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

Hubble Space Telescope Reveals Breathtaking Images of Ancient Spherical Clusters

Recent images from the NASA/ESA Hubble Space Telescope highlight NGC 1786, a spherical cluster located in the constellation of Dorado.



This Hubble image depicts NGC 1786, a spherical cluster approximately 163,000 light-years away in the Dorado constellation. The color images were created from various exposures captured in visible and near-infrared regions of the spectrum using Hubble’s Wide Field Camera 3 (WFC3). Three filters sampled different wavelengths. Colors were assigned by applying distinct hues to each monochromatic image related to individual filters. Image credits: NASA/ESA/Hubble/M. Monelli/M Hözsaraç.

Spherical clusters are ancient star systems, bound together by gravity, typically spanning around 100-200 light-years.

These clusters host hundreds of thousands, or even millions, of stars. The significant masses at the cluster’s core attract stars inward, forming a spherical configuration.

Considered among the universe’s oldest known objects, spherical clusters are remnants from the early Galactic era. It’s believed that all galaxies harbor a population of these structures.

The Large Magellanic Cloud, a neighboring dwarf galaxy located about 163,000 light-years away, possesses roughly 60 spherical clusters, including NGC 1786.

This spherical cluster, also referred to as ESO 56-39, was discovered on December 20, 1835, by the British astronomer John Herschel.

“Data from the new image is derived from spherical clusters within Milky Way galaxies, including the Large and Small Magellanic Clouds, as well as Fornax dwarf spheroidal galaxies,” stated Hubble astronomers.

“Our galaxy contains over 150 of these extensively studied ancient spherical formations.

“Due to its stability and longevity, it acts as a galactic time capsule, preserving stars from the galaxy’s formative stages.”

“While it was once believed that all stars in spherical clusters formed nearly simultaneously, our research on ancient clusters within our galaxy has revealed multiple populations of stars of varying ages,” they further explained.

“To utilize spherical clusters as historical markers, it’s essential to comprehend their formation and the origins of stars from different ages.”

“This observational program analyzed older spherical clusters like NGC 1786 in external galaxies to determine whether they contained multiple star populations.”

“Such studies can provide insights into the original formation mechanisms of the Large Magellanic Cloud as well as the Milky Way galaxy.”

Source: www.sci.news

Hubble Space Telescope Seizes Stunning Images of Dynamic Spiral Galaxies

The NASA/ESA Hubble Space Telescope captured this image of UGC 11397, the Barred Spiral Galaxy, which houses a rapidly growing, supermassive black hole.



The Hubble image depicts UGC 11397, a barred spiral galaxy, located about 250 million light years away in the constellation Lyra. Image credits: NASA/ESA/Hubble/MJ Koss/AJ Barth.

Also referred to as IRAS 19019+3346, Leda 62725, or TC 872, UGC 11397 is situated in the constellation Lyra and is approximately 250 million light years distant.

The first documented mention of this spiral galaxy appeared in a galaxy catalogue compiled by Swiss astronomer Fritz Zwicky in 1966.

“At first glance, UGC 11397 seems like a typical spiral galaxy,” stated Hubble astronomers.

“It showcases two graceful spiral arms illuminated by stars, framed by dark, dense dust clouds.”

“What sets UGC 11397 apart from a standard spiral is the ultra-massive black hole at its core, which has a mass 174 million times that of the sun,” they noted.

“As the black hole ejects gas, dust, and even entire stars from its vicinity, this material heats up, creating a spectacular cosmic display.”

“Materials engulfed by black holes emit radiation ranging from gamma rays to radio waves, leading them to brighten and dim unexpectedly.”

“Nonetheless, in some galaxies like UGC 11397, thin dust clouds obscure much of this energetic activity from optical light observation.”

“Still, the rapidly growing black hole in UGC 11397 has been identified through its intense X-ray emissions.”

This discovery led astronomers to categorize it as a Type 2 Seyfert Galaxy, a classification for active galaxies whose central cores are obscured by dust and gas formations.

“Utilizing Hubble, we will examine hundreds of galaxies that host ultra-massive black holes similar to UGC 11397,” the researchers stated.

“Hubble’s observations aid us in measuring nearby supermassive black holes, understand their growth early in the universe’s history, and explore star formation in extreme conditions at the galaxy’s center.”

Source: www.sci.news

Hubble Space Telescope Reveals New Images of NGC 4449

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured remarkable new images of the Dwarf Starburst Galaxy NGC 4449.



This Hubble image illustrates NGC 4449, a galaxy of dwarf stars located roughly 12.5 million light years away within the Canes constellation. Image credits: NASA/ESA/Hubble/E. Sabbi/D. Calzetti/A. Aloisi.

NGC 4449 is situated about 12.5 million light years away in the constellation of Canes.

Also known as Caldwell 21, Leda 40973, or UGC 7592, this galaxy is approximately 20,000 light-years in age.

NGC 4449 was first identified by German-born British astronomer William Herschel on April 27, 1788.

This galaxy is part of the M94 Galaxy group and is in close proximity to the local group that contains our Milky Way.

“NGC 4449 is a dwarf galaxy, meaning it is significantly smaller than our Milky Way and contains fewer stars,” a Hubble astronomer remarked.

“However, its small size is deceptive; NGC 4449 is prolific in star formation.”

“This galaxy is referred to as a Starburst galaxy because it produces new stars at a rate much higher than would be expected for its size.”

“While most Starburst Galaxies primarily produce stars in their centers, NGC 4449 is scattered with bright young stars throughout its structure.”

Astronomers believe this global surge in star formation has resulted from interactions between NGC 4449 and its neighboring galaxies.

“Due to its proximity, NGC 4449 offers a valuable opportunity for Hubble to investigate how intergalactic interactions influence new star formation,” they noted.

The new color image of NGC 4449 is derived from Hubble observations utilizing the Advanced Cameras for Surveys (ACS) and the Widefield Camera 3 (WFC3) across the UV, near-infrared, and optical segments of the spectrum.

Seven filters were employed to capture various wavelengths, assigning different hues to each monochrome image linked to the specific filters.

“The Hubble images of NGC 4449 were previously released in 2007,” the researchers stated.

“This updated version includes several additional wavelengths of light gathered by Hubble through multiple observational programs.”

“These programs encompass groundbreaking science, ranging from exploring the history of star formation in NGC 4449 to mapping galaxies with the brightest, hottest, and most extensive stellar structures.”

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 Space Telescope Reveals Fresh Perspective on NGC 3511

The Hubble Team has unveiled a stunning new image of the intermediate Spiral Galaxy NGC 3511.



This Hubble image depicts NGC 3511, a mid-spiral galaxy located about 43 million light years away in the crater constellations. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 3511 is situated approximately 43 million light years away from Earth, in the crater’s constellation.

Also referred to as ESO 502-13, Leda 33385, IRAS 11009-2248, or UGCA 223, this spiral galaxy spans a diameter of 107,000 light years.

NGC 3511 was discovered by the German and British astronomer William Herschel on December 21, 1786.

This galaxy is part of the NGC 3511 group, a small collection of galaxies that includes NGC 3513 and ESO 502-024.

“From Hubble’s perspective in orbit around Earth, NGC 3511 is tilted about 70 degrees, sitting in between galaxies that display edge-on features and those that exhibit dense flat discs, ideal for visualization,” Hubble astronomers stated.

Color images of NGC 3511 were created from individual exposures using UV light with the Hubble Wide Field Camera 3 (WFC3).

Six filters were employed to capture different wavelengths. Colors are assigned by applying distinct hues to each monochromatic image tied to a specific filter.

“We are examining NGC 3511 as part of our research into the star formation cycle in nearby galaxies,” stated the astronomers.

“This observational program involves Hubble recording the properties of 55 local galaxies using five filters that permit light of varying wavelengths or colors.”

“One of these filters specifically transmits red light at a particular wavelength.”

“This vast cloud of hydrogen gas glows red when stimulated by the ultraviolet rays of a hot young star.”

“As illustrated in this image, NGC 3511 is filled with numerous bright red gas clouds, some of which encircle clusters of vibrant blue stars.”

“Hubble plays a crucial role in cataloging and determining the ages of these stars, which are generally a few million years old and several times larger than the Sun.”

Source: www.sci.news

Hubble Space Telescope Observes Deformed Spiral Galaxy: NGC 1961

The Hubble team has unveiled a breathtaking new series of images showcasing the majestic Spiral Galaxy NGC 1961, featuring NASA/ESA Hubble’s cosmic insights.

This Hubble image depicts the Spiral Galaxy NGC 1961. Image credits: NASA/ESA/Hubble/J. Dalcanton/RJ Foley, UC Santa Cruz/C. Kilpatrick.

NGC 1961 is located about 190 million light-years away in the constellation Camelopardalis.

This spiral galaxy spans 240,000 light-years, making it the largest member of a small group of ten galaxies.

NGC 1961 was first discovered by German and British astronomer William Herschel on December 3, 1788.

French astronomer Guillaume Bigon observed the galaxy on December 22, 1891, and it was cataloged as IC 2133.

NGC 1961 displays a distinctive perturbation that led to its classification as ARP 184.

“The designation ARP 184 is derived from Halton Arp’s 1966 Atlas of Peculiar Galaxies,” the Hubble astronomers noted.

“The 338 galaxies listed in the Atlas often exhibit unusual shapes, lacking perfect oval or spiral forms.”

“Many of these galaxies are in interaction with others, while some show characteristics of duster galaxies without well-defined structures.”

“ARP 184 earned its spot in the catalog due to its prominent, elongated spiral arm extending towards us,” they elaborated.

“The galaxy’s far side shows clusters of gas and stars but lacks a similarly impressive spiral arm.”

The latest images of NGC 1961 include optical and near-infrared data captured by Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3).

“This Hubble image merges data from three short observation programs that fit into time gaps between other proposals,” the astronomer explained.

“One of these programs focuses on ARP 184 due to its unique structure.”

“It reviewed galaxies in the Atlas of Peculiar Galaxies, compiled by Halton Arp and Barry Madore, among others, along with catalogues of singular galaxies in the southern hemisphere.”

The remaining two programs aimed to study transient astronomical events, including supernovae and tidal disruption phenomena.

“Given that ARP 184 has hosted four known supernovae in the past 30 years, it has become a prime target for supernova research.”

Source: www.sci.news

The green comet is most likely disintegrating and cannot be seen without a telescope.

Newly discovered Green Comet is being tracked by a telescope, which suggests it may break apart as it approaches the sun. Naked Eye Spectacle.

Comet Swan from the Oort Cloud Beyond Pluton has been visible through telescopes and binoculars in recent weeks, but experts suggest it may not have survived its most recent journey. Travel past the sun and is fading rapidly.

“We’ll soon be left with a dusty cleavage pile,” stated astrophysicist Carl Battamus in an email.

A newly discovered comet swan on April 6th.Mike Orathon via the AP

Comets are frozen balls of gas and dust from billions of years ago that frequently pass through the inner solar system.

“These are artifacts from when the solar system first formed,” explained Jason Ibarra, director of the West Virginia University Planetarium and Observatory.

The latest comet was spotted by amateur astronomers who used photos from cameras on a spacecraft operated by NASA and the European Space Agency to study the sun.

Unlike Tsuchinshan-Atlas, comets do not come close to Earth. Other notable flybys include Neowise in 2020, and from the 1990s, Halebop and Hi-Aku Take.

A newly discovered comet swan with a streaming tail on April 6th. Mike Orathon via the AP

The comet, also known as C/2025 F2, would have been visible just after sunset, slightly north of the sun. Its green color may be challenging to see with the naked eye.

This was the first journey past the sun for this object, making it particularly susceptible to disintegration, according to Batam. After the flyby, the remainder of the comet vanishes into the outer reaches of the solar system, believed to be its birthplace by scientists.

“I don’t know if it’s ever coming back,” noted Batam.

Source: www.nbcnews.com

New Images of Messier 77 Captured by Hubble Space Telescope

NASA has released an incredibly beautiful image taken by the Hubble Space Telescope for the Barred Spiral Galaxy Messier 77.



This Hubble image shows the Messier 77, a Barred Spiral Galaxy, about 62 million light years away in the Cetus constellation. Color images were created from individual exposures taken with UV rays. The visible and near-infrared regions of the spectrum feature Hubble’s advanced camera (ACS) and widefield camera 3 (WFC3) equipment. Based on data obtained through six filters. Colors are attributed to assigning different hue to each monochromatic image associated with an individual filter. Image credits: NASA/ESA/Hubble/LC Ho/D. Thilker.

Messier 77 is located 62 million light years from Earth in the constellation of Cetus.

Also known as the Squid Galaxy, NGC 1068, Leda 10266, and Cetus A. This galaxy is 9.6 in size.

It was discovered in 1780 by French astronomer Pierre Messhin and originally identified it as a nebula.

Mechine then conveyed the discoveries to her colleague, the French astronomer Charles Messier.

Messier believed that the very bright objects he saw were a herd of stars, but it was realized that technology had truly achieved its position as a galaxy.

“The Messier 77 designation comes from the location of the Galaxy, a well-known catalogue edited by French astronomer Charles Messier,” the Hubble astronomer said in a statement.

“Pierre Messhin, another French astronomer, discovered the galaxy in 1780.”

“Messier and Messhin were both comet hunters cataloguing ambiguous objects that could be mistaken for comets.”

“Messier, Méchain and other astronomers of that era mistaken the Squid Galaxy for either a spiral nebula or a star cluster.”

“This false characteristic is not surprising. For over a century, we pass between discovering squid galaxies and the realization that the “spiral nebulae” scattered across the sky are not part of our galaxies, but are actually millions of light years away. ”

“The appearance from the small telescope of the squid galaxy (a very bright center surrounded by ambiguous clouds) closely resembles one or more stars in a wreath to the nebula.”

At 100,000 light years, Messier 77 is one of the largest galaxies in the Messier catalog.

This galaxy is also one of the closest galaxies with an active galactic nucleus (AGN).

Such active galaxies are one of the brightest objects in the universe, ejecting at best, if not all, wavelengths, from gamma rays and x-rays to microwaves and radiation waves.

However, despite its status as a popular target for astronomers, the Galaxy’s accretion disk is obscure by thick clouds of dust and gas.

“The name ‘Squid Galaxy’ has only happened recently,” the astronomer said.

“The name comes from an extended filament structure that curls around the galaxy’s discs like squid tentacles.”

“The squid galaxy is a great example of how advances in technology and scientific understanding can completely change the perception of astronomical objects.

Source: www.sci.news

The Hubble Space Telescope Takes Another Look at Messier 104

Looking ahead to the future NASA/ESA Hubble Space Telescope 35th Anniversary released by the Hubble team Beautiful new image The Sombrero Galaxy, also known as the Messier 104.

This Hubble image shows Messier 104, a galaxy 28 million light years away in the Virgo constellation. Image credits: NASA/ESA/Hubble/K. Noll.

Messier 104 It is about 28 million light years away from the Virgo constellations.

Also known as the Sombrero Galaxy, M104 or NGC 4594, this galaxy is I discovered it May 11, 1781, by French astronomer Pierre Mechine.

It has a diameter of approximately 49,000 light years. This is about three times the Milky Way galaxy.

The Messier 104 has a very large central bulge, hosting an ultra-high Massive black hole.

At a 6-degree angle south of the plane, you can see the Galaxy Edge-On. That dark Dustlane dominates the scenery.

Over the past 20 years, Hubble has released several images of the Messier 104. This well-known image Since October 2003.

“It’s packed with stars, but the Sombrero galaxy is surprisingly not a hotbed of star formation,” Hubble astronomers said in a statement.

“Less than one solar mass gas is converted into a star in a dusty disk with a fading knot.”

“At the 9 billion solar mass, even the central, ultra-huge black holes in a large galaxy, more than 2,000 times the central black holes in the Milky Way, are pretty calm.”

“The galaxy is not too faint to find with sincerity, but it is easily viewed with a modest amateur telescope.”

“From Earth’s perspective, galaxies are about a third of the diameter of a full moon.”

“The galaxy in the sky is too large to fit in Hubble’s narrow field of view, so this image is actually a mosaic of several images sewn together.”

“One of the things that make this galaxy particularly noteworthy is its viewing angle, tilting just six degrees away from the galaxy’s equator.”

“From this perspective, the complex clumps and shattering chains stand out in the nucleus and bulge of the bright white galaxy, unlike Saturn and its rings, produce an effect on the scale of the epic galaxy.”

“At the same time, this extreme angle makes it difficult to identify the structure of the Sombrero galaxy,” they said.

“It’s not clear if it’s a spiral galaxy like our own Milky Way or an elliptical galaxy.”

“Unbelievably, galaxy disks look like fairly typical discs of spiral galaxies. The spheroid bulge and halos look quite typical in oval galaxies, but the combination of the two components is neither a spiral nor an elliptical galaxy.”

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.

____

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

The Hubble Space Telescope Observes NGC 3274

Astronomers using the NASA/ESA Hubble Space Telescope took an incredible new photo of the Spiral Galaxy NGC 4941.

This Hubble image shows NGC 4941, a spiral galaxy in Virgo’s constellation, about 67 million light years away. The color image consists of near-infrared, optical and ultraviolet observations from Hubble’s Wide Field Camera 3 (WFC3). Six filters were used to sample different wavelengths. Colors are attributed to assigning different hue to each monochromatic image associated with an individual filter. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 4941 It is approximately 67 million light years away from Earth, the Virgo constellation.

Also known as AGC 530009, IRAS 13016-0516, Leda 45165, or UGCA 321. 60,000 light years Crossing.

It was discovered on April 24, 1784 by German and British astronomer William Herschel.

NGC 4941 is a member of two galaxy groups, the NGC 4941 group and the NGC 4697 group.

“Because this galaxy is nearby, in cosmic terms, Hubble’s sharp instruments can choose exquisite details such as individual star clusters and filament clouds of gas and dust,” said the Hubble astronomer.

“The Hubble data used to construct this image was collected as part of an observation program that investigates star formation and stellar feedback cycles in nearby galaxies.”

“When stars form in densely cold gas clusters, they start to affect their surroundings.”

“The stars heat and stir the gas clouds created by exploding as supernoves for the wind, starlight, and ultimately the large stars.”

“These processes collectively are called stellar feedback and affect the rate at which galaxies can form new stars.”

“After all, stars aren’t the only entities that provide feedback in NGC 4941,” they added.

“It’s in the heart of this galaxy Active galactic nuclei (AGN) – Look at Gas.

“When a black hole accumulates gas from the surroundings, it swirls into an overheated disk that glows brightly at wavelengths throughout the electromagnetic spectrum.”

“It resembles a star, but on a much larger scale – the active galactic nucleus shapes its surroundings through wind, radiation and powerful jets, changing not only the formation of stars but also the evolution of the entire galaxy.”

Source: www.sci.news

Discovering Aurora on Neptune for the First Time with NASA’s Webb Telescope

The Northern and Southern Lights Vermillion, Amethyst, and Jade Ribbons are some of the most distinctive features of the Earth. However, our planet has no monopoly of the Aurora. Scientists spy on them throughout the solar system, weaving the Martian sky into Saturn, Jupiter and even some of Jupiter’s fiery softening.

The light shines in the sky Uranus too. However, the aurora around Neptune, the farthest planet of our Sun, has long escaped astronomers.

That was changed by the powerful infrared equipment installed in the James Webb Space Telescope. In a study published in the journal on Wednesday Natural Astronomy scientists reveal unique auroras spilling on either side of Neptune’s equator. This contrasts with the sparkling Gossamers, arcing at Poles in other worlds.

Astronomers are excited that the Aurora Hunting Quest has been completed over decades. “Everyone is very excited to prove it’s there, as we thought,” he said. Rosie Johnson an astrophysics researcher at Aberystwyth University in Wales who was not involved in new research.

The discovery allows scientists to study previously out-of-reach aspects of Neptune. “They use the aurora to understand the shape of the magnetic field on planets looking at the invisible,” he said. Karl Schmidt Boston University planetary astronomers were not involved in new research.

Each world produces aurora differently, but it is basically the same. Energy particles (often from the sun, but sometimes from the eruption of a lunar volcano) hit the atmosphere and bounce back the gas. The collision of the particles causes a temporary flash of light. And if there is a magnetic field in the world, it will guide the position…

Luckily, the Webb Telescope, released in 2021, came to rescue.

Heidi Hammel Another astronomer of the University Association for Astronomical Studies and the author of the research, has been studying Neptune since the 1980s. She said that if Webb “is powerful enough to see the early galaxies of the universe, it would be strong enough to see something like Neptune’s Aurorae.” “And by Golly, that was the case.”

Using the telescope’s near-infrared spectrometer, astronomers captured Neptune’s infrared aurora in June 2023. This is because Neptune has an unstable magnetic field tilted to 47 degrees from the planet’s spin axis.

New Webb observations also reveal why Neptune’s Auroras has never been visible until now. Almost 40 years ago, Voyager 2 recorded a temperature of about 900 degrees Fahrenheit in the Neptune’s upper atmosphere. However, the Webb telescope shows that the temperature has dropped nearly 200 degrees. This low temperature means that the aurora is a dimmer.

In fact, Neptune’s Aurora said, “It’s less than 1% of the expected brightness and explains why I’ve never seen it before.” James O’Donohew a planetary astronomer at the UK’s Reading University and one of the authors of the study. “But that means we have a new mystery in our hands now. How did Neptune get so cold?”

Neptune’s Strange Light Show detection may bring your answers closer.

“The Aurora is like a TV screen,” he said. Lee Fletcher a planetary scientist at the University of Leicester in the UK and one of the authors of the study. They said, “We are able to see the delicate dance of the magnetosphere processes.

Source: www.nytimes.com

First Data Drop from Euclidean Space Telescope Reveals 26 Million Galaxies

Galactic sea photographed by the Euclidean Space Telescope

ESA/Euclid/Euclid Consortium/NASA, J.-C. Image processing by Cuillandre, E. Bertin, G. Anselmi

The extraordinary image from the Euclidean Space Telescope has acquired 26 million galaxies.

Euclid was launched by the European Space Agency (ESA) in July 2023, and in November of that year it sent its first image back. The six-year mission will image about a third of the sky and build the most detailed 3D map of Cosmos ever created. Once completed, this investigation will help to lighten how dark matter and dark energy behave on a cosmic scale.

ESA is currently being released The first large data on this missionstarts with three “deep fields.” This is an area where the telescope becomes a more detailed peer than the rest of the study area. These three spots represent 63 squares of sky, which corresponds to an area where the full moon is covered 300 times. Over the next few years, Euclide will pass these regions 30-52 times to build more detailed images.

It'll be Percival The University of Waterloo in Canada says that current batches of images are less than 50% of what gather on missions, but there is already plenty of researchers to collaborate. “There's so much you can do about many individual galaxies and their properties because it's not something that's done in space-based research with nearby infrared light or optics like this,” he says. “It's not exactly the same quality as HST [the Hubble Space Telescope]but it's so close that it doesn't just point to individual objects and shoot. We are conducting an investigation. ”

Researchers have already used Euclidean data to find hundreds of powerful gravity lenses. These phenomena are formed when the gravity of an object in the foreground distorts light from a distant galaxy, creating an arc shape or a complete ring. Previously, scientists had to hunt these individually, point them to the HST, and collect more images. Currently, astronomers can search for survey data from Euclidean and find more at once. This helps to gather insights into the evolution of galaxies and the universe.

Using AI models, researchers were able to find and catalog 500 galaxies with powerful gravity lenses with this first data alone, doubling the total seen to date. “The statistics are incredible,” Percival says. “Euclidean ultimately gets this amount of data 200 times.”

The data released so far represents only one week of images from Euclidean, but up to 35 terabytes. This is equivalent to 200 days of high quality video streaming. The next batch of data is expected to be released later next year, and will be a year's worth of images covering 2,000 square degrees and over 2,000 terabytes of storage space.

It can take over 100 years to view each galaxy manually, so AI is used to dramatically speed up the process, he says. Mike Walmsley At the University of Toronto. “We can ask new questions in weeks, not years, but in weeks,” he says.

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Source: www.newscientist.com

NGC 4900: Surveillance with the Hubble Space Telescope

Astronomers using the NASA/ESA Hubble Space Telescope have produced the epic image of the Spiral Galaxy NGC 4900.

This Hubble image shows the NGC 4900, a spiral galaxy about 45 million light years away in the Virgo constellations. Image credits: NASA/ESA/Hubble/SJ Smartt/C. Kilpatrick.

NGC 4900 It is about 45 million light years away from the Virgo constellations.

Also known as the Leda 44797 or IRAS 12580+0246, this Spiral Galaxy has 66,000 light years.

The NGC 4900 was discovered by German and British astronomer William Herschel on April 30, 1786.

Galaxy is a member of the NGC 4753 group and a member of the Virgo II group.

New images of the NGC 4900 were created from individual exposures taken in the visible and near-infrared regions of both spectra. Hubble Advanced Camera for Survey (ACS) and Widefield Planet Camera 2 (WFPC2).

“The data are more than 20 years apart in two different observational programs. This is a true testament to Hubble's long scientific life,” said the Hubble astronomer.

“Both programs aimed to understand the end of a giant star.”

“For one, researchers were aiming to study the locations of past supernovaes, estimate the masses of the exploded stars, and investigate how the supernova interacts with their surroundings.”

“NGC 4900 was selected for research because it hosted a named supernova SN 1999BR. ”

“In other programs, researchers have laid the foundation for studying future supernovaes by collecting images of more than 150 nearby galaxies.”

“After a supernova is detected in any of these galaxies, researchers can look up these images and search for stars at the supernova location.”

“Identifying supernova progenitor stars in pre-explosion images gives valuable information about how, when, and why supernovae occur.”

Source: www.sci.news

NGC 5042 Under Observation by Hubble Space Telescope

Astronomers using the NASA/ESA Hubble Space Telescope have created a beautiful new image of the Intermediate Spiral Galaxy NGC 5042.



This Hubble image shows NGC 5042, a mid-spiral galaxy, about 48 million light years away in the Hydra constellations. Image credits: NASA/ESA/Hubble/D. Thilker.

NGC 5042 It is located approximately 48 million light years from Earth, the Hydra constellation.

The galaxy has a diameter of 80,000 light years, known as ESO 508-31, LEDA 46126 or IRAS 13127-2343.

That's what NGC 5042 was I discovered it by British astronomer John Herschel on March 25, 1836.

“The NGC 5042 fills this frame of Hubble image nicely, and there is a single milky star marked with cross-shaped diffraction spikes that attempt to blend in with bright stars along the edge of the galaxy,” the Hubble astronomer said in a statement.

The NGC 5042 is packed with ancient stars, and the galaxy's spiral arms are decorated with patches of young blue stars.

“The elongated yellow orange objects scattered around the image are background galaxies that are far more distant than NGC 5042,” the astronomer said.

“Perhaps the most impressive feature of the NGC 5042 is its collection of vibrant pink gas clouds scattered throughout the spiral arm.”

“These flashy clouds are called the H II region and get a unique color from hydrogen atoms ionized by ultraviolet rays.”

“If you look closely at this image, it appears that many of these reddish clouds are associated with a mass of blue stars, often appearing to form shells around the stars.”

“The H II region is generated by vast clouds of hydrogen gas, producing sufficient high energy light to create the HI II region, and only hot, large stars are produced.”

“The stars that can create the H II region only live for millions of years, and therefore the eye blinks from the galaxy's perspective, so this image represents a fleeting snapshot of the life of this galaxy.”

New images of NGC 5042 are Hubble Wide Field Camera 3 (WFC3) UV, near-infrared, and spectral optical parts.

Six filters were used to sample different wavelengths. Colors are attributed to assigning different hue to each monochromatic image associated with an individual filter.

“Hubble observed NGC 5042 in six wavelength bands ranging from ultraviolet to infrared and created this multicolored portrait,” the researchers said.

Source: www.sci.news

NASA to launch Spherex Space Telescope for Sky Scanning Mission

Impressions of the artists of Spherex Space Telescope

NASA/JPL-Caltech

The latest addition to NASA's Space Telescope Fleet will be launched this weekend and will soon scan the entire sky in near-infrared wavelength ranges, collecting a wealth of data on more than 450 million galaxies.

The history of the universe, the reionization epoch, and the spectrophotometer for Ice Explorer (Spherex) will be released on March 2nd on a SpaceX Falcon 9 rocket from the Vandenberg Space Force Base in California at 10:09 pm local time.

It carries a camera with filters that divide the light that enters like a prism and beams different parts of the spectrum into 102 separate color sensors. As the telescope pans around the sky, it slowly tightens the full image pixels pixel by pixel. This strategy allows you to use a relatively small and simple camera to do what you need to have a heavy, expensive suite of sensors, even without moving parts.

“If you slowly scan the sky slowly by moving the telescope, after a sufficient amount of time, every pixel in the sky is observed over a very wide wavelength range, giving you a coarse spectrum of every bit of the sky that has never been done before.” Richard Ellis University College London. “It's a very small space telescope, but it has some very unique features.”

Ellis says this rich dataset allows for accidental discoveries. “There's a high chance that you'll find something unexpected,” he says.

Infrared data is outside the human vision range, allowing scientists to determine the distance of objects and learn how to form galaxies. It can also be used to determine the chemical composition of an object, potentially revealing the presence of water and other important components.

The interesting stuff thrown by Spherex can be investigated in a more focused way using NASA's existing space telescope fleet.

Christopher Conseris At the University of Manchester in the UK, Spherex says it doesn't match the JWST solution or create similarly adoring images, but it says it will become a “maintainer” for scientific discovery.

“JWST can point to a part of the sky and take some big photos [and reveal] Something completely new. And Spherex really can't do the same thing,” he says. “It's going to be an analysis that takes years, and it's going to cover the sky many times.”

Spherex orbits the Earth 14.5 times a day away from the Earth's surface, completing 11,000 orbits over a two-year lifespan. Three cone-shaped shields protect the instrument from the Earth's radiant heat and interference from the sun.

The same rocket will be released on the polarimeter, another NASA mission to unify the Corona and Heliosphere Fair (punch), which will study the solar winds of the sun.

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Source: www.newscientist.com

Exploring the Colorful Veil Nebula with the Hubble Space Telescope

The NASA/ESA Hubble Space Telescope produced excellent images of a small portion of the Veil Nebula, part of the remnants of a supernova called the Cygnus loop.

This Hubble image shows part of the Veil Nebula. Image credits: NASA/ESA/Hubble/R. Sankrit.

Cygnus loop It is a large donut-shaped nebula located approximately 2,400 light years from Earth.

Also known as the W78 and Sharpless 103, it is actually an explosive blast from a supernova explosion that occurred 10,000 to 20,000 years ago.

Its name comes from the position of the northern constellations of Cygnus and covers an area 36 times the full moon.

The visual part of the supernova remains is known as the veil nebula, also known as the caterpillar or filamentous nebula.

“This nebula is about 20 times more star remnants than the sun that exploded 10,000 to 20,000 years ago,” said Hubble astronomers.

This new image consists of observations from Hubble Wide Field Camera 3 (WFC3) Optical part of the spectrum.

“This view combines images taken with three different filters to highlight the release from hydrogen, sulfur and oxygen atoms,” the astronomer said.

“The image shows just a small part of the Veil Nebula. If we could see the entire nebula without the help of a telescope, it would be as wide as six full moons were placed side by side.”

“The image captures the Veil Nebula at just one point, but it helps researchers understand how the remnants of the supernova have evolved over the decades.”

“Combining this snapshot with Hubble observations from 1994 reveals the movement of individual knots and gas filaments over that time, improving our understanding of this stunning nebula.”

Source: www.sci.news

Space Flower Spotted by Gemini Telescope in Large Magellan Cloud

Using Gemini South Telescope, NSF's Noirlab astronomers imaged a beautiful nebula around the young open cluster NGC 2040.

The nebula, including the NGC 2040, resembles the vivid roses in this image taken by a Gemini Southeres scope. Image credits: International Gemini Observatory / Neur Love / NSF / Aura / J. Miller & M. Rodriguez, International Gemini Observatory & NSF No Arab/TA Rector, University of Alaska Anchorage & NSF No Arab/NSF No Arab/NSF No Arab, NSF No Arab.

NGC 2040 It is about 160,000 light years away from Earth, the constellation of Dorado.

This cluster, also known as the Cal 60 or ESO 56-164, resides within the large Magellan cloud, a satellite d-star galaxy of the Milky Way.

NGC 2040 is a so-called OB association, usually a stellar group containing stars between 10 and 100 stars O and B.

“O- and B-spectral types of stars live a short life of just millions of years, burning very hot before they explode like supernovae during that time,” Noirlab astronomers said in a statement.

“The energy released by these massive star explosions will be fed into the formation of NGC structures in the 2040s, while the material emitted sowing the growth of the next generation of stars.”

Most of our galaxy stars are thought to have been born in the OB Association, as well as NGC 2040.

“NGC 2040 is part of a large structure of interstellar gas known as LH 88, one of the largest active star-forming regions within the large Magellan cloud,” the astronomer said. Ta.

“Thousands of new stars will be born in the region over the millions of years to come.”

“When stars O and B end their supernovae life, they enrich the clusters with elements like carbon, oxygen and iron,” they said.

“Along with the rich hydrogen in the cluster, these elements provide the components necessary for the formation of new stars, planets, and perhaps life.”

“The bright stars seen in the image are widely separated, but their movements through space are similar, indicating that they have a common origin.”

“The layered ambiguous structure of LH 88 is the remains of an already dead star.”

“The delicate leaves of the rose were formed by both the shock waves of the supernova and the stellar winds of the stars of O and B.”

Source: www.sci.news

The Hubble Telescope Reveals a Galaxy Hosting a Supernova

The NASA/ESA Hubble Space Telescope has captured an impressive photo of a well-known galaxy called Wisea J070815.11+210422.3.



SN 2022AJN looks like a blue point in the center of this Hubble image, brightening the Wisea J070815.11+210422.3 blurred body. Image credit: NASA / ESA / Hubble / RJ Foley, UC Santa Cruz.

Wisea J070815.11+210422.3 is situated approximately 600 million light years away in the Gemini constellation.

This image was captured about two months following the supernova event in the galaxy, known as SN 2022AJN.

“Up until the announcement made in November 2022, SN 2022AJN had not been the focus of published research,” stated Hubble astronomers.

“Hubble observed this supernova for a reason. SN 2022AJN is classified as a Type IA supernova, resulting from the explosive death of a star’s core.”

Type IA Supernovae are valuable to astronomers for determining distances to distant galaxies.

“This is feasible because Type IA supernovae exhibit consistent brightness, emitting the same amount of light regardless of their distance from Earth,” they explained.

“Thus, by comparing observed brightness to expected brightness, the distance to the supernova and its host galaxy can be calculated.”

“Despite its apparent simplicity, this measurement method is complicated by intergalactic dust.”

“A supernova appearing red when it should be blue can be due to dust between galaxies affecting its appearance.”

“To address this complication, Hubble is being employed to study a total of 100 Type IA supernovae across seven wavelength bands, ranging from ultraviolet to near-infrared.”

The color image of Wisea J070815.11+210422.3 was produced from various exposures collected in the infrared part of the spectrum using Hubble Wide Field Camera 3 (WFC3).

Four filters were utilized to sample different infrared wavelengths, with each filter assigned a different hue to represent a single color image.

“This image blends data from four infrared wavelengths,” explained scientists.

“Infrared light passes through dust more effectively than visible or ultraviolet light.”

“By comparing supernova brightness across different wavelengths, researchers can mitigate the impact of dust and distance, enhancing measurements of distant galaxies and the universe’s expansion.”

Source: www.sci.news

Hubble Space Telescope takes a second look at NGC 5643

The Hubble team has released a striking new image of the center of NGC 5643, a spectacularly designed spiral galaxy in the constellation Lupus.



This Hubble image shows NGC 5643, the Grand Design Spiral in the constellation Lupus, about 55 million light-years away. Image credits: NASA / ESA / Hubble / A. Riess / D. Thilker / D. De Martin, ESA & Hubble / M. Zamani, ESA & Hubble.

NGC5643 It is located approximately 55 million light years away in the constellation Lupus.

The planet, also known as ESO 272-16 and LEDA 51969, was discovered by James Dunlop on May 10, 1826.

NGC 5643 is classified as a Grand Design Spiral due to its prominent and graceful spiral arm.

It is approximately 100,000 light-years in diameter and contains an active galactic nucleus of type Seyfert 2.

“NGC 5643 is what is known as a Grand Design Spiral, which refers to how the galaxy's two large, sinuous spiral arms are clearly visible,” Hubble astronomers said in a statement.

“The spiral arms are defined by bright blue stars, lacy reddish-brown dust clouds, and pink star-forming regions.”

“As fascinating as the galaxy is at visible wavelengths, some of NGC 5643's most interesting features are invisible to the human eye.”

New images of NGC 5643 consist of observations from. Hubble's Wide Field Camera 3 Found in the ultraviolet, infrared, and optical portions of the spectrum.

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

“The ultraviolet images, X-ray images, and spectra of NGC 5643 show that this galaxy has an active galactic nucleus, a particularly bright galactic nucleus driven by a feast of supermassive black holes,” the astronomers said. said.

“When a supermassive black hole takes in gas from its surroundings, it collects in a disk and heats it up to hundreds of thousands of degrees.”

“Superheated gases glow brightly across the electromagnetic spectrum, but especially at X-ray wavelengths.”

“However, NGC 5643's active galactic nucleus is not the brightest X-ray source in the galaxy,” the researchers added.

“Researchers using ESA's XMM Newton discovered an even brighter X-ray emitting object called NGC 5643 X-1 on the outskirts of the galaxy.”

“What source of X-rays is more powerful than a supermassive black hole? Surprisingly, the answer appears to be a much smaller black hole.”

“The exact identity of NGC 5643 X-1 is not yet known, but evidence points to it being a black hole with about 30 times the mass of the Sun.”

“A black hole trapped in an orbital dance with a companion star captures gas from the companion star, creating a superheated disk above the center of the galaxy.”

Hubble astronomers previously released images of NGC 5643 in 2020.

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

Hubble Space Telescope Spots Spiral of Condensation in NGC 2090

Astronomers using the NASA/ESA Hubble Space Telescope have taken surprising new photos of spiral galaxy NGC 2090.

This Hubble image shows NGC 2090, a spiral galaxy located south of the constellation Columba, about 40 million light-years away. Color images were created from separate exposures taken in the ultraviolet, visible, and near-infrared regions of the spectrum using Hubble's Wide Field Camera 3 (WFC3). This is based on data obtained through six filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / D. Tilker.

NGC2090 It is a spiral galaxy located south of the constellation Columba.

Also known as ESO 363-23, IRAS 05452-3416, LEDA 17819. discovered It was announced by Scottish astronomer James Dunlop on October 29, 1826.

“NGC 2090 is notable as part of a group of galaxies being studied. Hubble's Extragalactic Distance Scale Key Project“This study aimed to determine a new, state-of-the-art value for the Hubble constant, one of the main scientific goals of the then-new telescope,” Hubble astronomers said in a statement.

“NGC 2090's contribution was to calibrate the Tully-Fisher (TF) distance method by observing Cepheid variable stars in the galaxy.”

“Cepheid-based measurements from a 1998 study estimated the distance of NGC 2090 to be 37 million light-years.”

“Latest measurements in 2020 using the TF method place NGC 2090 slightly further away, at 40 million light-years.”

Before and after that project, NGC 2090 has been well studied as a very prominent nearby example of star formation.

It has been described as a cotton-like spiral, meaning a spiral galaxy with a speckled, dusty disk and flaky or no visible arms.

“This Hubble image gives a good indication of why NGC 2090 received such a description, with its spiral arms looking like lanes of light winding through the dust,” the astronomers said. said.

“NGC 2090 remains an active galaxy, with clusters of star formation in various stages of evolution spread throughout the disk.”

“Investigating star formation and the movement of matter within galaxies was the motivation for these Hubble observations taken in October of this year.”

“Likewise, Hubble's partner in space astronomy, NASA/ESA/CSA's James Webb Space Telescope, also scouted this galaxy to add infrared data to the picture of galaxy evolution.”

Source: www.sci.news

Reports show that an unprecedented failure led to the collapse of a world-famous radio telescope in Puerto Rico.

Four years after the radio telescope at Puerto Rico’s Arecibo Observatory collapsed. Report from the National Academies of Sciences, Engineering, and Medicine sheds light on the unprecedented failures that led to its destruction.

A steel cable supporting the telescope’s 900-ton receiver platform came loose after a zinc-filled socket built to support it failed, according to a report released Oct. 25. That’s what it means.

The report said the failure was caused by excessive “zinc creep,” a phenomenon in which the metal used to protect the socket from corrosion and rust deforms over time and loses its grip.

The zinc gradually lost its hold on the cable suspending the telescope’s main platform above the reflector dish. This caused multiple cables to be pulled from their sockets, ultimately causing the platform to crash into a reflector more than 400 feet below, according to the report.

Roger L. McCarthy, chairman of the committee for the analysis of the causes of failure and collapse of Arecibo’s 305-meter telescope, said, “This type of failure has been the most common occurrence in more than a century, when zinc spelter sockets have been widely and successfully used. This has never been reported before.” The observatory wrote in its report:

The committee that prepared the report said there was insufficient data to definitively prove the exact cause of the acceleration of “zinc creep.” The only hypothesis the committee was able to develop based on the data was that low current electroplastic effects were responsible. In other words, the constant current flowing through the socket could have strengthened the plastic behavior of the metallic zinc and, as a result, weakened its grip.

The committee reviewed an array of documents commissioned by the University of Central Florida and the National Science Foundation, the federal agency that owns the observatory, including a forensic investigation, structural analysis, engineering plans, inspection reports, photographs, and repair proposals. Reach that conclusion. They also gathered information from Arecibo Observatory employees, other “related research” sources, and the National Academies of Sciences, Engineering, and Medicine. I mentioned this in a media advisory last month..

The commission also issued a series of recommendations in its report. These include making the remaining sockets and cable sections of the radio telescope available for further research and increasing careful monitoring of aging research facilities to detect deterioration and potential new failure modes. Included.

The telescope was used to track asteroids as they headed toward Earth, conduct research that led to Nobel Prizes, and determine whether planets were potentially habitable. It also functions as a training venue for graduate students, and is visited by approximately 90,000 people annually.

The telescope was built in the 1960s with funding from the Department of Defense during the development of ballistic missile defense. In its 57 years of operation, it has withstood hurricanes, tropical humidity, and a recent series of earthquakes.

The observatory began to collapse in August 2020 when an auxiliary cable snapped, damaging the telescope’s antenna and the receiver platform suspended above it, according to the National Science Foundation. After several other cable failures, the federal agency decided to begin a plan to decommission the telescope in November 2020.

This transition did little to stop the telescope’s complete collapse on December 1, 2020.

In 2022, the National Science Foundation says: Puerto Rico’s famous radio telescope won’t be rebuilt. Instead, it called for a $5 million education center to be established in its place to promote programs and partnerships related to science, technology, engineering and mathematics.

Source: www.nbcnews.com

Stunning Galaxy Duo Captured by NASA Telescope

NASA has released a beautiful composite image of two overlapping spiral galaxy pairs, IC 2163 and NGC 2207, taken by the NASA/ESA Hubble Space Telescope and the NASA/ESA/CSA James Webb Space Telescope.

This composite image shows the galaxies IC 2163 (left) and NGC 2207 (right). Image credit: NASA/ESA/CSA/STScI.

of IC 2163-NGC 2207 pair It is located about 114 million light years from us in the direction of the constellation Canis Major.

The large and massive galaxy is registered as NGC 2207, and the smaller galaxy is registered as IC 2163.

Strong tidal forces from the former distorted the shape of the latter, blowing stars and gas into long streams stretching 100,000 light years.

IC 2163 made its closest approach 40 million years ago, passing NGC 2207 in a counterclockwise direction.

However, IC 2163 does not have enough energy to escape NGC 2207's gravity and is doomed to be pulled back again in the future, passing by the larger galaxy.

“The pair's eerie colors represent a combination of mid-infrared light from the web and visible and ultraviolet light from Hubble,” NASA astronomers said.

“Look for potential evidence of their light scrapes on impact surfaces where material from galaxies may have collided.”

“These lines, rendered in bright red, including the eyelids, may be responsible for the appearance of the galaxy's bulging, vein-like arms.”

“The galaxy's first passage may also have distorted its delicately curved arms and elicited tidal extensions in some places.”

“The small diffused spiral arm between IC 2163's core and its leftmost arm may be an example of this activity.”

“More tendrils appear to be hanging between the galactic cores.”

“Another extension drifts off the top of the larger galaxy, forming a thin translucent arm that essentially extends out of the picture.”

These images show two overlapping spiral galaxies, IC 2163 and NGC 2207. On the left is Hubble's ultraviolet and visible light observations, and on the right is Webb's mid-infrared observations. Image credit: NASA/ESA/CSA/STScI.

IC 2163 and NGC 2207 form stars at such high rates that they appear to have millions of individual hearts flapping across their arms.

These galaxies produce the equivalent of 20 solar-mass stars of new solar-mass stars every year.

“Our Milky Way galaxy only forms two to three new Sun-like stars a year,” the astronomers said.

“Both galaxies have experienced seven known supernovae in recent decades, compared to the Milky Way's average of once every 50 years.”

“Each supernova may have removed space within the arms, rearranging gas and dust that later cooled, allowing many new stars to form.”

“To identify sequences of star-forming activity, look for the bright blue regions seen by Hubble in ultraviolet light and the pink and white regions detailed primarily by Webb's mid-infrared data.” the researchers said.

“Stars in larger regions are known as superclusters.”

“Look for examples of these in the top spiral arms that wrap around larger galaxies and point to the left.”

“Other bright regions of the galaxy are ministarbursts, where many stars form in quick succession.”

“In addition, the upper and lower 'eyelids' of IC 2163, the small galaxy on the left, are filled with newer star formation and are burning brighter.”

Source: www.sci.news

New X-ray Telescope NICER Makes Exciting Discovery of Fast-Spinning Neutron Star

The neutron star in X-ray binary system 4U 1820-30 rotates 716 times per second, the fastest rate ever observed, according to an analysis of data collected by NASA’s Neutron Star Internal Composition Explorer (NICER). It is one of the rotating celestial bodies. 2017 and 2022.

Artist’s depiction of the X-ray binary star system 4U 1820-30 at the center of globular cluster NGC 6624. Image credit: NASA.

4U 1820-30 It is located approximately 26,000 light years from Earth in the constellation Sagittarius.

This X-ray binary star system is part of a metal-rich globular cluster called NGC6624.

It consists of two stars: a neutron star and a white dwarf companion. The latter orbits a neutron star every 11 minutes, making it the star system with the shortest known orbital period.

The 4U 1820-30 typically displays short bursts of X-rays that last only 10 to 15 seconds. This is likely due to the ignited helium-rich fuel burning out quickly on the surface.

“Due to its strong gravity, the neutron star pulls matter away from its companion star,” said Dr. Gaurava Jaisawal of DTU Space and colleagues.

“When enough material accumulates on the surface, a violent thermonuclear explosion occurs on the neutron star, similar to an atomic bomb.”

Astronomers observed 4U 1820-30 using NASA’s NICER X-ray telescope mounted outside the International Space Station.

“While studying thermonuclear explosions from this system, we discovered significant oscillations, caused by the neutron star rotating around its central axis at an astonishing speed of 716 times per second. “This suggests that the

“If future observations confirm this, the 4U 1820-30 neutron star would be one of the fastest rotating objects ever observed in the universe, rivaled by a star called PSR J1748-2446. There will only be another neutron star.”

From 2017 to 2021, NICER detected 15 thermonuclear X-ray bursts from 4U 1820-30.

This was one of the bursts that exhibited symptoms known as “thermonuclear burst oscillations,” which occur at a frequency of 716 Hz.

These bursts of oscillations match the rotational frequency of the neutron star itself, meaning it is rotating around its axis at a record speed of 716 times per second.

“During the burst, the neutron star becomes up to 100,000 times brighter than the Sun and releases an enormous amount of energy,” said DTU space researcher Dr. Jerome Cheneves.

“We are therefore working on very extreme events, and studying them will provide new insights into the existing life cycles of binary star systems and the formation of elements in the universe.”

of findings will appear in astrophysical journal.

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Gaurava K. Jaisawal others. 2024. A comprehensive study of the 4U 1820-30 thermonuclear X-ray burst by NICER: accretion disk interactions and candidate burst oscillations. APJ 975, 67; doi: 10.3847/1538-4357/ad794e

Source: www.sci.news

Allen Telescope Array seeks radio signatures of technology from TRAPPIST-1 system

The TRAPPIST-1 system is a compact system of at least seven exoplanets that are similar in size to Earth. Astronomers from Pennsylvania State University and the SETI Institute spent 28 hours scanning the system for signs of alien radio technology using the Allen Telescope Array. This project marks the longest single-target search for radio signals from TRAPPIST-1. Although astronomers found no evidence of extraterrestrial technology, their work introduced new ways to search for wireless techno-signatures in the future.

This artist's impression shows a surface view of one of the exoplanets in the TRAPPIST-1 planetary system. Image credit: ESO / M. Kornmesser / Spaceengine.org.

TRAPPIST-1 is an ultracool dwarf star located 38.8 light-years away in the constellation Aquarius.

This star is barely larger than Jupiter and has only 8% the mass of the Sun. It rotates rapidly and produces an energetic flare of ultraviolet light.

TRAPPIST-1 is the home planet of seven transit planets named TRAPPIST-1b, c, d, e, f, g, and h.

All of these planets are the same size or slightly smaller than Earth and Venus, and have very short orbital periods of 1.51, 2.42, 4.04, 6.06, 9.21, 12.35, and 20 days, respectively.

Presumably they are all tidally locked, meaning that the same side of the planet always faces the star, just as the same side of the moon always points towards the Earth. This creates a persistent night side and a persistent day side for each planet in TRAPPIST-1.

Three of the planets, TRAPPIST-1e, f, and g, are located in the star's habitable zone, meaning they may have an environment suitable for life.

“The TRAPPIST-1 system is relatively close to Earth and has detailed information about the planet's orbit, making it an excellent natural laboratory for testing these technologies,” said Penn State graduate student Nick Tasei said.

“The methods and algorithms we developed for this project could eventually be applied to other star systems, increasing the likelihood of finding regular communications between planets beyond our solar system (if they exist). ).

Tusay and his colleagues focused on a phenomenon called interplanetary occultations.

These occultations occur when one planet moves in front of another. If intelligent life exists in that star system, it is possible that radio signals sent between the planets could leak and be detected from Earth.

Astronomers used the upgraded Allen Telescope Array to scan a wide range of frequencies, looking for narrowband signals that could be a possible sign of alien technology.

They filtered through millions of potential signals and narrowed it down to about 11,000 candidates for further analysis.

They detected 2,264 of these signals during the predicted interplanetary occultation period. However, none of the signals were of non-human origin.

New features of the Allen Telescope Array include advanced software to filter signals, helping researchers separate possible alien signals from those on Earth.

They believe that improving these techniques and focusing on phenomena such as interplanetary occultations could increase the chances of detecting alien signals in the future.

Although scientists did not find any alien signals this time, they plan to continue refining their search techniques and exploring other star systems.

Future explorations using larger and more powerful telescopes could help scientists detect even fainter signals and expand our understanding of the universe.

“This study shows that we are getting closer to detecting radio signals similar to those we send into space,” Tusey said.

“Most searches assume some kind of intent, such as a beacon, because our receivers have a sensitivity limit to the minimum transmit power above what we transmit unintentionally.”

“But with better instruments, such as the upcoming Square Kilometer Array, we may soon be able to detect signals from alien civilizations communicating with our spacecraft.”

of the team result will appear in astronomy magazine.

_____

Nick Tasei others. 2024. TRAPPIST-1 wireless technology signature search using the Allen Telescope Array. A.J.in press. arXiv: 2409.08313

Source: www.sci.news

Hubble Space Telescope and New Horizons team up to study Uranus

In a new study, astronomers compared high-resolution images of Uranus from the NASA/ESA Hubble Space Telescope with more distant views from NASA’s New Horizons spacecraft. Their results could serve as “ground truth” observations to use as a baseline for interpreting exoplanet direct imaging data from future observatories.

In this image, two three-dimensional shapes of Uranus (top) are compared to the actual views of Uranus from Hubble (bottom left) and New Horizons (bottom right). Image credits: NASA/ESA/STScI/Samantha Hasler, MIT/Amy Simon, NASA-GSFC/New Horizons Planetary Science Theme Team/Joseph DePasquale, STScI/Joseph Olmsted, STScI.

Direct imaging of exoplanets is an important technique for understanding their potential habitability and provides new clues to the origin and formation of our own solar system.

Astronomers use both direct imaging and spectroscopy to collect light from observed planets and compare their brightness at different wavelengths.

However, exoplanets are notoriously difficult to image because they are so far away.

Their images are just pinpoints, so they aren’t as detailed as our close-up view of the world around the sun.

Astronomers can also directly image exoplanets only in “partial phase,” when only part of the planet is illuminated by its star as seen from Earth.

Uranus was an ideal target as a test to understand future long-range observations of exoplanets by other telescopes for several reasons.

First, many known exoplanets are gas giants with similar properties. Also, at the time of the observation, New Horizons was on the far side of Uranus, 10.5 billion kilometers (6.5 billion miles) away, and was able to study the twilight crescent moon. This is not possible from Earth.

At that distance, New Horizons’ view of the planet was just a few pixels wide of its color camera (Multispectral Visible Imaging Camera).

Meanwhile, Hubble’s high resolution allowed it to see atmospheric features such as clouds and storms on the dayside of the gas world from its low orbit, 2.7 billion kilometers (1.7 billion miles) from Uranus. .

Samantha Hassler, an astronomer at the Massachusetts Institute of Technology, said: “We expected Uranus to look different depending on the observation filter, but New Horizons data taken from different perspectives actually show that Uranus looks different than expected.'' It turned out to be much darker than that.”

The gas giant planets in our solar system have dynamic and variable atmospheres with changing cloud cover. How common is this in exoplanets?

Knowing the details of what Uranus’ clouds looked like from Hubble will allow researchers to test what they can interpret from New Horizons’ data.

In the case of Uranus, both Hubble and New Horizons observed that the brightness does not change as the planet rotates. This indicates that the cloud characteristics are not changing due to the rotation of the planet.

But the significance of New Horizons’ detection has to do with how the planet reflects light at a different phase than what Hubble and other observatories on or near Earth can see.

New Horizons showed that exoplanets can be dimmer than predicted at partial and high phase angles, and that their atmospheres reflect light differently at partial phase.

“The groundbreaking New Horizons study of Uranus from a vantage point that cannot be observed by any other means adds to the mission’s treasure trove of new scientific knowledge and, like many other data sets obtained on the mission, will Dr. Alan Stern, Principal Investigator of New Horizons and Research Scientist at the Southwest Research Institute, said:

“NASA’s next Nancy Grace Roman Space Telescope, scheduled to launch by 2027, will use a coronagraph to block out starlight and directly observe gas giant exoplanets,” Hassler said. Ta.

“NASA’s Habitable World Observatory, in its early planning stages, will be the first telescope specifically designed to search for biosignatures in the atmospheres of rocky Earth-sized planets orbiting other stars. .”

“Studying how known benchmarks like Uranus appear in distant images will help us have more solid expectations as we prepare for these future missions. And it will help our It’s critical to success.”

Scientists are result this week’s DPS56Annual Meeting of the Planetary Science Division of the American Astronomical Society.

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S. Hassler others. 2024. Observations of Uranus at high phase angles by New Horizons Ralph/MVIC. DPS56

This article has been adapted from the original release by NASA.

Source: www.sci.news

NGC 5248’s Starburst Region Uncovered by Hubble Space Telescope

Hubble's Wide Field Camera 3 (WFC3) has captured a striking new image of the grand design spiral galaxy NGC 5248.

This Hubble image shows the Grand Design spiral galaxy NGC 5248, located approximately 42 million light-years away in the constellation Bootes. The color images were created from separate exposures taken in the visible, ultraviolet, and near-infrared regions of the spectrum using Hubble's WFC3 instrument. Six filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: NASA / ESA / Hubble / F. Belfiore / J. Lee / PHANGS-HST team.

NGC5248 It is located in the constellation Bootes, about 42 million light years away.

This spiral galaxy, also known as Caldwell 45, LEDA 48130, UGC 8616, IRAS 13353+0908, and TC 830, has a diameter of 95,000 light years.

beginning discovered It was discovered on April 15, 1784 by German-born British astronomer William Herschel and is a member of the NGC 5248 galaxy group.

NGC 5248 has an apparent magnitude of 10, so it doesn't appear very bright, but it can be spotted with a small telescope.

The galaxy is noteworthy Because of the nuclear ring, which has “hot spots” of starburst activity.

“NGC 5248 is one of the so-called 'grand design' spirals, with prominent spiral arms extending from near the center through the disk,” Hubble astronomers said in a statement.

“There is also a faint bar structure in the center between the inner edges of the spiral arms, which is less obvious in this visible-light portrait from Hubble.”

“Features like this that break a galaxy's rotational symmetry have profound effects on how matter moves through it and ultimately on its evolution over time.”

“They can supply gas from the outer reaches of the galaxy to the inner star-forming regions and even to the black hole at the center of the galaxy, where it can start an active galactic nucleus.”

“These gas flows have significantly shaped NGC 5248, with many bright regions of intense star formation spread throughout the disk and dominated by populations of young stars.”

“This galaxy has two very active ring-like starburst regions filled with young star clusters around its core.”

“While these 'nuclear rings' are noteworthy enough, nuclear rings usually tend to prevent gas from penetrating further into the center of the galaxy.”

“The fact that NGC 5248 has a second ring inside the first shows how powerful its flow of matter and energy is.”

“Due to its relatively close proximity and highly visible starburst region, this galaxy is a target for professional and amateur astronomers alike.”

Source: www.sci.news

First Detailed Map of Solar Coronal Magnetic Field Created by Inouye Solar Telescope

This groundbreaking achievement will improve our understanding of the Sun’s atmosphere and shed light on how its changing conditions affect our technology-dependent society.



The Inouye Solar Telescope has released the first map of the magnetic field signal in the solar corona measured using the Zeeman effect. Image courtesy of NSF/NSO/AURA/NASA’s Solar Dynamics Observatory.

The Earth’s magnetic field protects us from the solar wind, protects our atmosphere and makes life possible.

But electromagnetic fields and high-energy particles from extreme solar activity could disrupt satellites, power grids, and other systems necessary for an increasingly technological society.

Understanding these dynamic interactions, which change on timescales ranging from days to centuries, is crucial to safeguarding our infrastructure and current ways of life.

Measuring the magnetic properties of the Sun’s corona, or outer atmosphere, has long challenged astronomers and the limits of technology.

today, Daniel K. Inouye Solar TelescopeLocated near the summit of Haleakala on the Hawaiian island of Maui, the facility is a state-of-the-art facility designed to study coronas.

The satellite has produced the first and most detailed map of the coronal magnetic field to date, taking an important first step in solving these mysteries.

“Inoue’s achievements in mapping the Sun’s coronal magnetic field are a testament to the innovative design and capabilities of this pioneering and unique observatory,” said Dr. Tom Shad, NSF National Solar Observatory investigator.

“This groundbreaking discovery is expected to greatly improve our understanding of the Sun’s atmosphere and its impact on the solar system.”

The researchers used the Zeeman effect, which measures magnetic properties by observing the splitting of spectral lines, to create a detailed map of the magnetic field of the solar corona.

“Spectral lines are distinct lines that appear at particular wavelengths in the electromagnetic spectrum and represent light absorbed or emitted by atoms and molecules,” they explained.

“These lines are unique to each atom and molecule and act like a fingerprint. By looking at the spectrum, scientists can determine the chemical composition and physical properties of an object.”

“When exposed to a magnetic field like the Sun’s, these lines split apart, giving us insight into the magnetic properties of the object.”

Previous attempts to detect such signals, last reported 20 years ago, have lacked the detail and regularity needed for widespread scientific investigation.

Now, Inouye’s unparalleled capabilities make it possible to study these important signals in detail and on a regular basis.

The solar corona can usually only be seen during a total solar eclipse, when most of the Sun’s light is blocked and Earth’s sky becomes dark.

But the Inouye Telescope uses a technique called coronagraphy to create an artificial eclipse that allows it to detect extremely faint polarized signals, highlighting its unparalleled sensitivity and cementing its status as a unique window into viewing our home star.

This telescope is Cryogenic near-infrared spectropolarimeter (Cryo-NIRSP) is one of the telescope’s main instruments used to study the corona and map its magnetic field.

“Just as detailed maps of the Earth’s surface and atmosphere have improved the accuracy of weather forecasts, this remarkably complete map of the magnetic field of the Sun’s corona will help us more accurately predict solar storms and space weather,” said Dr. Carrie Black, program director for NSF’s National Solar Observatory.

“The invisible yet incredibly powerful forces captured in this map will continue to drive solar physics for the next century and beyond.”

“Mapping the strength of the corona’s magnetic field is a fundamental scientific advance not only for solar research but for astronomy in general,” said Dr. Christoph Keller, director of the National Solar Observatory.

“This marks the beginning of a new era in understanding how stars’ magnetic fields affect planets in our solar system and the thousands of exoplanetary systems currently known.”

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This article has been edited from an original release by the National Solar Observatory.

Source: www.sci.news

The Hubble Space Telescope Discovers a Spiral Galaxy Forming Stars

of NASA/ESA Hubble Space Telescope It has provided astronomers with a detailed new image of the barred spiral galaxy NGC 5668.



In this image of the barred spiral galaxy NGC 5668, the Hubble Space Telescope was used to survey the area surrounding a Type II supernova event called SN 2004G to study the types of stars that end their lives as supernovae. The color image is composed of near-infrared and visible light observations by the Hubble Space Telescope's Advanced Camera for Surveys (ACS). Two filters were used to sample different wavelengths. The colors are obtained by assigning a different color to each monochromatic image associated with an individual filter. Image courtesy of NASA / ESA / Hubble / C. Kilpatrick.

NGC 5668 It is located in the constellation Virgo and is about 90 million light years away from Earth.

This galaxy, also known as IRAS 14309+0440, LEDA 52018, and UGC 9363, Found It was discovered on April 29, 1786 by German-born British astronomer William Herschel.

NGC 5668 belongs to two galaxy groups: the NGC 5638 group and the NGC 5746 group.

“At first glance, NGC 5668 does not appear to be a remarkable galaxy,” the Hubble astronomers said.

“It has a diameter of about 90,000 light-years and is roughly the same size and mass as our own Milky Way galaxy. It faces almost head-on, revealing open spiral arms made up of irregular, cloud-like patches.”

“One striking difference between the Milky Way and NGC 5668 is that new stars are forming 60 percent faster in this galaxy.”

“This confirms a galaxy with swirling clouds and gas flows, and bad weather that creates the perfect conditions for new star formation.”

Astronomers have identified two main drivers of star formation in NGC 5668.

“First, this high-quality Hubble Space Telescope snapshot reveals a central bar,” the researchers said.

“Although it may appear slightly elliptical rather than truly bar-shaped, it is likely to influence the galaxy's star formation rate, similar to the bar-like structure at the centers of many spiral galaxies.”

“Second, a high-velocity hydrogen gas cloud has been tracked moving perpendicularly between the galaxy's disk and the faint, spherical halo that surrounds it.”

“They are produced by the powerful stellar winds of hot, massive stars, which feed gas into new star-forming regions.”

“The elevated star formation rate in NGC 5668 is accompanied by a corresponding abundance of supernova explosions,” the researchers said.

“It has been discovered three times in our galaxy, in 1952, 1954, and 2004.”

Source: www.sci.news

Hubble Space Telescope Snaps Photo of NGC 346 in Ultraviolet Light

The Hubble team has released a striking new photo taken with the NASA/ESA Hubble Space Telescope of NGC 346, an open star cluster in one of our Milky Way galaxy’s closest neighbors.



This Hubble Space Telescope image shows the open star cluster NGC 346, located about 210,000 light-years away in the constellation Sigurd. Image courtesy of NASA/ESA/C. Murray, Space Telescope Science Institute/Gladys Kober, NASA, and The Catholic University of America.

NGC 346 is located in the constellation Tucana and is about 210,000 light-years away.

Also known as ESO 51-10, Kron 39, and Lindsay 60, the star cluster was discovered on August 1, 1826, by Scottish astronomer James Dunlop.

NGC 346 is part of the Small Magellanic Cloud, a dwarf galaxy that is a satellite of the Milky Way galaxy.

The cluster was formed approximately 3 million years ago, has a diameter of 150 light years, and a mass 50,000 times that of the Sun.

“NGC 346’s hot stars are unleashing torrents of radiation and energy outflows that are eating away at the dense gas and dust of the surrounding nebula N66,” Hubble astronomers said in a statement.

“Dozens of hot, blue, high-mass stars shine within NGC 346, and the cluster is thought to contain more than half of the known high-mass stars in the entire Small Magellanic Cloud.”

The Hubble Space Telescope has previously observed NGC 346, but this new image shows the cluster in ultraviolet light, along with visible light data.

“Ultraviolet light helps us understand star formation and evolution, and Hubble is the only telescope capable of sensitive ultraviolet observations thanks to its sharp resolution and its location above the ultraviolet-blocking atmosphere,” the astronomers write.

“These particular observations were collected to learn more about how star formation shapes the interstellar medium – the gas distributed throughout seemingly empty space – in metal-poor galaxies like the Small Magellanic Cloud.”

“Elements heavier than hydrogen and helium are called ‘metals’, and the Small Magellanic Cloud has a lower metal content than most of the Milky Way.”

“This situation serves as an excellent example of a galaxy similar to those that existed in the early universe when there were few heavy elements to take up.”

Source: www.sci.news

Active Spiral Galaxy Discovered by Hubble Telescope

Astronomers have captured stunning photos of the lenticular spiral galaxy IC 4709 using the NASA/ESA Hubble Space Telescope.



The Hubble Space Telescope has captured a beautiful picture of IC 4709's swirling disk, filled with stars and dust bands, and the faint halo that surrounds it. The color image is composed of observations in the near-infrared and visible parts of the spectrum by the Hubble Space Telescope's Advanced Camera for Surveys (ACS). The image is based on data obtained through two filters. The colors are obtained by assigning a different hue to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / M. Koss / A. Barth.

No. 4709 It is located in the Southern Telescope constellation and is about 240 million light years away from Earth.

Also known as ESO 182-14 or LEDA 61835, the galaxy has a diameter of 60,000 light years.

IC 4709 is Found It was discovered on September 14, 1901 by American astronomer DeLisle Stewart.

In the galaxy Active galactic nucleiIt is a compact region at the center, and the material inside it is being pulled towards the supermassive black hole.

“If IC 4709's core were simply filled with stars, it would not be as bright as it is,” Hubble astronomers said in a statement.

“Instead, we have a massive black hole with a mass 65 million times that of the Sun.”

“A disk of gas swirls around and eventually enters this black hole. As it spins, the gas collides with itself and heats up.”

“It reaches such high temperatures that it emits electromagnetic radiation ranging from infrared to visible light to ultraviolet light and beyond, including in this case x-rays.”

“The active galactic nucleus of IC 4709 is obscured by a dark dust belt that is barely visible in the galaxy's centre in Hubble Space Telescope images, blocking optical radiation from the nucleus itself,” the researchers added.

“But Hubble's incredible resolution gives us a detailed picture of very small active galactic nuclei and their interactions with their host galaxies.”

“This is essential for understanding supermassive black holes in galaxies much more distant than IC 4709, where it's impossible to resolve such fine detail.”

Source: www.sci.news

Observation of the diffuse nebula NGC 261 in the Small Magellanic Cloud by the Hubble Space Telescope

NGC 261 is located within the Small Magellanic Cloud, one of the Milky Way's closest neighbors.



This Hubble Space Telescope image shows the diffuse nebula NGC 261, about 200,000 light-years from Earth in the constellation Sivir. Image courtesy of NASA/ESA/LC Johnson, Northwestern University/Gladys Kober, NASA and The Catholic University of America.

NGC 261 It is a diffuse nebula located about 200,000 light years away in the constellation Tetranychus.

The object, also known as Brook 42, ESO 29-12, and IRAS 00447-7322, Found It was discovered on September 5, 1826 by Scottish astronomer James Dunlop.

“The ionized gas burning up from within this diffuse region characterizes NGC 261 as an emission nebula,” the Hubble astronomers said.

“The stars are so hot that they irradiate the surrounding hydrogen gas, giving the clouds a pinkish-red glow.”

The Hubble Space Telescope has turned its keen eye to NGC 261 to study how efficiently stars form within molecular clouds, extremely dense regions of gas and dust.

“These clouds are often composed of large amounts of molecular hydrogen and are the cold regions where most stars form,” the researchers explained.

“But molecular hydrogen is poorly radiative, making it difficult to measure this fuel for star formation in stellar nurseries.”

“Because they're difficult to detect, scientists instead track other molecules present within the molecular cloud.”

“The Small Magellanic Cloud contains a gas-rich environment of young stars, as well as traces of carbon monoxide, which correlates with hydrogen and is a chemical often used to confirm the presence of such clouds.”

The new composite image is Hubble's Advanced Camera for Surveys (ACS) and Wide-angle camera 3 (WFC3) shows such a star in the southwestern part of the Small Magellanic Cloud, where NGC 261 resides.

“The combined powers of the ACS and WFC3 instruments allowed us to probe the star formation properties of the nebula through its carbon monoxide content at visible and near-infrared wavelengths,” the scientists said.

“This work helps us better understand how stars form in our host galaxy and in our Galactic neighbours.”

Source: www.sci.news

Hubble Space Telescope focuses on Pegasus dwarf spheroidal galaxy

The NASA/ESA Hubble Space Telescope captured this stunning image of the Pegasus dwarf elliptical galaxy, a moon of the Andromeda galaxy.



The Pegasus dwarf elliptical galaxy is located about 959,000 light-years away from the Andromeda galaxy. Image credit: NASA / ESA / D. Weisz, University of California, Berkeley / Gladys Kober, NASA and The Catholic University of California.

of Pegasus dwarf spheroidal galaxy It is located about 2.7 million light years away in the constellation Pegasus.

“The Andromeda Galaxy, also known as Messier 31, is the closest large spiral galaxy to the Milky Way and is orbited by at least 13 dwarf moons,” Hubble astronomers said in a statement.

“The Pegasus dwarf spheroidal galaxy is one of these compact galaxies.”

“Dwarf spheroidal galaxies are the faintest and most massive galaxies known,” they explained.

“They tend to have an elliptical shape and a relatively smooth distribution of stars.”

“Dwarf spheroidal galaxies are typically devoid of gas and contain mostly old and intermediate-stage stars, although some have recently undergone a small amount of star formation.”

The Pegasus dwarf spheroidal galaxy, also known as Andromeda VI, was discovered in 1996 in images from the Second Palomar Observatory Sky Survey (POSS II).

“The galaxy is characterised by a low abundance of heavy elements, leaving very little gas needed to form the next generation of stars, although it still has more than many of the dwarf spheroidal galaxies in our Local Group,” the astronomers said.

“Researchers suspect that Andromeda's gravitational field is stripping away star-forming gas, leaving it with insufficient material to form more than a few generations of stars.”

“By comparison, some of the Milky Way's comparable distant dwarf spheroidal companions contain intermediate-age stars, which may be because the Andromeda Galaxy is so massive and extended that its gravitational influence reaches farther.”

“The jury is still out on how dwarf elliptical galaxies form,” they noted.

“Theories include collisions between galaxies that break off smaller pieces, the gravitational influence of larger galaxies on small, disk-like dwarf galaxies, and processes related to the birth of small systems among dark matter aggregates.”

“Andromeda and the Milky Way are the only galaxies close enough for astronomers to observe these faint satellite galaxies, so clues to their formation come from nearby galaxies like this one.”

“Hubble studied this galaxy as part of a survey of the entire Andromeda moon system to investigate important topics such as dark matter, reionization, and the growth of galactic ecosystems through the ages of the universe.”

Source: www.sci.news

UGC 3478 observed by the Hubble Space Telescope

Stunning new images taken by the NASA/ESA Hubble Space Telescope show spiral galaxy UGC 3478 in great detail.

This Hubble Space Telescope image shows UGC 3478, a spiral galaxy located 128 million light-years away in the constellation Camelopardalis. Image credit: NASA / ESA / Hubble / M. Koss / A. Barth.

3478 posts It is located in the constellation Camelopardalis and is approximately 128 million light years away from Earth.

Also known as LEDA 19228, INTREF 304, IRAS 06280+6342, Seyfert galaxyA type of galaxy centered around an active galactic nucleus (AGN).

“If you look at the long, star-filled spiral arms and the dark threads of dust that crisscross them, your eye may be drawn to a bright spot at the center of UGC 3478,” the Hubble astronomers said.

“This spot is the core of a galaxy, and there's something very special about it: it's a growing massive black hole, what astronomers call an AGN.”

“As with other active galaxies, the brightness seen here hides a supermassive black hole at the galaxy's centre,” the researchers added.

“A disk of gas spirals into this black hole, and as the material collides and heats up, it emits extremely intense radiation.”

“The spectrum of this radiation includes hard X-ray emission, which makes it clearly distinguishable from stars in the galaxy.”

“Despite the strong brightness of the compact central region, the surrounding galactic disk is still clearly visible, making it a Seyfert galaxy.”

“Astronomers know that many active galaxies are far away from Earth because their nuclei are so bright that they stand out next to other fainter galaxies.”

“Located 128 million light-years away, UGC 3478 is Earth's very own neighbour,” the astronomers said.

The new image of UGC 3478 is Hubble's Advanced Camera for Surveys (ACS) is in the near infrared and optical parts of the spectrum.

Two filters were used to sample different wavelengths, and color was generated by assigning a different hue to each monochromatic image associated with an individual filter.

“The data used to create this image come from Hubble Space Telescope surveys of nearby powerful AGNs discovered in such relatively high-energy X-rays and are expected to help us understand how galaxies interact with their central supermassive black holes,” the researchers said.

Source: www.sci.news

The Importance of Saving the Chandra Space Telescope

Chandra X-ray Observatory

NASA/CXC & J. Vaughan

On July 23, 1999, just a few months before I enrolled in college, NASA’s Space Shuttle Columbia launched with a precious cargo. Not only was it carrying a crew led by the first woman, Eileen Collins, its primary purpose was to launch the Chandra X-ray Observatory, a new flagship space telescope. Chandra This was the heaviest payload ever carried by a NASA space shuttle and turned out to be one of the last two missions completed by Columbia before it tragically exploded after launch on February 1, 2003.

Chandra is the first, and so far only, NASA mission named after a person of color. The late theoretical astrophysicist and Nobel Prize winner Subramanian Chandrasekhar was called Chandra by his friends and family. Chandrasekhar, whose last name means “crown of the moon,” made many important contributions to astrophysics. His most important work was discovering the Chandrasekhar limit, the maximum mass a white dwarf remnant can have before it collapses into a black hole.

It's fitting that an X-ray telescope mission should be named after a scientist who has spent his life thinking about the physics of black holes, as X-ray telescopes play a key role in black hole research. X-rays are high-energy light waves, which means they are produced in extremely energetic environments, such as those around black holes, where extreme distortions of space-time cause strong gravitational forces to accelerate particles to extremely high speeds. In other words, when we look at the universe through the lens of X-ray astronomy, rather than the visible wavelengths of traditional telescopes, we see an entirely different universe.

Importantly, X-ray astronomy can't be done from the Earth's surface, because it's blocked by the Earth's atmosphere. That's good for human health, but not so good for astronomers. Chandra is therefore a reminder of just how important it is to keep low Earth orbit debris-free, so we can safely launch space telescopes that perform tasks that are simply beyond the control of the Earth.

I feel like I have grown up with Chandra. And not just because I attended college at Chandra headquarters, now known as the Center for Astrophysics (CfA) in Massachusetts, and was often mistakenly called “Chandra”. One of my lab projects as an undergraduate was to adjust the light-gathering part of Chandra's backup camera. The following year, I wrote my undergraduate thesis under the guidance of Martin Elvis, an expert in X-ray astronomy. My research focused on the particle winds that fly out of galaxies that contain supermassive black holes. I used Chandra data to analyze what structures these galaxies take. It is true that Martin's letter helped me secure admission to at least one PhD program. In other words, without Chandra, my career may never have begun.

I am one of thousands of scientists in the fields of physics and astronomy who can tell similar stories of how Chandra data was the foundation of the early stages of their careers, or how they have dedicated their lives to using Chandra to explore the mysteries of the universe. Laura Lopez Ohio State University has used Chandra for many years to study supernovae. Daniel Castronow a staff scientist at CfA, is doing the same thing. The three of us were postdoctoral fellows at MIT and are from a generation that grew up on the power of the Chandra X-ray Observatory.

Now, after 25 years in orbit, Chandra is under threat – not the reality of space debris and aging equipment, but the political climate. US President Joe Biden's appointees to head NASA recently tried to scale back the project, but the scientific community worked with Congress to save the mission. But things will never be the same. A compromise proposal, which has not yet been signed into law, would drastically cut Chandra's funding and limit its scientific scope. Notably, there is no scientific basis for opposing the plan. Recommendations They have an army of expert advisers, but NASA has cut funding it had already promised to scientists, leaving PhD students and postdocs without enough money to cover living expenses.

Chandra deserves better. And so does its global audience. Thanks to Chandra, we have discovered new neutron stars and learned about their interiors. Our knowledge of black holes has blossomed. We have gained a deeper understanding of stellar life cycles and the history of our galaxy. We have been able to study galaxy clusters and learn how dark matter is distributed within them, putting the Milky Way in context. There is still time to save Chandra, a monument to human ingenuity. The fact that it is still going strong after 25 years should be celebrated and it should be honoured by the continuation of the mission.

Chanda's Week

What I'm Reading

My friend is Andrea Kindried. From Slavery to the Stars: A Personal Journey And it's beautiful.

What I'm seeing

I've seen some classic episodes Star Trek: The Next Generation Like “Remember Me”.

What I'm working on

I am developing a new course that prepares students to understand science in a social context..

Chanda Prescod Weinstein is an associate professor of physics and astronomy and a faculty member of women's studies at the University of New Hampshire. Her latest book is A Disordered Universe: A Journey into Dark Matter, Space-Time, and Dreams Deferred.

topic:

Source: www.newscientist.com

New Images of UGC 4879 Captured by Hubble Space Telescope

Hubble astronomers have released a stunning new image of the dwarf irregular galaxy UGC 4879, taken by the NASA/ESA Hubble Space Telescope.

This Hubble Space Telescope image shows irregular dwarf galaxy UGC 4879, about 3.6 million light-years away in the constellation Ursa Major. Image credit: NASA / ESA / Hubble Space Telescope / K. Chiboucas, NOIRLab and Gemini North / M. Monelli, Canarian Astrophysics Institute / Gladys Kober, NASA and Catholic University.

UGC 4879 is an irregular dwarf galaxy in the constellation Ursa Major.

Also known as VV124 and LEDA 26142, this galaxy is quite isolated.

It lies 3.6 million light years from our Milky Way galaxy and 3.9 million light years from the Andromeda galaxy.

Dwarf galaxy Leo A, located about 1.6 million light-years away, is UGC 4879's closest neighbor.

This isolation makes UGC 4879 an ideal laboratory to study primordial star formation, without the complications of interactions with other galaxies.

There are only two other galaxies in the Local Group that have a similar, though slightly lower, isolation to UGC 4879: DDO 210 and SgrDIG, which are located in the opposite direction from UGC 4879.

“UGC 4879 is an isolated dwarf galaxy that lies just outside our Local Group of galaxies,” Hubble astronomers said in a statement.

“Because of its isolation, we are studying UGC 4879 to determine whether it is an old, relatively undisturbed galaxy.”

“Theories suggest that the least massive dwarf galaxies may have formed first.”

“If UGC 4879 is a relic from the early universe, it may offer clues about the hierarchy and evolution of galaxies, galaxy clusters, and even the universe itself.”

This image of UGC 4879 combines data from two Hubble observing programs focused on learning more about how dwarf galaxies form and evolve.

Source: www.sci.news

Hubble Space Telescope captures photo of obscure barred spiral galaxy

Astronomers have created a beautiful image of the barred spiral galaxy UGC 11861 using the NASA/ESA Hubble Space Telescope.

This Hubble Space Telescope image shows UGC 11861, a barred spiral galaxy in the constellation Cepheus, 69 million light-years from Earth. Image credit: NASA / ESA / Hubble / C. Kilpatrick.

11861 posts It is located in the northern constellation Cepheus and is about 69 million light years away from Earth.

The galaxy, also known as LEDA 67671, IRAS 21557+7301, or TC 609, is classified as a barred spiral galaxy and a candidate active galactic nucleus.

UGC 11861 is Composed It consists of an exponential disk, a central box-shaped structure, and two broad spiral arms.

“The galaxy is actively forming new stars amidst clouds of gas and dark dust grains, visible as glowing blue spots in the outer arms,” ​​Hubble astronomers said in a statement.

“As a result of this activity, three supernova explosions have been observed in and near UGC 11861, in 1995, 1997, and 2011.”

“The first two were both Type II supernovae, the kind that result from the collapse of a massive star at the end of its life.”

“This Hubble image was made from data collected to study a Type II supernova and its environment.”

The color image of UGC 11861 was created from images taken separately in the visible and near-infrared regions of the spectrum. Hubble’s Advanced Camera for Surveys (ACS).

Two filters were used to sample different wavelengths, and color was generated by assigning a different hue to each monochromatic image associated with an individual filter.

“UGC 11861 is located 69 million light-years from Earth, which may seem a very long distance, but it was just the right distance for the Hubble Space Telescope to capture this spectacular photo of the galaxy’s spiral arms and the short, bright bar at its center,” the astronomers wrote.

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Hubble Space Telescope captures stunning image of a barred spiral galaxy

Astronomers have used the NASA/ESA Hubble Space Telescope to capture striking new photos of LEDA 12535, a barred spiral galaxy located in the famous Perseus Cluster of galaxies.

This Hubble Space Telescope image shows LEDA 12535, a barred spiral galaxy about 320 million light-years away in the constellation Perseus. The color composite was created from images taken with the Hubble Space Telescope's Wide Field Camera 3 (WFC3) in ultraviolet, visible, and near-infrared light. It is based on data obtained through three filters. The colors are obtained by assigning a different hue to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / I. Chilingarian.

LEDA12535 It is located about 320 million light years away in the constellation Perseus.

Also known as MCG+07-07-072 or SDSS J032041.39+424814.8, it is classified as a barred spiral galaxy.

“LEDA 12535 has a highly unusual shape for a spiral galaxy, with thin arms extending from the ends of its barred nucleus and tracing a nearly circular path around the disk,” the Hubble astronomers said.

“Using a common extension of Hubble's basis system, it is classified as an SBc(r) galaxy. The c indicates that the two spiral arms are loosely wound, each completing only a half revolution around the galaxy, and the (r) refers to the ring-like structure they produce.”

“Galactic rings come in a variety of shapes, from merely unusual to rare and astrophysically important.”

“Lenticular galaxies are a type of galaxy that lies intermediate between elliptical and spiral galaxies,” the astronomers added.

“Unlike elliptical galaxies, they feature large disks but lack spiral arms.”

“Lenticular means lens-shaped, and these galaxies often feature a ring-like shape in their disks.”

“The classification of ring galaxies, on the other hand, is only applied to unusual galaxies with a round ring of gas and star formation that closely resembles spiral arms but is either completely detached from the galactic core or lacks a visible core at all.”

“They are thought to have formed from the collision of galaxies.”

“Finally, there is the famous gravitational lensing, where the ring is actually a distorted image of a distant background galaxy, formed by the 'lensing' galaxy bending the light around it.”

“The ring-shaped images, called Einstein rings, can only form if the lensed galaxy and the photographed galaxy are perfectly aligned.”

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