood.



This image from the Gemini North Telescope Multi-Object Spectrometer (GMOS-N) showcases the interstellar comet 3i/Atlas. Image credits: International Gemini Observatory/Noirlab/NSF/Aura/K. Meech, Ifa&U. Hawaii / Jen Miller & Mahdi Zamani, Noirlab.

Interstellar objects are those that emerge from and traverse beyond our solar system.

Ranging from several meters to a few kilometers in size, these cosmic fragments are remnants from the formation of the host star’s planetary system.

As they orbit their stars, interactions with the gravitational pull of nearby planets and stars can eject them into interstellar space, allowing them to traverse other solar systems.

Studying interstellar visitors provides critical insights into distant star systems.

They carry valuable information about chemical elements, including their formation timelines and locations, offering scientists glimpses into the formation of planetary systems throughout the history of the Milky Way galaxy.

3i/Atlas marks the third interstellar object discovered, following 1i/Oumuamua in 2017 and 2i/Borisov in 2019.

Astronomers suspect that numerous interstellar objects might regularly pass through our solar system, but capturing them is challenging as they are only visible when telescopes are oriented correctly at the right time.

Multiple teams worldwide utilize various telescopes to monitor 3i/Atlas during its brief visitation, enabling them to collectively assess its key properties.

While many aspects remain unknown, 3i/Atlas is already recognized as distinct in comparison to 1i/Oumuamua and 2i/Borisov.

Previous observations suggest that 3i/Atlas could have a diameter of up to 20 km (12 miles).

New comets typically exhibit highly eccentric orbits, which define how much the object’s path deviates from a perfect circle.

An eccentricity of 0 indicates a circular orbit, while 0.999 signifies a highly elongated ellipse.

Objects with an eccentricity greater than 1 follow paths that do not loop around the Sun and come from, then return to, interstellar space.

The eccentricity of 3i/Atlas is recorded at 6.2, classifying it as a highly hyperbolic interstellar object.

In contrast, “Oumuamua’s” eccentricity was around 1.2, and Borisov’s was about 3.6.

As of now, 3i/Atlas resides in Jupiter’s orbit, approximately 465 million km (290 million miles) from Earth and 600 million km (370 million miles) from the Sun.

On December 19, 2025, it will come within roughly 270 million km (170 million miles) of Earth, posing no threat to our planet.

The closest approach to the Sun will occur around October 30, 2025, at a distance of 210 million km (130 million miles).

During this close approach, it is expected to travel at about 25,000 km (15,500 miles) per hour.

The latest image of 3i/Atlas was obtained using the Gemini North Telescope Multi-Object Spectrometer (GMOS-N).

“The sensitivity and scheduling precision of the International Gemini Observatory played a critical role in observing this interstellar wanderer,” remarked Martin Still, NSF Program Director at the International Gemini Observatory.

“We eagerly anticipate the wealth of new data and insights as this object warms in sunlight before continuing its cold, dark journey through interstellar space.”

Source: www.sci.news

VLT Captures Final Images of the Discarded Supernova

Astronomers utilizing ESO’s Extremely Large Telescope (VLT) have captured images of SNR 0509-67.5.



This image, obtained with the multi-unit spectroscopic explorer (Muse) located on ESO’s Extremely Large Telescope (VLT), displays the supernova remnant SNR 0509-67.5. The Calcium shown in blue is arranged in two concentric shells, indicating a double explosion of the star. Image credits: ESO/DAS et al. / Noll et al.

“White dwarfs—small, inert cores resulting from the demise of sun-like stars—are capable of producing what astronomers classify as type Ia supernovae,” states a PhD student from the University of New South Wales University of Canberra.

“Our understanding of the universe’s expansion hinges on these supernovae, which also serve as the primary source of iron on Earth, including in blood.”

“Yet, despite their significance, the mechanisms driving their explosions are still not fully understood.”

All theories surrounding Type Ia supernovae begin with pairs of white dwarf stars.

When one of the stars’ orbits is sufficiently close to its counterpart, it can siphon material from its companion.

According to the most prevalent theory regarding Type Ia supernovae, the white dwarf accumulates matter until it hits a critical mass and then experiences a singular explosion.

However, new research indicates that at least some Type Ia supernovae could be better explained by a series of double explosions occurring before the stars reach this critical mass.

The recent VLT images of SNR 0509-67.5 confirm these predictions.

In this alternative model, the white dwarf forms a helium layer through theft, which becomes unstable and can ignite.

This initial explosion generates a shockwave that moves inward, resulting in another explosion at the core of the star, ultimately leading to the supernova.

Until now, there had been no clear visual proof supporting the occurrence of a double explosion in white dwarfs.

Recent studies have suggested that this process creates identifiable patterns or “fingerprints” on the still-glowing debris from the supernova, surfacing long after the primary explosion.

Research proposes that the remains of such supernovae contain two distinct calcium signatures.

Das and his colleagues have found these fingerprints on the supernova remnants.

“The findings clearly indicate that white dwarfs can explode well before reaching the famous Chandrasekhar limit, demonstrating that the ‘double explosion’ mechanism naturally occurs,” remarks Dr. Ibo Seitenzar, an astronomer at the Heidelberg Institute.

Astronomers were able to identify these calcium layers in SNR 0509-67.5 by employing VLT’s multi-unit spectroscopic explorer (Muse).

This provides compelling evidence that Type Ia supernovae can occur prior to their progenitor white dwarfs reaching critical mass.

“This tangible evidence of double explosions not only aids in resolving historical mysteries but also offers a visual interpretation,” explains Das.

“It’s incredibly satisfying to reveal the intricate workings behind such colossal cosmic explosions.”

The team’s results are published today in the journal Nature Astronomy.

____

P. Das et al. Calcium in the remnants of the supernova as fingerprints of the sub-Chandrasekhar explosion. Nature Astronomy Published online on July 2, 2025. doi:10.1038/s41550-025-02589-5

Source: www.sci.news

Fireball Captures Spectacular Meteor Shower Lighting Up the Southeastern US Sky

A fireball was spotted soaring through the sky in the southeastern United States on Thursday afternoon, coinciding with reports of a meteor shower in the region, according to officials.

A representative from Forsyth County Emergency Management in Georgia stated that the meteor shower, validated by the National Weather Service, was still visible hours after the initial sighting.

The representative noted that there have been no reports of impacts or injuries, and monitoring of the showers is ongoing.

Earlier, the National Weather Service office in Charleston indicated that just before noon, there were “numerous reports of fireballs” across the area.

“While it’s not confirmed, satellite-based lightning detection indicated markings in the clear sky above the NC/VA border in Gasbury, Virginia,” reported between 11:51 am and 11:56 am the weather service noted at the time.

A video circulating on social media displays a fireball descending into a wooded area in South Carolina.

Kathryn Far posted a dashcam video taken while driving south on Interstate 85 toward Anderson, South Carolina, around 12:25 pm.

A video shared on social media shows a fireball being shot down into a wooded area of ​​South Carolina.
Kathryn Rose Fur via Facebook

“It’s not something you witness every day.” She mentioned on Facebook.

Another perspective from Andrew Colley Road in Lexington, South Carolina depicted suspected meteor stones blazing bright white with an orange flame tail before vanishing into a wooded area.

The Newton County Sheriff’s Office in Georgia reported that the weather department has informed them that the fireball is likely a meteor.

“Currently, there is no information on where the meteor may have landed.” The sheriff’s office stated, noting that fireballs have been reported by residents in Covington and nearby areas.

Source: www.nbcnews.com

Proba-3: Stunning Image Captures the First Artificial Solar Eclipse

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The sun’s corona appears as it would to the human eye during a solar eclipse, but through a green filter.

ESA/proba-3/aspiics

The synchronized movement of the twin satellites has produced the first artificial solar eclipse in space, revealing the burnt corona of the sun in remarkable detail.

The ProBA-3 mission, launched last December, is operated by the European Space Agency (ESA) and consists of two satellites positioned 150 meters apart.

One of the satellites, known as Occulter, features 1.4-meter wide discs made from carbon fiber and plastic, effectively blocking sunlight coming from the second satellite, Coronagraph. The alignment accuracy of the satellites is within one millimeter for capturing images.

In March, the satellites autonomously synchronized for extended periods, providing lengthy exposures of the solar eclipse. ESA scientists can stitch these exposures together to generate a comprehensive image of the solar corona, the outermost layer of the sun’s atmosphere.

“When I first viewed these images, it was unbelievable,” says Damien Galano from ESA. “But shortly after, it transformed into an incredible sense of achievement and pride for all our hard work.”

The image above captures the visible light of the corona, resembling how it would appear to the human eye but through a green filter.

This image illustrates the light emitted from electron-depleted iron in the most heated sections of the corona.

ESA/proba-3/aspiics

The Proba-3 satellite camera also captures light frequencies linked to specific elements within the solar corona, exemplified by the dark green image above.

“We can clearly see the substantial achievements made during COVID,” remarks Galano.

The sun’s corona shown in polarized white light, artificially tinted to look violet.

ESA/proba-3/aspiics

The image above illustrates the sun’s corona, artificially colored purple in polarized white light. This technique allows scientists to distinguish the polarized light from the hot corona from that scattered by interplanetary dust.

These images were primarily captured to verify the ProBA-3 mission’s functionality. When fully operational, they will take pictures of the artificial food every 19.6 hours.

This will enhance our comprehension of solar corona physics, and according to Galano, it will also improve understanding of solar winds and coronal mass ejections that influence space weather.

Total Solar Eclipse 2026: Travel from Iceland to Greenland

Join an incredible journey in August 2026 and experience an awe-inspiring total solar eclipse.

Topics:

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Source: www.newscientist.com

Hubble Captures the Breathtaking Barred Spiral Galaxy: IC 758

The NASA/ESA Hubble Space Telescope has captured a stunning new image of IC 758, a spiral galaxy located within the constellation Ursa Major.



This Hubble image depicts IC 758, a barred spiral galaxy located roughly 60 million light years from Earth in the Ursa Major constellation. The colorful image is based on observations from Hubble’s advanced cameras used for the Investigation of the Near-Infrared and Optical Parts (ACS). Two filters were utilized to capture different wavelengths, with colors assigned by applying distinct hues to each monochromatic image linked to an individual filter. Image credits: NASA/ESA/Hubble/C. Kilpatrick.

IC 758, located about 60 million light years from our planet in the constellation Ursa Major, is also known as Leda 38173 or UGC 7056.

This galaxy was discovered by the American astronomer Lewis Swift on April 17, 1888.

IC 758 is a member of the NGC 4036 Galaxy Group (also referred to as LGG 266), which encompasses more than 10 galaxies.

“In this captivating Hubble image taken in 2023, IC 758 appears serene, with its gentle blue spiral arm gracefully curving around its prominent Barred Center,” remarked a Hubble astronomer.

“However, in 1999, astronomers detected a significant event in this galaxy: the supernova SN 1999bg.”

“SN 1999BG marked the explosive conclusion of a star much larger than our sun.”

“We are still uncertain about the mass of this star before its explosion,” they added.

“Utilizing these Hubble observations, we can determine the mass of the nearby stars in SN 1999BG, aiding in the estimation of the supernova’s progenitor.”

“Hubble’s data might also provide insights into whether the precursor star of SN 1999BG has a companion.”

“A supernova signifies more than just the end of a single star; it is a formidable force that can influence its surroundings,” the astronomer noted.

“When a massive star collapses and triggers a supernova, its outer layers rebound from the diminishing core.”

“This explosion disrupts the interstellar medium of gases and dust from which new stars are born.”

“This upheaval may lead to the formation of new stars by scattering and heating adjacent gas clouds or compressing them to generate new stars.”

“The expelled outer layers also contribute to the materials needed for new star formation.”

Source: www.sci.news

Hubble Space Telescope Captures Stunning Image of Star-Forming Spiral Galaxy NGC 685

The NGC 685 is abundant in star-forming nebulae and appears as a dazzling pink cloud in recent images captured by the NASA/ESA Hubble Space Telescope.



This Hubble image illustrates the Spiral Galaxy NGC 685 on the bar. The color images were created from individual exposures captured in ultraviolet light using Hubble’s Wide Field Camera 3 (WFC3) and derived from visible and near-infrared sections of the spectrum. Built upon data gathered through six filters, different hues are assigned to each monochromatic image related to a specific filter. Image credits: NASA/ESA/Hubble/J. Lee/F. Belfiore.

NGC 685 is situated approximately 64 million light-years away in the southern constellation of Eridanus.

Previously known as ESO 152-24, IRAS 01458-5300, or LEDA 6581, the galaxy was discovered by British astronomer John Herschel on October 3, 1834.

Spanning around 74,000 light-years, the galaxy features a luminous central bar and a distinctively curved arm.

“NGC 685 is classified as a barred spiral galaxy, with its delicate spiral arms emerging from the edge of a stellar bar at the heart of the galaxy,” Hubble astronomers stated.

“The Milky Way, while not a perfect spiral, is nearly twice the size of NGC 685.”

Astronomers utilized Hubble for two observational programs focused on star formation in NGC 685.

“It’s no surprise that NGC 685 was selected for these studies. The galaxy’s spiral arms are marked by numerous patches of young blue stars,” they noted.

“Many of these star clusters are enveloped by a vibrant pink gas cloud known as the H II region.”

“The H II region is a gas cloud that gleams momentarily, especially during the birth of a massive, hot star.”

“The particularly striking H II region can be seen near the lower edge of the image.”

“Despite the visible star-forming regions, NGC 685 converts gas into stars each year at a rate of less than half the mass of the sun.”

“The data collected by Hubble across two observational programs enables us to catalog 50,000 H II regions and 100,000 star clusters in nearby galaxies.”

“By merging Hubble’s sensitive visibility and ultraviolet observations with data from the NASA/ESA/CSA James Webb Space Telescope and wireless data from the Atacama Large Millimeter/submillimeter Array, we explore the depths of dusty star nurseries and illuminate the stars within.”

Source: www.sci.news

Hubble Captures Stunning Spiral Galaxy: NGC 3507

Astronomers utilizing the NASA/ESA Hubble Space Telescope captured a stunning new image of the Face-On Barred Spiral Galaxy NGC 3507.



This Hubble image illustrates the NGC 3507, a barred spiral galaxy located 46 million light years away in the constellation Leo. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 3507 is situated approximately 46 million light years from Earth in the Leo constellation.

Also referred to as Hipass J1103+18, Leda 33390, or UGC 6123, this galaxy spans nearly 50,000 light years.

It was discovered on March 14, 1784, by the German-British astronomer William Herschel and is paired with the large spiral galaxy NGC 3501.

A Hubble astronomer explained, “NGC 3507 is classified as a barred spiral because its prominent spiral arms emerge from the edge of the galaxy’s central bar instead of its center.”

“In this image, we focus on NGC 3507, which is alongside its galactic companion NGC 3501, though NGC 3501 lies outside the frame.”

“While the NGC 3507 follows the typical spiral galaxy structure, its companion has a more dynamic appearance as it travels through space.”

“Though both are classified as spiral galaxies, they present themselves differently depending on the observed angle.”

“Features like spiral arms, dusty gas clouds, and vibrant star clusters are vividly displayed for galaxies as distant as NGC 3507 and NGC 3501,” the researchers noted.

“Distant galaxies tend to lack fine details.”

“See if you can identify other distant galaxies in this image; they often appear orange or yellow, showcasing hints of spiral arms with variations from round stars to elongated shapes.”

Along with its distant neighbors, NGC 3507 also features much closer objects, identifiable by four light spikes, which represent a star in the Milky Way, located merely 436 light years from Earth.

Source: www.sci.news

Webb Captures Dynamic Infrared Auroras on Jupiter

Jovian auroras shine hundreds of times brighter than those visible from Earth, according to a team of astronomers led by Dr. Jonathan Nichols at the University of Leicester.

These observations of Jupiter’s aurora were captured on December 25, 2023 by Webb’s near-infrared camera (NIRCAM). Image credit: NASA / ESA / CSA / STSCI / RICARDO HUESO, UPV / IMKE DE PATER, UC BERKELEY / THIERRY FOUCHET, OBSERVATORY OF PARIS / LE FLETCHER, JOSEPH DEPASQUALE, STSCI/J. NICHOLS, UNIVERSITY OF LEICESTER/M. ZAMANI, ESA & WEBB.

When high-energy particles enter the planet’s atmosphere near its magnetic poles, they collide with gas atoms, creating the auroras.

Jupiter’s auroras are not only massive in scale but also exhibit energy levels hundreds of times greater than those seen on Earth.

These auroras are primarily triggered by solar storms, where charged particles entering the atmosphere excite gas particles, resulting in vibrant red, green, and purple hues.

Additionally, Jupiter has a unique source of auroral activity—its strong magnetic field captures charged particles from its surroundings.

This includes not only those from the solar wind but also particles ejected from the volcanic moon Io.

The eruptions from Io’s volcanoes release particles that escape both the moon’s and Jupiter’s gravitational pull.

Solar storms also discharge vast amounts of charged particles towards Jupiter.

Jupiter’s immense magnetic fields accelerate these charged particles to extraordinary speeds.

When these high-velocity particles collide with the planet’s atmosphere, they excite the gas and produce radiant displays.

https://www.youtube.com/watch?v=if0vpfergju

Thanks to the advanced capabilities of the NASA/ESA/CSA James Webb Space Telescope, new insights into Jovian auroras can be gained.

The telescope’s sensitivity enables astronomers to use faster shutter speeds to capture the rapidly evolving features of the auroras.

This latest data was collected using Webb’s near-infrared camera (NIRCAM) on Christmas Day 2023.

“What a Christmas gift; it truly astonished me!” exclaimed Dr. Nichols.

“We aimed to observe how quickly the aurora transformed, hoping to see beautiful fluctuations within about an hour.”

“Instead, we witnessed the entire aurora region illuminating the sky in a spectacular display.

Astronomers noted fluctuations in the effects caused by trihydrogen ions, known as H.3+, which varied more than previously assumed.

These observations help scientists unravel how Jupiter’s upper atmosphere undergoes heating and cooling.

Additionally, several unknown phenomena were identified in the data.

“What made these observations particularly intriguing was that the NASA/ESA Hubble Space Telescope was capturing images simultaneously in ultraviolet light,” Dr. Nichols commented.

“Strangely, the brightest light observed by Webb seemed to have no corresponding feature in Hubble’s images. This left me puzzled.”

“To produce the brightness observed in both Webb and Hubble, we would require an improbable mix of a substantial quantity of very low-energy particles impacting the atmosphere.

study Published in the journal Nature Communications.

____

JD Nichols et al. 2025. The dynamic infrared aurora of Jupiter. Nature Communications 16, 3907; doi:10.1038/s41467-025-58984-z

Source: www.sci.news

Hubble Captures Direct View of Intermediate Spiral Galaxy

A stunning new image from the NASA/ESA Hubble Space Telescope captures the beauty of the Spiral Galaxy NGC 3596.



This Hubble image showcases NGC 3596, a mid-spiral galaxy roughly 90 million light years from Earth in the constellation Leo. The color image features observations from Hubble’s Wide Field Camera 3 (WFC3), taken in the ultraviolet, near-infrared, and optical spectra. The colors result from assigning varying hues to each monochromatic image linked with individual filters. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 3596 is situated approximately 90 million light years away in the constellation Leo.

This galaxy was first discovered by German and British astronomer William Herschel on April 8, 1784.

Also recognized as Leda 34298, UGC 6277, or Hipass J1115+14, NGC 3596 belongs to the Leo II Group, a collection of galaxies within the Virgo supercluster.

“NGC 3596 is nearly perfectly oriented face-on relative to Earth, revealing the galaxy’s beautifully wound spiral arms,” stated the Hubble astronomer.

“The bright arms are densely packed with stars, gas, and dust.”

“Star formation is particularly vigorous in the spiral arms, as indicated by the vibrant pink regions of star formation and the young blue stars tracing the arms of NGC 3596 in this image.”

“What triggers the formation of these spiral arms? Given the vast variety of spiral galaxies, it’s a complex question,” they noted.

“Some galaxies exhibit clear spiral arms, while others have more erratic feathered arms.”

“Some display prominent bars at their centers, whereas others have compact circular cores.”

“Some galaxies are surrounded by neighbors, while others stand alone.”

“Early theories about the formation of spiral arms were complicated by what they termed a convoluted problem,” the researchers explained.

“If the spiral arms are a coherent feature, they would be tightly wrapped as the galaxy rotates, eventually rendering them invisible.”

Currently, researchers think that spiral arms represent patterns of varying density rather than fixed structures.

“Material such as stars, gas, and dust flows in and out of the spiral arms as they orbit within the galaxy’s disc,” they added.

“Much like vehicles encountering traffic jams, these materials decelerate as they enter the spiral arms, become gravitationally bound, and continue their journey through the galaxy.”

Source: www.sci.news

Webb captures stunning new image of Planet Nebula NGC 1514

The two central stars of the NGC 1514 are displayed as one of the images from the NASA/ESA/CSA James Webb Space Telescope, forming this scene for thousands of years and maintaining it for thousands more.

This web image shows the planetary nebula NGC 1514. Image credits: NASA/ESA/CSA/STSCI/Michael Ressler, JPL/Dave Jones, IAC.

NGC 1514 It is about 1,500 light years away from the Taurus sign.

The object, also known as the Crystal Ball Nebula, was discovered on November 13th, 1790 by German and British astronomer William Herschel.

He pointed out that NGC 1514 was the first deep sky object that really looked cloudy. He couldn’t resolve what he saw on individual stars in the cluster, like other objects he catalogued.

The ring around NGC 1514 was discovered in 2010, but Webb is now allowing astronomers to comprehensively examine the nature of the turbulent flow of this nebula.

“This scene has been formed for at least four,000 years and will continue to change over a thousand years,” Webb Astronomers said in a statement.

“In the center there are two stars that appear as one in Webb observations, caused by vivid diffraction spikes.”

“The star follows a solid, elongated nine-year orbit, covered in an arc of dust, represented by orange.”

“One of these stars, once a massive scale several times larger than our sun, played the lead role in producing this scene.”

“When the outer layers of the star were exhausted, only the hot, compact core was left behind.”

“As a white dwarf star, its winds rose sharply and weakened, and could have blown away the material into a thin shell.”

New Webb observations show that the nebula is at a 60-degree angle, which makes it appear that the can is poured in, but it is much more likely that the NGC 1514 took the shape of an hourglass and dropped the edges.

“Look for pinchwaist hints near the top left and bottom right. The dust is orange and drifts in a shallow V-shaped shape,” the astronomer said.

“When the star reached its peak of losing material, our peers may have become very close and have had these unusual shapes.”

“Instead of creating a sphere, this interaction may have instead formed a ring.”

“The NGC 1514’s outline is most clear, but the hourglass also has some sides of the 3D shape.”

“Look for a dim, translucent orange cloud between the rings that give to the nebula body.”

Nebula’s two rings are illuminated unevenly by Webb’s observations, appearing to be more diffused at the bottom left and top right.

Researchers believe that the rings are primarily made up of very small dust grains. This will get hot enough for Webb to detect when hit by ultraviolet rays from a white star star.

“In addition to dust, Webb revealed oxygen in its chunky pink center, especially at the edges of the bubbles and holes,” they said.

Source: www.sci.news

Hubble Captures Breathtaking Images of Obscure Planet Nebula

Officially named Kohoutek 4-55, this little-known planetary nebula is located within our Milky Way galaxy.



This Hubble image shows Kohoutek 4-55, a nebula of planets 4,600 light years away in the Cygnus constellation. Image credits: NASA/ESA/Hubble/K. Noll.

“The Nebula of Planets is a spectacular final exhibition at the end of the life of a giant star,” Hubble Astherm said in a statement.

“When the giant red star runs out of available fuel and flows the final gas layer, its compact core shrinks further, allowing for a final burst of fusion.”

“The exposed core reaches very high temperatures and emits very energetic UV rays, activating a huge cloud of casting gas.”

“Molecules in the gas are ionized and brighten.”

“Here, red and orange represent nitrogen molecules, green represent hydrogen, and blue represent nebulae oxygen.”

Kohoutek 4-55 is located approximately 4,600 light years away from the Cygnus constellation.

Also known as UHA 15 or G084.2+01.0, this nebula has an unusual multilayered form.

“The bright inner ring of the Kohoutek 4-55 is surrounded by a loose layer of gas, all wrapped in a wide halo of ionized nitrogen,” the astronomer said.

“The view is bittersweet. The short phase of the fusion of the cores ends tens of thousands of years, leaving behind a white dwarf who will never illuminate the surrounding clouds again.”

This image of Kohoutek 4-55 was captured by Hubble’s Widefield and Planetary Camera 2 (WFPC2).

“Installed in 1993 to replace the original Widefield and Planetary Camera (WFPC), WFPC2 was responsible for some of Hubble’s most persistent images and fascinating discoveries,” the researchers said.

“It was replaced in 2009 by Widefield Camera 3 (WFC3) during Hubble’s final service mission.”

“The data in this image was collected 10 days before the instrument was removed from the telescope, as a proper postponement for WFPC2,” he said.

“The latest and most advanced processing techniques are used to bring data to life once more, creating this breathtaking new view of Kohoutek 4-55.”

Source: www.sci.news

Webb telescope measures size of asteroid 2024 YR4 and captures images of potential danger

The destructive forces of shocking asteroids are estimated primarily by knowledge of their size. Near Earth Asteroid 2024 YR4 reached a peak 2032 impact probability on Earth at 3%, motivated the desire to determine its size. Due to its infrared capabilities, the NASA/ESA/CSA James Webbspace Telescope is uniquely suited to such evaluations. Johns Hopkins University astronomer Andrew Livkin and his colleagues used two Webb instruments to measure the diameter for 2024.

These web images show asteroid 2024 YR4 near Earth. Image credits: NASA/ESA/CSA/STSCI/A. RIVKIN, JHU/APL.

2024 yr4 On December 27, 2024, the Asteroid Terrestrial Impact of Río Hurtado was discovered by the Last Alert System (Atlas) station.

The asteroid took a close approach to Earth at a distance of 828,800 km (515,000 miles) two days before its discovery.

Initial observations from the 2024 YR4 showed that the diameter was 40-90 m (131-295 ft).

Dr. Eric McLennan, an astronomer at the University of Helsinki, said:

“However, thermal radiation at infrared wavelengths is a direct indicator of size.”

Dr. Livin, Dr. McLennan and his colleagues observed using the 2024 YR4 Webb’s Near-Infrared Camera (nircam) Mid-infrared instrument (Milli).

Nircam data reflects light, while Miri’s observations show heat light.

“The observations were taken to study the thermal properties of the 2024 YR4, including how quickly it heats and cools at the current distance from the sun, and how hot the heat is,” the astronomer said.

“These measurements show that this asteroid does not share the properties observed on the larger asteroid.”

“This could be a combination of its fast spin and a lack of fine sand on its surface.”

“More research is needed, but this is thought to coincide with surfaces dominated by rocks that are roughly below the size of a fist.”

New Webb observations show that the asteroid measures approximately 60 m (197 feet).

“The 2024 YR4 has been the smallest object that Webb has ever targeted and is one of the smallest objects that directly measure its size,” the researchers said.

“New observations from Webb provide unique information about the size of the YR4 in 2024, as well as complement the ground-based observations of the object’s location to improve understanding of the object’s trajectory and future trajectory.”

Team’s Survey results It was published in AAS research notes.

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As Livin et al. 2025. JWST observation of potentially dangerous asteroid 2024 YR4. res. Note AAS 9, 70; doi:10.3847/2515-5172/ADC6F0

Source: www.sci.news

Webb captures Aurorae on Neptune for the first time while detecting trihydrogen

Emission from trihydrogen cations of large atmospheres flames (h3+) It has been used for over 30 years to study the global interactions of Jupiter, Saturn and Uranus with the surrounding space environment, revealing the process of aurora formation. However, despite repeated attempts, and against models that predict it should exist, this ion has proven elusive in Neptune. Currently, using observations from the NASA/ESA/CSA James Webspace telescope, astronomers have detected Neptune’s trihydrogen cations and distinct infrared South Aurorae.

This composite image, created using data from the NASA/ESA Hubble Space Telescope and the NASA/ESA/CSA James Webbspace Telescope, shows the aurora activity (cyan bevel) in Neptune. Image credits: NASA/ESA/CSA/STSCI/HEIDI HAMMEL, Aura/Henrik Mellin, University of Northumbria/Leafletcher, University of Leicester/Stefanie Millam, NASA-GSFC.

“In the past, astronomers have seen appetizing hints for Aurora’s activities in Neptune,” said Henrik Mellin, an astronomer at Northumbria University and his colleagues.

“However, imaging and confirmation of Aurorae in Neptune has been avoiding astronomers for a long time despite successful detections on Jupiter, Saturn and Uranus.”

“Neptune was a missing part of the puzzle when it came to detecting the giant planet of the solar system, Aurorae.”

In this study, the authors analyzed the obtained data. Webb’s Near-Infrared Spectroscopy (NIRSPEC) June 2023.

In addition to the image of the planet, astronomers have characterized the composition and acquired spectra to measure the temperature of the planet’s upper atmosphere (ionosphere).

They discovered a very prominent efflux system indicating the presence of trihydrogen cations.

“In Neptune’s Webb image, the glowing aurora appears as a spot, represented by cyan,” the astronomer said.

“The aurora activity seen in Neptune is markedly different from what we are used to seeing here on Earth, or even Jupiter and Saturn.”

“Instead of being trapped in the north and south poles of the planet, Neptune’s aurora is located in the mid-latitudes of the planet. Think about where South America is on Earth.”

“This is due to the strange nature of Neptune’s magnetic field, originally discovered by NASA’s Voyager 2 in 1989, tilting 47 degrees from the planet’s axis of rotation.”

“The activity of the aurora is based on where the magnetic field converges into the planet’s atmosphere, so Neptune’s aurora is far from the rotating pole.”

“The groundbreaking detection of Neptune’s Aurorae helps us understand how Neptune’s magnetic fields interact with particles flowing through far-flung areas of the solar system.

Researchers were also able to measure the temperature above the Neptune atmosphere for the first time since the flyby of the Voyager 2.

Their results suggest why Neptune’s Aurorae remained hidden from astronomers for a long time. The upper atmosphere of the Neptune was cooled several hundred degrees.

For many years, astronomers have predicted the strength of Neptune Aurorae based on temperatures recorded by Voyager 2.

“A rather cold temperature would result in a very prominent aurorae,” the scientist said.

“This cold temperature could be the reason why Neptune’s Aurorae remains undetected for a long time.”

“Dramatic cooling suggests that even though Earth is more than 30 times more seated from the Sun compared to Earth, this area of ​​the atmosphere can change dramatically.”

result Today I’ll be appearing in the journal Natural Astronomy.

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H. Merin et al. Discovery of h3+ JWST and Neptune’s infrared aurorae. Nut AthlonPublished online on March 26th, 2025. doi:10.1038/s41550-025-02507-9

Source: www.sci.news

Webb successfully captures images of several massive exoplanets orbiting two youthful stars

Astronomers using Near-infrared camera (NIRCAM) NASA/ESA/CSA James Webb Space Telescope equipped and captured corona graphic images of the HR 8799 and 51 Eridani Planetary Systems. These observations revealed HR 8799 and four known gas giants around 51 Eridani. They also revealed that all HR 8799 planets are carbon dioxide-rich.

This Webb/Nircam image shows the multiplanet system HR 8799. Image credits: NASA/ESA/CSA/STSCI/W. BALMER, JHU/L. PUEYO, STSCI/M. PERRIN, STSCI.

HR 8799 is a star from 30 million years ago, about 129 light years away from the Pegasus constellation.

Hosts large chip disks and four supergipers: HR 8799b, c, d, and e.

Unlike most exoplanet discoveries inferred from data analysis, these planets are seen directly via ground telescopes.

“We have shown that the atmosphere of these planets has quite a lot of heavy elements, such as carbon, oxygen and iron.

“Given what we know about the stars, it's likely that it indicates that they were formed through Core landing this is an exciting conclusion for the planet we can see firsthand. ”

The planets within HR 8799 are still hot from the formation of the turbulent, ejecting a large amount of infrared rays that provide valuable data about how scientists formed.

Giant planets can take shape in two ways. Like giants in the solar system, by slowly building heavy elements that attract gas, or the particles of gas rapidly merge into giant objects from a cooling disk of a young star made of the same kind of material as the stars.

The first process is called core accretion and the second is called disk instability.

Knowing which formation models are more common can provide clues to scientists distinguish the types of planets they have found in other systems.

“Our hope in this type of study is to understand our own solar system, life and ourselves, in comparison to other exoplanet systems.

“We want to take photos of other solar systems and see how they look similar or different from us.”

“From there we can feel how strange or normal our solar system is.”

This Webb/Nircam image shows the 51 Eridani system. Image credits: NASA/ESA/CSA/STSCI/W. BALMER, JHU/L. PUEYO, STSCI/M. PERRIN, STSCI.

51 Eridanus is located approximately 97 light years from Earth in the constellation of Eridanus.

51 If called ERI, C ERIDANI, or HD 29391, the star is only 20 million years old and by astronomy standards it is merely a toddler.

Host one giant planet, 51 Eridani B. It orbits the star at a distance of approximately 13 AU (astronomical units), equivalent to that of Saturn and Uranus in the solar system.

Images of HR 8799 and 51 rib ticks were made possible by Webb's Nircam Coronagraph.

This technique allowed astronomers to look for infrared rays emitted by planets at wavelengths absorbed by a particular gas.

They discovered that the four HR 8799 planets contain more heavy elements than previously thought.

“There is other evidence suggesting these four HR 8799 planets formed using this bottom-up approach,” says Dr. Laurent Puueyo, an astronomer at the Institute of Space Telescope Science.

“How common is this on planets we don't know yet?

“We knew that Webb could measure the colour of outer planets in a directly imaged system,” added Dr. Remi Somer of the Institute of Space Telescope Science.

“We waited for 10 years to ensure that the finely tuned operations of the telescope had access to the inner planet.”

“We now have results and we can do some interesting science.”

Survey results It was published in Astronomy Journal.

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William O. Balmer et al. 2025. JWST-TST High Contrast: Living on the Wedge, or Nircam Bar Coronagraph reveals CO2 HR 8799 and 51 ERI extracts atmosphere. AJ 169, 209; doi:10.3847/1538-3881/ADB1C6

Source: www.sci.news

Hera Asteroid Mission Captures Breathtaking Image of Deimos, Moon of Mars

Mars appears bright blue in this near-infrared image taken by Hera's spacecraft. The month's deimos is a dark mark towards the center of the image

ESA

Space exploration mission to study asteroids that NASA deliberately crashed a spacecraft three years ago takes stunning bonus images of Mars and its moon Deimos is on the way to his final destination.

NASA's 2022 Double Planet Redirect Test (DART) was an attempt to show that bodies on a collision course with the planet could be deliberately redirected to avoid catastrophic effects. Observations from Earth showed that NASA successfully alters the orbit of the asteroid by crushing the 610-kilogram ship into distant asteroid shaped leaves at 6.6 km/sec. Dimorphos did not present any risk to the Earth, and simply acted as a subject.

Hera is a subsequent European Space Agency mission designed to explore the effects of crashes in detail. The craft is the size of a small car weighing 1081 kilograms when fully fueled. It was released on October 7, 2024 from Cape Canaveral, Florida, aboard the SpaceX Falcon 9 Rocket, and on March 12, 2025 I made a flyby to Mars on my way to the asteroid.

Deimos looks dark surrounded by Mars

ESA

Hera came close to 5,000 kilometers to the surface of Mars, received a gravity boost and cast it at Dimorphos. The operation reduced travel time by months and saved fuel.

It was very close to Mars, but I was able to turn on the trio of sensors to take detailed photos of some of the planets. Demos in the same frame. We captured images, infrared cameras and hyperspectral imagers that can sense different colors beyond the limits of the human eye using a 1020 x 1020 pixel resolution.

Hera moved at 9 km/sec compared to Mars, allowing him to image Deimos, a distance of just 1000 kilometers, ranging from 12.4 kilometers long. You can also photograph the side of the moon, which is attractively trapped from Mars, but that's not very common.

Deimos shines much brighter than Mars in this shot taken by Hera's thermal infrared imager

ESA/JAXA

The first concept behind the Hera mission was that it existed when Dart collided with Dimorphos, but delays in funding made it impossible. It will arrive a few years after the impact.

The mission also features two miniature satellites, called Juventus and Milani, or Cubesat. Rather than rotating the traits, these will fly before them and make a drastic pass at smaller, risky distances to collect data. Both are expected to look better if they eventually land on an asteroid and do everything they can in the distance.

https://www.youtube.com/watch?v=hu31-crtr9s

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Source: www.newscientist.com

ARP 105: Hubble Captures Ongoing Merger of Two Massive Galaxies

The ARP 105 features star and gas tide tails that exceed 362,000 light years.



The elliptical galaxy NGC 3561B (top left) and the Spiral Galaxy NGC 3561A (bottom right) form the ongoing merger-sparking guitar shapes known comprehensively as ARP.

ARP 105 It is located approximately 400 million light years from Earth, in the constellation of Ursa major.

Also known as NGC 3561, it was discovered by British astronomer John Herschel on March 30, 1827.

It consists of two huge galaxies, the elliptical galaxy NGC 3561B and the Spiral Galaxy NGC 3561A.

“The ARP 105 is one of the brightest objects in the busy Galaxy Cluster Abell 1185,” Hubble Astronomers said in a statement.

“Abell 1185 is a chaotic cluster of at least 82 galaxies, many of which are not only interacting, but many wandering spherical clusters that are not gravity attached to a particular galaxy.”

The gravity dance between the NGC 3561B and NGC 3561A creates the features of an attractive collision galaxy.

“The giant tail is drawn from two galaxies by gravity interaction, embedding a cluster of stars and a galaxy of d star,” the astronomer said.

“The uniquely shaped arrangement of the galaxy and tail gives the grouping the nickname: guitar.”

“The long lanes of dark dust emerging from the NGC 3561b oval galaxy may be ingesting the bright blue region of star-forming at the bottom of the guitar known as Ambartsumian's Knot.”

“Ambartsumian's Knot is a tidal star galaxy. It is a type of star-forming system that develops from fragments of the tidal arms of interacting galaxies.”

“The two bright blue regions of star formation are evident in Hubble images at the edge of a distorted helical galaxy.”

“The region on the left of the spiral galaxy may be very similar to the knot of Ambartumian, the knot of intense star-forming knot caused by the merger.”

“The area on the right is still under investigation. It may be part of the collision, but its velocity and spectral data are different from the rest of the system, so it could be a galaxy in the foreground.”

“The thin, faint gas tips are barely visible that stretch between two galaxies.”

“These tendrils are of particular interest to astronomers as they may help define the timescale of this collision evolution.”

Source: www.sci.news

Hubble captures UGC 5460: A dazzling view of a face-on spiral galaxy

Astronomers using the NASA/ESA Hubble Space Telescope have produced an excellent image of the Spiral Galaxy UGC 5460.

This Hubble image shows the UGC 5460, a spiral galaxy about 60 million light years away in the URSA major constellations. Image credits: NASA/ESA/Hubble/W. Jacobson-Galán/A. Filippenko/J. Mauerhan.

UGC 5460 is It was located His major in Ursa is about 60 million light years.

Otherwise known as IRAS F10048+5205, Leda 29469, or TC 132, the galaxy is seen to be very close to face.

Two supernova explosions, named in 2011 and 2015 SN 2011ht and SN 2015ASwere observed with UGC 5460, respectively.

“Hubble targeted this galaxy because of the explosion of these two stars, collecting data from three observational programs aimed at studying different types of supernova,” says Hubble astronomers. said in a statement.

“SN 2015as was what is known as the Core Collapse Supernova. The intense events occur when the solar nucleus collapses under its own gravity, and begins to rebound material outside the core. It's an explosion.”

“The Hubble observations in SN 2015A help researchers understand what happens when the supernova's expanding shock wave collides with the gas surrounding the exploded star.”

“SN 2011HT may have been a Core Collapse Supernova, but it could also be a con man called the Luminous Blue variable.”

“The bright blue variable is a rare star that experiences eruptions so large that it can mimic a supernova.”

“Crucially, while these eruptions are intact, bright blue variables appear, but stars going to supernovae are not.”

“Hubble searches for stellar survivors at the location of SN 2011HT and it is possible that the explosion's identity will finally be revealed.”

The color image of the UGC 5460 is Hubble Wide Field Camera 3 (WFC3) UV, near-infrared, and optical parts of the spectrum.

“The image combines light of four different wavelengths to reveal the central bar of the star, a winding spiral arm, and a bright blue star cluster on the UGC 5460,” the astronomer said.

“In the upper left corner of this image there is an object much closer to it. It's a star just 577 light years away in our own galaxy.”

Source: www.sci.news

The incredible picture captures the closest Einstein ring ever seen

The closest Einstein ring ever picked up by the European Space Agency's Euclidean Space Telescope

ESA

Astronomers have identified the closest Einstein ring ever. This is a rare phenomenon in which light from even more off-the-sea galaxies bend due to the gravity of galaxies near Earth. The ring was previously thought to be one galaxy, and was identified over 100 years ago.

Such a galaxy lens, the closest astronomer to date, was predicted by Albert Einstein in 1936 from his general theory of relativity. At the time, he thought it was impossible to observe such an effect. In fact, if he had a strong enough telescope, he would have seen it. “It was there all along, but we didn't know.” Thomas Collett At the University of Portsmouth, UK.

Colette and his team are about 600 million light years from Earth, and the oval galaxy NGC 6505, first discovered in 1884, is actually the second galaxy behind about 600 million light years from Earth. I noticed that the light was bent.

Close-up of Einstein Ring

ESA/Euclid/Euclid Consortium/NASA, J.-C. Image processing by Cuillandre, T. Li

Team Members Bruno Artieri We observed Einstein rings at the European Space Agency while verifying early test data from the Euclidean telescope. “There was this abundant and obvious Einstein ring. There aren't many in the universe that can produce rings like this,” says Colette.

“We would have expected about one of three opportunities to find something as spectacular as this throughout the research,” he says. “It's essentially a great fortune to find it in the first data. This is probably the most beautiful lens we find on a mission.”

The ring itself is very bright compared to most Einstein rings we know, Colette says. This is not only very close to us, but also due to the Euclidean imaging capabilities. “I'm like someone with poor eyesight,” says Colette. This makes it easy to see four images of distant galaxies. The faint orange lights surrounding the bright ring are the galaxy of Rensing.

Bringing the Einstein ring closer to Earth allows us to test relativity in ways that we cannot do with other distant lenses, says Colette. This is because galaxies can be measured in two ways. , often too far to measure accurately. Einstein's general theory of relativity states that these masses should be the same, so if there are differences it may suggest that the theory of gravity should be revised.

When Colette and his colleagues measured the mass of the lensed galaxy, they also found a slightly higher number than possible from the galaxy's estimated number of stars. This could be due to the dark matter aggregation together at Galaxy's Center. Frédéric Dux He says observatory in southern Europe needs to find more Einstein lenses to check.

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Source: www.newscientist.com

Hubble captures Type IA Super Shinsei and its host galaxy in stunning detail

Two years ago, a type IA supernova event called SN 2022ABVVT was discovered in Spiral Galaxy LEDA 132905.



This Hubble image LEDA 132905, a spiral galaxy over 400 million light years in sculptor constellation. Image credit: NASA / ESA / Hubble / RJ Foley, UC Santa cruz.

LEDA 132905 in the sculptor’s constellation is over 400 million light years away.

“The galaxy’s spiral structure, resembling a bright blue star patch, appears faint,” said members of the Hubble team.

“The bright white dot between the bright center of the galaxy and the faint left end is the SN 2022ABVVT supernova.”

The supernova SN 2022ABVT was discovered in 2022 by astronomers of the asteroid landlady impacted alert system (ATLAS).

About two months later, the NASA/ESA Hubble Space Telescope observed the star explosion.

“Atlas, designed to track faint-moving signals from asteroids near Earth, also detects objects that suddenly become brighter or fade, like supernovae in the centers of galaxies, various stars, and hungry black holes,” astronomers explained.

This Hubble image of LEDA 132905 was captured using the Hubble wide field camera 3 (WFC3) in the infrared part of the spectrum.

Astronomers are interested in studying type IA supernovae, which occur when the exposed core of ancient stars ignites in a sudden and destructive nuclear fusion burst.

These supernovae are valuable for measuring accurate distances to other galaxies.

“The universe is vast, and supernova explosions are faint,” researchers stated.

“How can we be in the right place at the right time to observe a supernova?”

“Today, most supernovae are discovered by robot telescopes constantly scanning the night sky.”

“However, some are still found the traditional way, with diligent observers taking repeated images of the sky and searching for any changes.”

Source: www.sci.news

BepiColombo captures images of Mercury’s shadowed craters and volcanic lands

The bright and dark part of Mercury's north pole seen from the BepiColombo spacecraft

ESA/BepiColombo/MTM

These images illustrate the pockmarked surface of Mercury and are a preview of what to expect as the BepiColombo mission enters orbit around the innermost region of our solar system in late 2026.

Since its launch in 2018, the joint Japan-Europe spacecraft BepiColombo has made six flybys of Mercury, gradually decelerating with each pass to fine-tune its trajectory for orbital insertion. While the mission’s primary scientific instruments are yet to be utilized, the spacecraft’s cameras have already provided detailed images of the planet.

The European Space Agency (ESA) recently released three striking images captured during BepiColombo’s latest flyby on January 8, taken from an altitude of around 300 kilometers above Mercury’s north pole and northern regions.

David Rothery, from the Open University, UK, shared his excitement about the images, saying, “We had to wake up early to see these close-ups, and they exceeded our expectations based on simulated views we studied beforehand.”

The image above showcasing Mercury’s north pole reveals the sharp contrast between light and darkness on the planet, known as the terminator line. This region shows extreme temperature variations, with some areas exposed to scorching sunlight while others remain perpetually shaded within craters.

Notably, shadowed regions containing potential frozen water deposits can be observed along the terminator line in the image. Rothery further highlights the fascinating details visible, such as the sunlit peak inside Tolkien Crater, providing key insights for the mission’s scientific objectives.

Scientific investigations suggest that these shadowed crater areas may harbor frozen water, a key aspect of BepiColombo’s mission to uncover the presence and extent of water on Mercury.

Mercury's vast volcanic plain known as Borealis Planum

ESA/BepiColombo/MTM

Mesmerizing images from BepiColombo’s mission highlight Mercury’s expansive volcanic plain known as Borealis Planitia, formed over 3 billion years ago from massive lava flows that engulfed existing craters, some of which are visible in the image. While most of these plains are relatively smooth, more recent impact craters provide intriguing targets for scientific study.

Spanning 1,500 kilometers, the Caloris Basin is the largest crater on Mercury, appearing as a semicircular light-colored feature on the planet’s surface. Once BepiColombo enters orbit, researchers aim to investigate the relationships between the Caloris Basin, Borealis Planitia, and the solidified lava flows connecting them.

Natal Facula, believed to be the remains of the largest volcanic eruption in Mercury's history, is seen as a bright spot in this image.

ESA/BepiColombo/MTM

The illuminated region at the top of the planet, known as Natal Facula, is believed to be the aftermath of Mercury’s most significant volcanic eruption. The presence of a central crater, approximately 40 kilometers wide, indicates multiple eruptions that scattered volcanic material over hundreds of kilometers.

Rothery expresses eagerness for future observations of Natal Facula by BepiColombo’s instruments, emphasizing its scientific importance in understanding Mercury’s volcanic history. Discovering the reasons behind Mercury’s enduring volcanic activity remains a key goal of the mission.

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  • solar system/
  • space exploration

Source: www.newscientist.com

DECam captures close-up of the Antria galaxy cluster

The Antria Galaxy Cluster is a group of at least 230 galaxies brought together by gravity. This galaxy cluster is rare. Unlike most other galaxy clusters, there appears to be no dominant galaxy within it.


The Antria star cluster is dominated by two giant elliptical galaxies: NGC 3268 (center) and NGC 3258 (bottom right). Image credits: Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA / R. Colombari & M. Zamani, NSF's NOIRLab.

Galaxy clusters, like stars and galaxies, are fundamental building blocks of the universe.

These structures typically contain thousands of galaxies of all ages, shapes, and sizes.

They have a mass about a million times the mass of the Sun and are formed over billions of years as groups of small galaxies slowly come together.

At one point, galaxy clusters were believed to be the largest structures in the universe, until they were supplanted by the discovery of superclusters in the 1980s. Its length spans hundreds of millions of light years.

However, there is one thing the cluster holds on to. Because superclusters are not held together by gravity, galaxy clusters still hold the title of the largest gravitationally bound structures in the universe.

“Galaxy clusters are some of the largest known structures in the known universe,” NOIRLab astronomers said in a statement.

“Current models suggest that these giant structures form as clumps of dark matter, and that the galaxies that form within them are pulled together by gravity to form groups of dozens of galaxies, which then merge to form groups of several dozen galaxies. This suggests that they form clusters of hundreds or even thousands of galaxies.

“One such group is antoria clusterlocated approximately 130 million light-years from Earth in the direction of the constellation Antolia. ”

The Antlia cluster, also known as Abell S636, 3rd closest Add it to the local group after the Virgo and Fornax clusters.

The new images of the Antolia star cluster were captured by the Dark Energy Camera (DECam) mounted on NSF's Victor M. Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile, a program of NSF's NOIRLab.

It captures only a portion of the 230 galaxies so far discovered to make up this cluster, as well as thousands of background galaxies.

“Antria Cluster” host Two giant elliptical galaxies: NGC3268 and NGC 3258,” the astronomers said.

“These central galaxies are surrounded by numerous faint dwarf galaxies.”

“Based on X-ray observations that revealed the existence of a 'rope' of globular clusters along the optical peak region between these two galaxies, we believe that these two galaxies are in the process of merging. Masu.”

“This may be evidence that the Antlia cluster is actually two smaller clusters joined together.”

“The cluster is rich in lenticular galaxies (a type of disk galaxy with little interstellar medium and therefore little continuous star formation), as well as some irregular galaxies,” the researchers added. .

“Many rarer, lower-luminosity dwarf galaxies have been discovered within this cluster, including ultracompact dwarfs, compact elliptical galaxies, and blue compact dwarfs.”

“The Antria cluster may also contain subtypes of dwarf spheroidal and superdiffuse galaxies, but further investigation is needed to confirm these.”

“Many of these galaxy types have been identified within the past few decades, as advances in observational instruments and data analysis techniques have allowed us to better capture the low luminosity and relatively small size of these galaxies. It just happened.”

“Assessing galaxy types allows us to plot details of their evolution, and some galaxies are rich in dark matter, providing further opportunities to understand this mysterious material, which makes up 25% of the universe. We will provide it.”

Source: www.sci.news

Hubble Captures Stunning Image of Barred Spiral Galaxy NGC 2566

Astronomers using the NASA/ESA Hubble Space Telescope have taken striking new photos of barred spiral galaxy NGC 2566.

The barred spiral galaxy NGC 2566 has a prominent star bar at its center, with spiral arms emerging from each end of the bar. Image credit: NASA / ESA / Hubble / D. Tilker.

NGC2566 It is located in the constellation Leo, about 76 million light years away from Earth.

The galaxy was discovered by German-British astronomer William Herschel on March 6, 1785.

Also known as ESO 495-3, LEDA 23303, or UGCA 138, this galaxy is a member of the PGC 80593 group of at least 16 large galaxies.

“NGC 2566 appears tilted from our perspective, so its disk is almond-shaped, giving the galaxy the appearance of a cosmic eye,” Hubble astronomers said in a statement.

“As NGC 2566 stares back at us, we’ll be looking directly behind it, using Hubble to study the galaxy’s star clusters and star-forming regions.”

“Hubble data is especially valuable for studying stars that are only a few million years old.”

“These stars are bright in the ultraviolet and visible wavelengths to which Hubble is sensitive.”

Using these data, astronomers will measure the ages of NGC 2566’s stars, helping them piece together the timeline of star formation in the galaxy and gas exchange between the star-forming clouds and the stars themselves.

“Several other observatories have investigated NGC 2566, including NASA/ESA/CSA’s James Webb Space Telescope,” the researchers said.

“Webb’s data complement this Hubble image, adding a view of NGC 2566’s warm, glowing dust to Hubble’s stellar portrait.”

“NGC 2566, at the long wavelength end of the electromagnetic spectrum, has also been observed by the Atacama Large Millimeter/Submillimeter Array (ALMA).”

“ALMA is a network of 66 radio telescopes working together to capture detailed images of the gas clouds where stars form.”

Source: www.sci.news

The Hubble Space Telescope captures an off-center spiral galaxy

Astronomers using the NASA/ESA Hubble Space Telescope have provided an unparalleled snapshot of intermediate spiral galaxy NGC 1637.

This Hubble image shows NGC 1637, an intermediate spiral galaxy located about 38 million light-years away in the constellation Eridanus. Image credit: NASA / ESA / Hubble / D. Tilker.

NGC1637 It is located in the constellation Eridanus, about 38 million light years from Earth.

This galaxy, also known as LEDA 15821 or UGCA 93, is located around this galaxy. 30,000 light years Across.

it was discovered It was discovered on February 1, 1786 by German-British astronomer William Herschel.

At first glance it looks like NGC1637 will be displayed Despite being a fairly symmetrical galaxy, it has some interesting features that have led astronomers to classify it as a biased spiral galaxy.

“The new images of NGC 1637 come from an observational program dedicated to studying star formation in nearby galaxies,” Hubble astronomers said.

“Stars form in cold, dusty gas clouds that collapse under their own gravity.”

“As young stars grow, they heat the nursery with starlight, wind, and strong outflow.”

“Together, these factors play a role in controlling the rate of star formation in future generations.”

“Evidence of star formation is scattered around NGC 1637, if you know where to look.”

“The spiral arms of the galaxy are dotted with what look like pink clouds, many with bright blue stars.”

“The pinkish color comes from hydrogen atoms excited by ultraviolet radiation from young, massive stars.”

“This contrasts with the warm yellow glow at the galactic center, where older, redder stars are densely clustered.”

“The stars that sparkle their birthplaces are relatively short-lived, and many of these stars explode as supernovae just a few million years after their birth.”

In 1999, Lick Observatory's supernova search discovered a type II supernova in NGC 1637.

named SN 1999emThis supernova was hailed as the brightest supernova observed that year.

It has been closely tracked by astronomers and has been shown to have dimmed relatively slowly over the years.

“When a massive star annihilates as a supernova, its explosion outstrips its entire home galaxy for a short period of time,” the astronomers said.

“Supernovae mark the end of a star's life, but by compressing nearby gas clouds, they can also jump-start the formation of new stars, starting a star's life anew.”

Source: www.sci.news

VLTI captures high-resolution images of red supergiant star in Large Magellanic Cloud

used by astronomers ESO’s Very Large Telescope Interferometer (VLTI) has taken an enlarged image of the dusty red supergiant star WOH G64.

This image, taken by ESO’s Very Large Telescope Interferometer’s GRAVITY instrument, shows the red supergiant star WOH G64. Image credit: ESO / Onaka others., doi: 10.1051/0004-6361/202451820.

WOH G64 is located in the constellation Shira, about 160,000 light years away.

The star, also known as IRAS 04553-6825, 2MASS J04551048-6820298, or TIC 30186593, is part of the Large Magellanic Cloud, one of the smaller galaxies orbiting the Milky Way.

WOH G64 is approximately 2,000 times larger than the Sun and is classified as a red supergiant star.

“We discovered an egg-shaped cocoon that tightly surrounds this star,” said Dr. Keiichi Onaka, an astrophysicist at Andres Bello University.

“We’re excited because this could be related to the rapid ejection of material from a dying star before it explodes into a supernova.”

“Astronomers have taken zoomed-in images of and characterized about two dozen stars in our Milky Way galaxy, but countless other stars exist in other galaxies. and were so far away that it was very difficult to observe one of them in detail.

Artist’s reconstruction of the red supergiant star WOH G64. Image credit: ESO/L. Calçada.

Dr. Onaka and his colleagues have been interested in WOH G64 for a long time.

In 2005 and 2007, they used VLTI to learn more about the star’s properties and continued their research in the years since. However, the actual appearance of this star remained elusive.

To achieve the desired photos, it was necessary to wait for the development of VLTI’s second generation equipment. gravity.

After comparing the new results with other previous observations of WOH G64, they were surprised to find that the star had become fainter over the past decade.

Professor Gerd Weigert, an astronomer at the Max Planck Institute for Radio Astronomy, said: “We found that this star has undergone significant changes over the past 10 years, and this is a rare opportunity to witness the life of a star in real time.” he said. .

During the final stages of their lives, red supergiant stars like WOH G64 shed their outer layers of gas and dust in a process that lasts thousands of years.

Dr Jacco van Loon, director of the Kiel Observatory at Kiel University, said: “This star is one of the most extreme of its kind and any dramatic changes could bring it closer to an explosive demise. ” he said.

“These ejected materials may also be responsible for the dimming and the unexpected shape of the dust cocoon around the star,” the astronomers said.

The new image shows the cocoon elongating, surprising researchers who had expected a different shape based on previous observations and computer models.

They believe that the cocoon’s egg-like shape could be explained by the star’s molting or the influence of an as-yet-undiscovered companion star.

As the star dims, it becomes increasingly difficult to take other close-up photos, even VLTI.

Nevertheless, in the future, an update of the telescope’s instruments is planned. Gravity+I promise to change this soon.

“Similar follow-up observations using ESO’s instruments will be important for understanding what is happening inside this star,” said Dr. Onaka.

of the team paper Published in a magazine astronomy and astrophysics.

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Kento Ohnaka others. 2024. Image of the innermost circumstellar environment of the red supergiant star WOH G64 in the Large Magellanic Cloud. A&A 691, L15; doi: 10.1051/0004-6361/202451820

Source: www.sci.news