Stunning images of NGC 4689 captured by Hubble

Astronomers using the NASA/ESA Hubble Space Telescope have captured sharp images of NGC 4689, a jewel-bright spiral galaxy in the constellation Coma.



This Hubble image shows spiral galaxy NGC 4689 located 52 million light-years away in the constellation of Coma. Image credits: NASA / ESA / Hubble / D. Tilker / J. Lee / PHANGS-HST Team.

NGC 4689 It is located approximately 52 million light-years away in the constellation Kamina.

“Of the 88 constellations officially recognized by the International Astronomical Union (IAU), Coma has the distinction of being the only constellation named after a historical figure. Queen Berenice II of Egypt” explained the Hubble astronomer.

“The Latin word ‘coma’ refers to her hair, meaning that NGC 4689 can be said to be present in the Queen’s hair.”

“Some of Berenice’s contemporaries may have meant this quite literally; her court astronomer believed that Berenice’s lost locks had been destroyed by God (“among the stars”). It was given this name because there is a story that it was thought to have been placed in It is the constellation of Coma. ”

NGC 4689 is discovered It was proposed by German-born British astronomer William Herschel on April 12, 1784.

Also known as LEDA 43186 or UGC 7965, this galaxy is a member of the Virgo Cluster, a group of more than 2,000 galaxies.

NGC 4689 is tilted 36 degrees and can be viewed almost head-on.

The new images of the galaxy were created from separate exposures taken in the ultraviolet, visible, and near-infrared spectral regions. Hubble’s Wide Field Camera 3 (WFC3).

This is based on data obtained through a gender filter. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

“This image was created using two sets of observations taken in 2019 and 2024, both as part of a program to observe multiple ‘nearby’ galaxies.” Astronomy said the people.

The 2024 observing program is an interesting example of how Hubble, a relatively old but highly productive telescope, can support the work of the technologically cutting-edge Webb Telescope. ”

“Observations collected by Webb change our understanding of how galaxies change and evolve over time by providing data of unprecedented detail and clarity. It will be.”

“But thanks to their complementary capabilities, new observations from Hubble (such as those used to create new images) can aid the work being done using the Web.”

“In this case, the Hubble data were collected to better understand the stellar populations of nearby galaxies, which is critical to understanding the evolution of galaxies.”

“NGC 4689 therefore plays an important role in advancing our understanding of how all galaxies evolve.”

Source: www.sci.news

Stunning images of small spiral galaxies captured by Hubble

Astronomers using the NASA/ESA Hubble Space Telescope have captured an excellent image of the spiral galaxy ESO 422-41 in the constellation Columba.

This Hubble image shows ESO 422-41, a spiral galaxy located in the constellation Columba, about 34 million light-years away. Image credit: NASA / ESA / Hubble / C. Kilpatrick.

ESO 422-41 It is located in the constellation Columba, about 34 million light years away.

DDO 230, LEDA 16864, or UGCA 103, the diameter of this spiral galaxy is 30,000 light years.

“The name ESO 422-41 comes from its appearance in the European Southern Observatory (B) Atlas of the Southern Sky,” Hubble astronomers said.

“In the era before automated sky surveys by space observatories such as ESA's Gaia satellite, large-scale photographic surveys discovered many stars, galaxies, and nebulae.”

“Astronomers used the then most advanced large telescopes to create hundreds of photographs covering parts of the sky.”

“They then studied the resulting photographs and attempted to catalog all the new objects revealed.”

“In the 1970s, a new telescope at ESO's La Silla facility in Chile probed the southern sky, which had not yet been explored as deeply as the northern sky,” they added.

“At that time, the primary technology for recording images was glass plates treated with chemicals.”

“The resulting collection of photographic plates became the ESO (B) Atlas of the Southern Sky.”

“Astronomers from ESO and Uppsala, Sweden, worked together to study the plates and recorded hundreds of galaxies (ESO 422-41 is just one of them), star clusters and nebulae. I was a beginner.”

“Since then, astronomical sky surveys have progressed from digital, computer-aided surveys such as the Sloan Digital Sky Survey (SDSS) and Legacy Survey to surveys performed by space telescopes such as Gaia and the Wide-Field Infrared Survey Explorer (WISE). It has transitioned to

“Nonetheless, photographic sky surveys have made significant contributions to astronomical knowledge over the decades, and the glass plate archive serves as an important historical reference for a wide range of skies. .”

“Some of them are still actively used, for example, to study variable stars over time,” the researchers pointed out.

“And the objects revealed by these surveys, including ESO 422-41, can now be studied in detail with telescopes like Hubble.”

The new images of ESO 422-41 consist of observations from Hubble's advanced survey camera (ACS) in the near-infrared and optical portions of the spectrum.

Two filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

Source: www.sci.news

Close-Up View of Io’s Unique Features Captured by NASA’s Juno Mission

In December 2023 and February 2024, NASA’s Juno spacecraft will fly extremely close to Jupiter’s volcanic moon Io, coming within about 1,500 kilometers (930 miles) of the surface and obtaining the first close-up images of the moon’s northern latitudes. Planetary scientists have now turned images collected during the flight into animations that show two of Io’s most dramatic features: its mountains and a nearly glassy rock formed by cooling lava called Loki Patera. It emphasized the smooth lake.

The JunoCam instrument aboard NASA’s Juno spacecraft imaged Io, the most geologically active object in the solar system, on February 3, 2024, from a distance of approximately 7,904 km (4,911 miles) . Image credit: NASA/SwRI/MSSS.

“There are only a few scattered volcanoes on the island of Io, and we captured some of them active,” said Juno principal investigator and Southwest Research Institute cosmologist. said Scott Bolton, director of science and engineering.

“We also obtained great close-ups and other data about a 200 km (127 mile) long lava lake called Loki Patera.”

“It shows in amazing detail how these crazy islands are embedded in the middle of a potential magma lake fringed with hot lava.”

“The specular reflections that our instruments record about the lake suggest that parts of Io’s surface are glass-smooth, reminiscent of the obsidian glass produced in volcanoes on Earth. “

Map generated using data collected by Juno microwave radiometer (MWR)’s instruments revealed that Io not only has a relatively smooth surface compared to Jupiter’s other Galilean moons, but also has poles that are colder than the mid-latitudes.

During Juno’s long-term mission, the spacecraft will fly closer to Jupiter’s north pole with each pass.

This change in direction allows the MWR instrument to improve the resolution of Jupiter’s polar cyclones.

This data allows us to compare multiple wavelengths at the poles and reveals that not all polar cyclones are created equal.

“Perhaps the most striking example of this difference is seen in the central cyclone at Jupiter’s north pole,” said Dr. Steve Levin, Juno project scientist and researcher at NASA’s Jet Propulsion Laboratory. states.

“Although clearly visible in both infrared and visible light images, the microwave signature is not as strong as other nearby storms.”

“This indicates that its subsurface structure must be very different from other cyclones.”

“As the MWR team continues to collect more and better microwave data in every orbit, we expect to develop more detailed 3D maps of these interesting polar storms.”

Source: www.sci.news

Young multi-star system captured in stunning Hubble Space Telescope photos

A new image from the NASA/ESA Hubble Space Telescope shows a jet emerging from the cocoon of the multistar system FS Tau.



This Hubble image shows the multistar system FS Tau about 450 light-years away in the constellation Taurus. Image credit: NASA / ESA / K. Stapelfeldt, NASA Jet Propulsion Laboratory / Gladys Kober, NASA / Catholic University.

FS Tau It is located about 450 light years away in the constellation Taurus.

The system is part of the Taurus-Auriga region, a collection of dark molecular clouds that is home to many newly formed young stars.

FS Tau, also known as HH 157 or TIC 58437437, is only about 2.8 million years old, making it an extremely young star system.

FS Tau is a multi-star system consisting of FS Tau A, a bright star-like object near the center of the image, and FS Tau B, a bright object on the far right hidden by a dark vertical dust lane. ''' said the Hubble astronomer.

“The young object is surrounded by gently illuminated gas and dust in this stellar nursery.”

“FS Tau B is a protostar surrounded by a protoplanetary disk. A protoplanetary disk is a pancake-like collection of dust and gas left over from star formation that eventually coalesces to form a planet. It will be.”

“A thick lane of dust seen almost head-on separates what is believed to be the illuminated surface of the flared disk.”

“FS Tau B is probably T TauriAlthough nuclear fusion has not yet begun, it is a type of young variable star that is beginning to evolve into a hydrogen-fueled star similar to the Sun. ”

“Protostars glow because of the thermal energy released when the gas clouds from which they formed collapse, and from the accretion of material from nearby gas and dust.”

“Variable stars are a type of star whose brightness changes significantly over time.”

“FS Tau A itself is a Tauri T binary system, consisting of two stars orbiting each other,” the researchers added.

“Protostars are known to emit fast-moving columns of energetic material called jets, and FS Tau B provides a striking example of this phenomenon.”

“Protostars are the source of the unusual, asymmetric, double-sided jets that appear blue here.”

“Their asymmetric structure may be due to differences in the rate at which mass is ejected from the object.”

“FS Tau B is Herbig halo object,” they said.

“Herbig halo objects form when jets of ionized gas emitted by young stars collide at high speed with nearby clouds of gas and dust, forming bright nebular patches.”

Source: www.sci.news

Stunning Shot of Spider Galaxy Captured by Hubble Space Telescope

New photos from the NASA/ESA Hubble Space Telescope show nearby irregular galaxy UGC 5829, also known as the Spider Galaxy.

This Hubble image shows UGC 5829, an irregular galaxy located approximately 30 million light-years away in the constellation Sera. Image credits: NASA / ESA / Hubble / R. Tully / M. Messa.

UGC 5829 It is located approximately 30 million light-years away in the constellation Serra.

“Although this relatively faint galaxy has not been observed very often, it has the characteristic soubliquet of a spider galaxy,” Hubble astronomers said in a statement.

“Perhaps the distorted galactic arms with glowing tips that form stars remind us of the clawed legs of arachnids.”

“Somewhat confusingly, there is another galaxy known as the Spiderweb galaxy that has a very similar nickname but is otherwise completely separate.”

“Despite the fact that this galaxy is about 300 times further away from Earth than the Spider Galaxy, it has been imaged more extensively.”

“Fortunately, the ability to accurately identify galaxies does not depend on chance names.”

“Rather, known galaxies are recorded in at least one catalog, such as the Uppsala Galaxy Catalog, and are often recorded in multiple catalogs. It has been given a name.”

“This same galaxy has been given several different names in various other catalogs,” they added.

“For example, LEDA 31923 in the Lyon-Meudon Extragalactic Database; MCG+06-24-006 in the Galactic Morphology Catalog; and SDSS J104242.78+342657.3 in the Sloan Digital Sky Survey Catalog.

“Spiderweb galaxies are not all recorded in the same catalog; each catalog is necessarily limited in scope. However, they are included in the LEDA catalog as LEDA 2826829.”

“It's clearly easier to avoid confusing the boring but unique names LEDA 31923 and LEDA 2826829 than the interesting but easily confused names Spider and Spiderweb.”

The new image of UGC 5829 consists of observations from. Hubble's advanced survey camera (ACS) and wide field camera 3 (WFC3) Found in the near-infrared and optical portions of the spectrum.

This is based on data obtained through four filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

Source: www.sci.news

New Stunning Images of Jupiter Captured by Hubble Space Telescope

The new Hubble images taken on January 5 and 6, 2024 show many large storms and small white clouds in Jupiter’s atmosphere, indicating a lot of activity.



Jupiter is revisited by the NASA/ESA Hubble Space Telescope in these images taken on January 5 and 6, 2024, capturing both sides of the giant planet. Image credit: NASA / ESA / STScI / Amy Simon, NASA Goddard Space Flight Center.

Jupiter’s colorful clouds create a constantly changing display of shapes and colors in its atmosphere.

The planet experiences various stormy weather patterns, including low-pressure systems, high-pressure systems, wind shear, and the Great Red Spot, the largest storm in the solar system.

Jupiter is covered by a cloud of ammonia ice crystals, about 48 km thick in an atmosphere that is tens of thousands of kilometers deep, resulting in the planet’s distinctive stripes.

The banding effect is caused by air moving at different latitudes and speeds of up to 563 km per hour.

The zones, where the atmosphere rises, are brightly colored, while the belts, where the air falls, are darker. Storms and turbulence occur when these opposing flows interact.

Hubble continues to monitor Jupiter and other exoplanets annually through the Outer Planet Atmosphere Legacy (OPAL) Program.

“The left Hubble image shows the iconic Great Red Spot prominently in Jupiter’s atmosphere,” stated Hubble astronomers.

“To the lower right is a feature known as Red Spot Junior, a high-pressure system resulting from storms in previous years.”

“This year, it appears to be turning red again, possibly due to compounds like sulfur and phosphorus.”

“In the right image, storm activity is visible in the opposite hemisphere, with two distinct storm systems rotating in opposite directions.”

These storms are expected to pass each other as they repel through their rotations.

“The presence of many storms and clouds in Jupiter’s atmosphere indicates a high level of activity,” said Dr. Amy Simon, OPAL project leader and astronomer at NASA Goddard Space Flight Center.

“Despite its small size, Jupiter’s moon Io shows volcanic activity, visible through Hubble’s sensitivity to blue and violet wavelengths.”

Source: www.sci.news

Gigapixel Images of Bella Supernova Remnant Captured by Dark Energy Camera

Astronomers harness powerful energy dark energy camera The Victor M. Blanco 4-meter Telescope (DECam) at Cerro Tororo Inter-American Observatory, a program of NSF's NOIRLab, Huge 1.3 gigapixel image The Vela supernova remnant is the remains of a giant star that exploded in the constellation Vela about 11,000 years ago.

This DECam image shows the Vela supernova remnant, the remnant of a supernova explosion 800 light-years away in the southern constellation of Vela. Image credits: CTIO / NOIRLab / DOE / NSF / AURA / TA University of Alaska Anchorage Chancellor and NSF's NOIRLab / M. Zamani and D. de Martin, NSF's NOIRLab.

of Bella supernova remnantVela SNR for short, is one of the most well-studied supernova remnants in the sky and one of the closest supernova remnants to Earth.

Its progenitor star exploded 11,000 to 12,300 years ago south of the constellation Vore.

The association of this supernova remnant with the bella pulsar, made by Australian astronomers in 1968, provided direct observational evidence that supernovae form neutron stars.

“When this star exploded 11,000 years ago, its outer layer was violently stripped away and splattered around, creating a shock wave that can still be seen today,” the astronomers said in a statement.

“As the shock wave spreads into the surrounding region, hot, energetic gas flies away from the point of explosion, becomes compressed and interacts with the interstellar medium, producing the blue and yellow thread-like filaments seen in the image. .”

“Vela SNR is a gigantic structure, almost 100 light-years long and 20 times the diameter of a full moon in the night sky.”

“Although the star's final moments were dramatic, he did not completely disappear.”

“After the outer layers were shed, the star's core collapsed into a neutron star, an ultra-dense ball of protons and electrons that collided with each other to form neutrons.”

“The neutron star, named Bela pulsar, is now a supercondensed object containing the mass of a Sun-like star in a sphere just a few kilometers in diameter.”

“The Bela pulsar, located in the lower left region of this image, is a relatively faint star and indistinguishable from the thousands of objects next to it.”

Vela SNR's new image is the largest DECam image ever published, containing an astonishing 1.3 gigapixels.

“The striking reds, yellows, and blues in this image were achieved by using three DECam filters, each collecting a specific color of light,” the researchers said.

“Separate images were taken with each filter and stacked on top of each other to produce this high-resolution color image showing the intricate web-like filaments snaking throughout the expanding gas cloud.”

Source: www.sci.news

First sighting of Asian elephant burying carcass captured

Elephant pulling a dead calf in a tea plantation in northern Bengal, India

Parveen Kaswan and Akashdeep Roy

Asian elephants intentionally burying the bodies of their calves has been documented in the first scientific report of such behavior in this species.

Five calves were found buried in a drainage ditch on a tea plantation in the northern state of Bengal, India, with their feet and legs sticking out of the ground.

Footprints and scat of various sizes indicate that members of the herd of all ages contributed to each burial. A night watchman at the complex reported hearing loud elephant cries, sometimes lasting 30 to 40 minutes, before the herd left the area.

Akashdeep Roy Researchers at the Indian Institute of Science Education and Research in Pune and Parveen Kaswan from the Indian Forest Service suggest that the sound of these bugles may represent mourning, and that during burials the herds are “helping and caring”. It suggests that the person exhibited a certain behavior.

“The burial of a calf is an extremely rare event in nature,” says Roy.

They were surprised to find the calf buried foot-deep, but if the herd had buried each calf together, this would be the most accessible position to place the carcass in the drain. , says Roy. For elephants, who are social animals, burying their calves' heads may be the most important thing they do, he says.

A baby elephant buried in a tea garden with its feet sticking out of the ground

Parveen Kaswan and Akashdeep Roy

The calf's body was later exhumed and examined. Their ages ranged from three months to one year old, and many were malnourished and suffering from infections. Bruises along each calf's back suggest that they were dragged or carried long distances to the burial site.

African bush elephant (african loxodonta) have been observed covering carcasses with plants and returning to the location later. However, the Asian elephant (maximum elephas) In this study, we typically avoided returning to the burial site and used an alternative route instead.

“These observations provide impressive evidence of the social complexity of elephants,” he says. Chase LaDue At the Oklahoma City Zoo and Botanical Garden. “Some people have suggested that elephants seem to behave in a unique way towards their deceased relatives. [but] This paper is the first to describe what appears to be a methodical and planned burial of an elephant calf after it was taken to a burial site. ”

Still, Professor Radu said: “We must be careful how we interpret these results, especially since the mental and emotional lives of elephants remain largely a mystery to us.” There is.

He is not convinced that the position of the calf was intentional. “I could imagine an elephant pushing a dead calf into a narrow ditch, and given its awkward shape and weight distribution, the calf would land on its back with its legs in the air,” he says. “And because the depth of the trench is shallow, the feet are not buried, but this is not due to intentional burying of the head, but due to the unique topography of the burial site.”

The land where elephants once roamed freely is shrinking as humans expand, especially in India, the world's most populous country. Only about 22 percent of the land used by elephants is within protected areas.

“Understanding how elephants behave and respond to rapid changes in human-dominated landscapes may help develop conservation strategies that promote human-elephant coexistence.” Mr. Radu says.

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Source: www.newscientist.com

Top 10 Groundbreaking Medical Advancements: Pure Moments of Eureka captured in Photos

The history of science is filled with moments of discovery, those “Eureka” moments when a theory is proven or a breakthrough is achieved. The latest image competition at Great Ormond Street Hospital, titled ‘A Moment of Discovery’, celebrates these breakthroughs.

Staff from Great Ormond Street Children’s Hospital NHS Foundation Trust (GOSH) and its partners have submitted images capturing significant milestones in research. The public voted on the three most popular images shortlisted by a panel of experts via social media.

The shortlisted images range from colorful micrographs to cartoon illustrations, offering a glimpse into the research conducted at GOSH. It is hoped that this research will lead to new treatments for rare and complex conditions, transforming the lives of children and young people with serious illnesses.

The winning image, taken by PhD student Giada Benedetti at the Zayed Pediatric Rare Disease Research Center (ZCR), shows exploding intestinal organoids revealing their inner workings.

Organoids are small three-dimensional tissue cultures derived from stem cells that can mimic different organs like the heart and liver in the human body.

In honor of Rare Disease Day on February 29, all winning and shortlisted images will be displayed at an event at the Zayed Pediatric Rare Disease Research Center.

Selected as a finalist – my lungs are on fire

These lung “mini-organs,” or organoids, were grown from stem cells to replicate the complexity of lungs. The image showcases cell nuclei in blue, cell membranes in red, and moving hair-like structures called cilia in yellow/orange. Photo courtesy of Giuseppe Cala at GOSH.

Shortlist – Active Glial Cells

The image showcases nerve helper cells, known as glial cells, with long fibrous structures that transport nutrients and oxygen to surrounding nerve cells. Photo courtesy of Lucien Bonfante at GOSH.

Finalist – Light of Life

The image shows the spinal cord of a zebrafish embryo with different neurons generated through asymmetric division. Photo courtesy of Atachapon Theppichaiyanond at GOSH.

Source: www.sciencefocus.com

First-ever photograph of a majestic yellow ibis bird captured

First photo of Kijimozu

Matt Brady/University of Texas at El Paso

A rare bird with a spectacular yellow crown has been photographed for the first time in the tropical mountains of the Democratic Republic of Congo, almost 20 years after it was last seen.

Yellow-bellied shrike (Prionops alberti)Also known as the King Albert Shrike, it is a small bird that lives in the damp forests of the Albertine Rift Mountains in Central Africa. Adults are covered in glossy black feathers, with a magnificent crown of bright golden feathers on their heads. Their eyes are surrounded by distinctive orange tissue called wattles.

After not being seen for many years, the long-eared shrike was listed as an endangered species. Find a lost bird partnership.

michael harvey Researchers at the University of Texas at El Paso finally encountered this phenomenon again during a six-week expedition into the Itobwe Mountains from December 2023 to January 2024.

As team members wandered through the cloud forest, they encountered a flock of elusive birds.

“It was a shocking experience to come across these birds. I knew it might be possible here, but I wasn't prepared for how spectacular and unique it would be in my life.” ,” Harvey said in a statement.

A total of 18 Long-tailed Shrikes were spotted at three locations during the expedition. This suggests that there may be healthy populations of birds currently considered vulnerable by the International Union for Conservation of Nature.

The group also developed the red-bellied mushroom frog (Articular leptis hematogaster), last seen in the 1950s.

“Now is a great time to protect these tropical forests so we don't lose species like the long-eared shrike before they are known and studied,” Harvey said. Ta.

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Source: www.newscientist.com

Stunning marine life captured in underwater photography contest

Gannet diving

Kat Chou/UPY 2024

Snow-white northern booby (Moras Bassanus) In this action-packed photo, a man dives for food in the icy waters off the coast of Scotland's Shetland Islands. The seabird is about the same size as an albatross, with a wingspan of up to 180 centimeters. They also have strong neck muscles and nostrils on the inside of their beaks that can close to prevent water from entering, making them uniquely adapted to high-speed diving.

This shot was one of the most spectacular in the 2024 Underwater Photographer of the Year competition, which celebrates the wonders of the marine world.here are some new scientistThese are carefully selected works from among the many entries.

Virgo Shipwreck near Recife, Brazil

Fabi Fregonesi/UPY 2024

In this photo by Fabiana Fregonesi, a school of fish swarms around a shipwreck, forming a shape that momentarily resembles a boat's sail. The ship, called Virgo, was intentionally sunk in 2017 to serve as a diving site near Recife, Brazil.

“At that moment, I knew the ship was ready to set sail and the journey into an unknown adventure began,” Fregonesi said in a statement.

gray whale eyes

Rafael Fernandez Caballero/UPY 2024

Eye of Eastern Gray Whale (Eschrichius Robtus) penetrates this mysterious shot taken from just above the surface of a saltwater lagoon in western Mexico. These marine giants are friendly creatures and often approach boats to show curiosity. Whales undertake the longest annual migration of any mammal, from their summer feeding grounds in the Arctic south along the west coast of North America to the warm lagoons of Baja California, Mexico.

Octopus ringed with pyrosomes

Dennis Corpus/UPY 2024

In contrast to the giant gray whales, this 10 centimeter wide creature was captured up close in the deep waters off the coast of the Philippines. The circular object in the image is a pyrosome. This is a colonial animal called a zooid, which is made up of hundreds or thousands of tiny individuals. Encased in a strange pyrosome, a tiny octopus peeks out.

diving cormorant

John Anderson/UPY 2024

This ravenous cormorant mistakes photographer John Anderson's camera for a fish and heads straight for it. This stunning image was taken on a bright summer afternoon in a kelp forest at a dive site in Monterey, California. Many cormorant species rely on these special marine ecosystems to survive. However, local kelp forests have declined by 80% over the past decade.

www.newscientist.com

Surprising Images of Nearby Star-Forming Regions Captured by Hubble

astronomer using NASA/ESA Hubble Space Telescope We captured a vivid image of IRAS 16562-3959, a beautiful star-forming region in the constellation Scorpius.



This Hubble image shows IRAS 16562-3959, a star-forming region about 5,900 light-years away in the constellation Scorpius. Image credits: NASA / ESA / Hubble / R. Fedriani / J. Tan.

IRAS 16562-3959The star, also known as 2MASX J16594225-4003451, is located 5,900 light-years away in the constellation Scorpius.

“At the center of the image, IRAS 16562-3959 is thought to contain a massive star with a mass approximately 30 times that of the Sun, which is still in the process of formation,” Hubble team members said in a statement. Ta.

“At the near-infrared wavelengths that Hubble detects, the central region appears dark because there is so much dust in the way.”

“Near-infrared light, however, primarily leaks out from two sides, the top left and bottom right, where powerful jets from massive protostars are removing dust.”

“The multi-wavelength images containing this amazing Hubble scene will help us better understand how the largest and brightest stars in the Milky Way are born.”

The new image of IRAS 16562-3959 was created from separate exposures taken in the near-infrared region of the spectrum. Hubble's Wide Field Camera 3 (WFC3).

Four filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

“A filter is a thin piece of highly specialized material that only allows light at very specific wavelengths to pass through,” the astronomer explained.

“We can slide them in front of the light-sensing part of the telescope, allowing us to control which wavelengths of light the telescope collects for each observation.”

“This is useful not only for certain scientific studies, but also for creating images like this.”

“Regardless of which filter was used, raw telescopic observations are always monochrome,” they added.

“However, specially trained artists and image professionals can choose colors that match the wavelength range covered by individual filters.”

“Alternatively, if a direct match is not possible, for example the data used in this image is all in the infrared range, to which the human eye is not sensitive, so the artist has chosen colors that are wisely representative of what they are trying to represent.” You can. It’s happening.”

“For example, shorter wavelengths might be assigned a bluer color and longer wavelengths a redder color, as is the case with the visible light range.”

“The data from multiple filters can then be combined to build multicolor images that look beautiful and have scientific meaning.”

Source: www.sci.news

Stunning Images of Jupiter’s Moon Io Captured by NASA’s Juno Orbiter

On February 3, 2024, NASA's Juno spacecraft made its second close approach to Io, the fifth and third largest of Jupiter's moons. Like the previous flyby on December 30, 2023, this second pass was approximately 1,500 kilometers (930 miles) away. During the twins' flyby, the spacecraft's JunoCam instrument returned stunning high-resolution images and raw data. The flyby is designed to provide new insights into how Io's volcanic engines work and whether a global magma ocean exists beneath the volcanic moon's rocky, mountainous surface. has been done.

The JunoCam instrument aboard NASA's Juno spacecraft imaged Io, the most geologically active object in the solar system, on February 3, 2024, from a distance of approximately 7,904 km (4,911 miles) . Image credit: NASA/SwRI/MSSS.

Io is the innermost of Jupiter's four Galilean moons and the fourth largest moon in the solar system.

Its diameter is about 3,630 km (2,556 miles), making it only slightly larger than our moon.

It is the only place in the solar system other than Earth that is known to have volcanoes spewing hot lava like those on Earth.

Io has over 400 active volcanoes, which are caused by tidal heating. This is the result of a gravitational tug of war between Jupiter's gravity and the small but precisely timed gravitational pulls from Europa and Ganymede.

The moon's yellow, white, orange, and red colors are produced by sulfur dioxide, frost on its surface, elemental sulfur, and various sulfur allotropes.

The volcano was first discovered on the island of Io in 1979, and since then studies using NASA's Galileo spacecraft and ground-based telescopes have shown that eruptions and lava fountains occur constantly, forming rivers and lakes of lava. Masu.

Only 13 large eruptions were observed between 1978 and 2006, in part because fewer astronomers were scanning the moon on a regular basis.

The JunoCam instrument aboard NASA's Juno spacecraft imaged Io on December 30, 2023, from a distance of approximately 5,857 km (3,639 miles). Image credit: NASA/SwRI/MSSS.

NASA's Juno spacecraft has been monitoring Io's volcanic activity from distances ranging from about 11,000 km (6,830 miles) to more than 100,000 km (62,100 miles), providing the first view of the moon's north and south poles .

On December 30, 2023, Juno came within approximately 1,500 km of Io's surface. The orbiter made her second close flyby of the Moon on February 3, 2024.

The second flyby mainly flew over Io's southern hemisphere, but previous flybys flew over Io's northern hemisphere.

Juno captured two plumes rising above Io's horizon on February 3, 2024. These plumes were emitted from two vents from one giant volcano, or from two volcanoes located close to each other. The JunoCam instrument photographed the plume from a distance of approximately 3,800 km (2,400 miles). Image credit: NASA / JPL-Caltech / SwRI / MSSS / Andrea Luck.

“We investigate the source of Io's massive volcanic activity, whether there is a magma ocean beneath its crust, and the importance of tidal forces from Jupiter that are relentlessly squeezing this beleaguered moon. doing.”

“There are active plumes, high mountain peaks with distinct shadows, and evidence of lava lakes, some of which look like islands.”

Starting in April 2024, Juno will conduct a series of occultation experiments that will use Juno's gravity science experiments to investigate the composition of Jupiter's upper atmosphere. This provides important information about the planet's shape and internal structure.

Source: www.sci.news

Close-up of Arp 140 captured by Hubble Space Telescope

The NASA/ESA Hubble Space Telescope has captured an excellent image of the interacting spiral lens galaxy pair Arp 140.



Lenticular galaxy NGC 274 can be seen on the right side of this Hubble image, and barred spiral galaxy NGC 275 can be seen on the left side. Image credit: NASA / ESA / R. Foley, University of California, Santa Cruz / Gladys Kober, NASA and The Catholic University of America.

Alp 140 Located approximately at 70 million light years Beyond Cetus.

This galaxy duo Atlas of unique galaxiesA catalog of 338 galaxies compiled in 1966 by American astronomer Halton Earp.

It consists of NGC274 (also known as LEDA 2980) and NGC275 (LEDA 2984).

NGC 274 is classified as a lenticular galaxy, and NGC 275 is classified as a barred spiral galaxy.

“Lentiform galaxies and barred spiral galaxies have different structures,” Hubble astronomer explained.

“In a barred spiral galaxy, a bar of stars runs through the galaxy's central bulge (seen here as a bright white vertical haze in NGC 275).”

“Typically, the arms of a galaxy begin at the end of the bar.”

“Lentiform galaxies, on the other hand, fall between elliptical and spiral galaxies,” the researchers added.

“Its name comes from its edgy appearance, which resembles a saucer.”

“Lenticular galaxies have a large central bulge and a flat disk-like spiral, but no spiral arms.”

“It doesn’t have much gas or dust, and it’s mainly made up of old stars.”

Previous observations of Arp 140 revealed a tidal tail extending light-years from NGC 275 beyond the interacting pair.

They also showed that, contrary to the often assumed picture of interacting galaxies, NGC 275 does not exhibit enhanced star formation.

Source: www.sci.news

NGC 5427 captured in close-up by Hubble Space Telescope

astronomer using NASA/ESA Hubble Space Telescope They captured a striking photo of NGC 5427, which is part of the interacting galaxy pair Arp 271.



This Hubble image shows NGC 5427, a spiral galaxy located about 120 million light-years away in the constellation Virgo. Image credit: NASA / ESA / R. Foley, University of California, Santa Cruz / Gladys Kober, NASA and The Catholic University of America.

Alp 271 It was originally discovered in 1785 by German-born British astronomer William Herschel.

a pair that interacts consisting of Two spiral galaxies of similar size: NGC5426 and NGC5427.

It is located about 120 million light-years away toward the constellation Virgo, and its extent is about 130,000 light-years.

It is unclear whether the interaction experienced by NGC 5426 and NGC 5427 will end in a collision and ultimately lead to the merger of the two galaxies, or whether the galaxies will simply experience a very close encounter.

It is absolutely certain that they are already interacting with each other, as material has been stripped from galaxies to create bridges of stars and dust that connect them.

In the distant future, our Milky Way galaxy will undergo a similar collision with the Andromeda galaxy, which is currently located about 2.6 million light-years away from the Milky Way.

“NGC 5426 is below NGC 5427 and outside the frame of this image,” Hubble astronomers said.

“However, the gravitational effects of this pair can be seen in the distortion of the galaxy and the cosmic bridge of stars seen in the lower right region of the image.”

“NGC 5426 and NGC 5427 are locked in an interaction lasting tens of millions of years.”

“Whether they will eventually collide and merge is still uncertain, but their mutual attraction has already led to the birth of many new stars.”

“These young stars are visible in the faint bridge connecting the two galaxies at the bottom of the image.”

“Such bridges provide a path for the two galaxies to continue sharing gas and dust that will form new stars.”

“We believe Arp 271 serves as a blueprint for future interactions between the Milky Way and Andromeda galaxies, which are expected to occur in about 4 billion years.”

Source: www.sci.news

Physicists have successfully captured direct images of noble gas nanoclusters at room temperature

For the first time, physicists have directly imaged small clusters of noble gas atoms at room temperature. This result opens up exciting possibilities for fundamental research in condensed matter physics and applications in quantum information technology.

Xenon nanoclusters between two graphene layers. Sizes range from 2 to 10 atoms. Image credit: Manuel L'Engle.

“When I was researching the use of ion irradiation to modify the properties of graphene and other two-dimensional materials, I noticed something unusual. They can become trapped between the sheets,” the University of Vienna said. Dr. Jani Kotaski and his colleagues.

“This happens when noble gas ions pass through the first graphene layer fast enough to pass through, but not the second graphene layer.”

“Once trapped between the layers, the noble gases are free to move because they do not form chemical bonds.”

“But to accommodate the noble gas atoms, the graphene bends to form tiny pockets.”

“Here, two or more noble gas atoms can meet and form two-dimensional noble gas nanoclusters that are ordered and densely packed.”

The researchers' method overcomes the difficulty that noble gases do not form stable structures under experimental conditions at ambient temperatures.

“We observed these clusters using a scanning transmission electron microscope, and they are really fascinating and very fun to look at,” said Dr. Manuel L'Engle, a physicist at the University of Vienna.

“They rotate, jump, grow, and shrink as we imagine them.”

“Getting the atoms between the layers was the most difficult part of the job.”

“Achieving this gives us a simple system to study fundamental processes related to the growth and behavior of materials.”

“The next step is to study the properties of clusters containing different noble gases and how they behave at low and high temperatures,” Dr Kotasky added.

“With the use of noble gases in light sources and lasers, these new structures may enable future applications such as quantum information technology.”

a paper The findings were published in this week's magazine Natural materials.

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M. Langre other. Two-dimensional few atomic noble gas clusters within a graphene sandwich. nut.meter, published online on January 11, 2024. doi: 10.1038/s41563-023-01780-1

Source: www.sci.news

The Chicken Nebula’s Best Image Ever Captured by OmegaCAM

astronomer using omega cam meter is on ESO’s VLT Survey Telescope (VST) captured 1.5 billion pixel image A vast stellar nursery called the Running Chicken Nebula.



The Running Chicken Nebula is made up of several clouds, all of which can be seen in this OmegaCAM/VST image. Image credit: ESO / VPHAS+ Team / CASU.

of running chicken nebulaThe star, also known as IC 2944, is located in the constellation Centaurus, about 6,500 light-years from Earth.

ESO astronomers said in a statement: “The Running Chicken Nebula is actually made up of several regions, all of which can be seen in this vast image, spanning an area of ​​the sky roughly the size of 25 full moons. ” he said.

“The brightest region in the nebula is IC 2948There, some people see the chicken’s head, and others see the butt. ”

“The wispy pastel outlines are fantastic plumes of gas and dust.”

“IC 2944 is characterized by a bright, vertical, almost column-like structure toward the center of the image.”

“The brightest glow in this particular area is lambda centauri, a star visible to the naked eye that is much closer to us than the nebula itself. ”

But IC 2948 and IC 2944 themselves are full of young stars. And while they may be bright, they are definitely not cheerful.

“They cut through their environment in the same way as chickens, exhaling enormous amounts of radiation,” the astronomers said.

“Some regions of the nebula, known as the Bok globules, can withstand the intense assault of ultraviolet radiation that spreads through this region.”

“If you zoom in on the image, you may see small, dark, dense pockets of dust and gas scattered throughout the nebula.”

“Other areas depicted here include: gum 39 and gum 40, there is gum 41 in the bottom right. ”

“Besides the nebula, there are countless orange, white, and blue stars in the sky, like fireworks.”

“Overall, this image is a wonder that cannot be explained. It’s a feast for the eyes as you zoom in and pan around.”

“This image is a large mosaic made of hundreds of individual frames carefully stitched together.”

“Individual images were taken through filters that let different colors of light through and combined into the final result presented here.”

“The data used to create this mosaic was acquired as part of the VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+), a project aimed at better understanding the life cycle of stars. .”

Source: www.sci.news

A spectacular first photo of a snow leopard captured under the stars

Looking for ghosts requires special patience. The chances of finding it are low, but doubting means giving up, so keep looking.

This is a technique for tracking snow leopards. Morap Namgair learned that early. He was five years old when he first saw the animal in his remote village of Ulay in Ladakh, India. The area is full of wildlife and is a paradise for aspiring photographers like Molap and his younger brother Stanzin. These big cats are called locally. Shanimmortalized in the BBC series Planet Earth II They were mainly grateful to their father, Norbu, who followed them as a crew member.

Ladakh had just become famous for its sightings, but everything was shut down due to the pandemic. That’s when the brothers vowed to photograph something no one had ever photographed before: a snow leopard under the stars. They hoped the image would highlight the beauty of this mountain region and its apex predator, thereby spurring efforts to conserve both. The region is warming twice as fast as the rest of the world, threatening landscapes and wildlife. The brothers believed that if the outside world could only see what was at stake, that would influence the government’s actions.

They spent months blanketing the area with cameras. However, halfway through the project, Stanzin died of heart disease. Although it was difficult, Morap pushed forward on his own.

Last August, on a 33°C (91°F) day, he climbed a ridge at 4,900 meters above sea level. “What I found on camera was a dream come true,” Morap says. He was bittersweet though. “Buddhism believes in reincarnation. I always look at snow leopards and often think, ‘What would happen if Stan Jin was reincarnated as a snow leopard?’ Perhaps he will stop for a photo or perhaps say hello. Maybe he did.”

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Source: www.newscientist.com