Discovering a Barred Spiral Galaxy: Unveiling Cosmic Secrets Just 2 Billion Years Post-Big Bang

Using high-resolution images, NIRCam, a near-infrared camera aboard the NASA/ESA/CSA James Webb Space Telescope, has led astronomers to discover COSMOS-74706, one of the earliest known barred spiral galaxies. This discovery is pivotal in shaping our understanding of cosmic evolution.



COSMOS-74706: Unsharp mask overlaid on F200W, F277W, and F356W filter configurations. The white lines represent logarithmic spirals along the galaxy’s arm structure while the lines indicate the north-south bar structure. Image credit: Daniel Ivanov.

The barred spiral galaxy COSMOS-74706 existed approximately 11.5 billion years ago.

“This galaxy developed its bar just two billion years after the universe’s inception,” stated Daniel Ivanov, a graduate student at the University of Pittsburgh.

“Stellar bars are linear features found at the centers of galaxies, confirming their namesakes.”

COSMOS-74706’s bar comprises a dense collection of stars and gas, appearing as a bright line bisecting the galaxy when viewed perpendicularly to its plane.

Stellar bars significantly influence a galaxy’s evolution, funneling gas from the outskirts into the center, which feeds the supermassive black hole and can inhibit star formation within the galactic disk.

While previous reports identified barred spiral galaxies, their analyses were inconclusive due to the less reliable optical redshift methods compared to the spectroscopy used for COSMOS-74706 verification.

In some instances, a galaxy’s light was distorted by a massive object, leading to a phenomenon known as gravitational lensing.

“Essentially, COSMOS-74706 is the most redshifted spectroscopically confirmed lensless barred spiral galaxy,” Ivanov noted.

“We were not surprised to find barred spiral galaxies so early in the universe’s timeline.”

“In fact, some simulations suggest the bar formed at redshift 5, or roughly 12.5 billion years ago.”

“However, I believe we shouldn’t expect to find many of these galaxies just yet.”

This discovery helps refine the timeline for bar formation, making it a significant finding.

Ivanov and colleagues presented their discoveries on January 8th during the 247th Annual Meeting of the American Astronomical Society.

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Daniel Ivanov et al. 2026 zspec>3 barred spiral without lens. AAS247

Source: www.sci.news

Hubble Captures Bizarre Spiral Galaxy: NGC 1511

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



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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

ALMA Observes Spiral Gas Streamers Controlled by Magnetic Fields in Star-Forming Areas

This stream of gas transports material from the clouds surrounding the star-forming area within Perseus directly into an emerging binary star system known as SVS 13A.

Artist’s impression of the SVS 13A system. Image credit: NSF/AUI/NSF’s NRAO/P.Vosteen.

Stars are formed from clouds of gas and dust, and recent observations indicate that the process of star formation is far more dynamic than previously understood.

New findings from the Atacama Large Millimeter/Submillimeter Array (ALMA) reveal both dust and molecules swirling around the SVS 13A system. This data shows how the magnetic field not only permeates these stellar nurseries but actively directs the flow of matter, offering a preferred path for gas to accumulate in the disk where new stars and planets arise.

“Visualize a garden hose, but instead of water, it smoothly channels materials for star formation through intricate pathways carved by unseen forces,” explains Dr. Paulo Cortes, an astronomer at the NSF National Radio Astronomy Observatory and the joint ALMA telescope.

“This perspective from ALMA observations presents channels of gas known as subalfvénic streamers, regulated by spiral magnetic field lines.”

“This new data provides an insightful glimpse into the star formation process.”

“These streamers illustrate how magnetic fields can influence star formation by managing material influx, akin to a private highway facilitating car travel.”

ALMA’s images and findings uncover two spiral arms of dust encircling the star, with gas streams closely mirroring the same trajectory.

This remarkable configuration implies that the gas within the streamer is traversing at a slower pace than previously believed, reinforcing the concept of a magnetized channel rather than a chaotic, collapsing cloud.

The presence of such streamers, linking clouds to disks and supplying them with material in a managed fashion, indicates that both gravity and magnetism are crucial in the formation of stars and the shaping of potential planetary bodies around them.

This groundbreaking result signifies the first instance where astronomers have directly mapped both a streamer and its associated magnetic field in a single observation.

“Subalfvenic streamers indicate a fresh role for magnetic fields amidst gravitational dominance, acting as ‘guides’ to assist the descent of material from the outer envelope to the disk,” the astronomers remarked.

Upcoming findings are detailed in a paper in the Astrophysics Journal Letter.

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PC Cortez et al. 2025. First results from ALPPS: SVS 13A subalfvenic streamer. APJL 992, L31; doi: 10.3847/2041-8213/ae0c04

Source: www.sci.news

Hubble Captures Stunning Image of Dusty Spiral Galaxy NGC 7496

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Spiral Lasers Can Manage Their Unruly Magnetic Counterparts

Materials resembling magnets exhibit internal spirals that can solely be controlled with circularly polarized lasers.

Andrew Ostrovsky/iStockphoto/Getty Images

Scientists have successfully regulated the behavior of a previously elusive material, akin to magnetism, which may eventually lead to improved hard drives.

When a bar magnet is introduced to a magnetic field, it rotates due to that influence. However, materials characterized by a property called strong axis remain stationary under all known magnetic fields. Recently, Zeng Zhiyang and his team at the Max Planck Institute for the Structure and Mechanics of Matter in Germany discovered a method to manipulate strong-axis properties using lasers.

A conventional magnetic material is often thought of as a collection of many small bar magnets. Zeng explains that for strong-axis materials, it is more accurate to envision a group of dipoles (two opposing charges separated by a small distance) swirling in a minor spiral. He and his team realized they could control these vortices with laser pulses containing a specific swirl.

The researchers adjusted the laser to emit circularly polarized light. Upon striking a strong-axis material (specifically a compound made of rubidium, iron, molybdenum, and oxygen), it induced rotation in the material’s atoms, altering the dipole’s direction of motion.

Team member Michael Forst from the Max Planck Institute for Structure and Mechanics of Matter remarked that while it has been established that light can effectively control materials—transforming conductors into insulators and vice versa—tailoring light’s properties for material control has presented a significant technical challenge.

“This serves as a strong proof of concept,” notes Theo Rasing at Radboud University in the Netherlands. He adds that this material adds to the growing array of options for constructing more efficient and stable memory devices, such as hard drives that store information in electromagnetic charge patterns.

However, the current experiments necessitate cooling the material to approximately -70°C.°C (-94°F). Additionally, because the team’s laser was relatively large, Forst indicates that more development is required before a practical device can realistically be constructed.

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Source: www.newscientist.com

Hubble Space Telescope Captures Stunning Spiral Galaxy: NGC 6000

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble Captures Image of Active Spiral Galaxy NGC 7456

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble Space Telescope Captures a Mesmerizing Spiral Galaxy Spin

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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 Captures the Breathtaking Barred Spiral Galaxy: IC 758

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble Captures Stunning Spiral Galaxy: NGC 3507

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



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

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

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

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

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

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

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

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

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

“Distant galaxies tend to lack fine details.”

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

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

Source: www.sci.news

Hubble Captures Direct View of Intermediate Spiral Galaxy

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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

Webb finds a Milky Way-like spiral galaxy in ancient universes

Astronomers using the NASA/ESA/CSA James Webb Space Telescope discovered a very ancient grand design spiral galaxy that existed just a billion years after the Big Bang. Named Zhúlóng (Torch Dragon), this galaxy is the most distant bulging disc galaxy candidate for which spiral arms have been known to date.

This image of Zhúlóng, the furthest spiral galaxy discovered to date, shows its very well-defined spiral arm, old bulge in the middle, and a large star-forming disc resembling the structure of the Milky Way. Image credits: NASA/CSA/ESA/M. Xiao, University of Geneva/G. Brammer, Niels Bohr Institute/Dawn JWST Archive.

Large spiral galaxies like our Milky Way are expected to take billions of years to form.

For the first billion years of universe history, galaxies are considered small, chaotic and irregular.

However, Webb is beginning to reveal very different photos.

Telescope deep infrared imaging reveals surprisingly large and well-structured galaxies much earlier than previously expected.

Among these new findings is Zhúlóng, the most distant spiral galaxy candidate ever identified, seen at a redshift of 5.2.

Despite this early period, galaxies exhibit surprisingly mature structures. Old bulge in the middle, large star-forming discs, spiral arms – a feature usually found in nearby galaxies.

“What stands out for Zhúlóng is both how similar it is to the Milky Way, its shape, size and star mass,” says Dr. Mengyuan Xiao, a postdoctoral researcher at Unige.

“The disc spans over 60,000 light years, comparable to our own galaxy, and the star contains over 100 billion solar masses.”

“This makes it one of the most persuasive Milky Way analogs discovered at such an early age, raising new questions about how a large, ordered spiral galaxy will form right after the Big Bang.”

The Zhúlóng Galaxy was discovered as part of a panoramic investigation.

“The findings highlight the possibility of purely parallel programs to reveal rare, distant objects that stress-test galaxy formation models,” says Dr. Christina Williams, a No-Arab astronomer and lead researcher of the Panorama Program.

Spiral structures were previously thought to take billions of years, but large galaxies were not expected to exist much later in the universe.

“The discovery shows that Webb is fundamentally changing the way we see the universe in its early days,” says Professor Pascal Oesch, an astronomer at Unige and a co-researcher of the Panorama Program.

a paper The discovery was published in the journal today Astronomy and Astrophysics.

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Mengyuan Xiao et al. 2025. Panorama: Discovery of a super gentle grand design spiral galaxy from z to 5.2. A&A 696, A156; doi:10.1051/0004-6361/202453487

Source: www.sci.news

Anomalies in the Universe: Massive spiral galaxies expel enormous pairs of relativistic jets

2MASX J23453268-0449256 (J2345-0449 for short), a very huge, rapidly spinning, jet lag spiral galaxy with approximately 947 million light years in the Aquarius constellation, a mass of billions of people billions that are billions of times the sun’s, and mounted on a massive radio jet spanning six million light years. This is one of the largest known in any spiral galaxy, and such powerful jets are almost exclusively found in elliptical galaxies rather than spiral, thus covering the conventional wisdom of galaxies’ evolution. It also means that the Milky Way can potentially create similar energetic jets in the future.



This image shows the Spiral Galaxy 2Masx J23453268-0449256 and its huge radio jet. Image credit: Bagchi et al. /Giant Metrure Lave Radio Telescope.

“This discovery is more than just weird. It forces us to rethink the evolution of galaxies and how super-large black holes grow and shape the environment within them,” said Professor Joydeep Baguch of Christ University.

“If spiral galaxies can not only survive, but also thrive under such extreme conditions, what does this mean for the future of our own Milky Way galaxies?”

“Can our Galaxy experience similar high-energy phenomena that have serious consequences for the survival of precious lives within it?”

In a new study, astronomers have unraveled the structure and evolution of the Spiral Galaxy J2345-0449, three times the size of the Milky Way.

Using observations from NASA/ESA Hubble Space Telescope, Giant Metruh Rave Radio Telescope, Atacama’s Large Millimeter/Sub-Millimeter Array (ALMA), and multi-wavelength analysis, we detected the giant ultrafine black holes of its mind and radio jets in the largest radio jets by creating rare galaxies.

Traditionally, scientists believed that such huge, superimpression violent activities would destroy the delicate structures of spiral galaxies.

But for all possibilities, J2345-0449 retains its quiet nature with a well-defined spiral arm, bright nuclear bars and an uninterrupted ring of stars.

In addition to enigma, the galaxy is surrounded by vast halos of hot x-ray exhaust, providing important insights into its history.

This halo cools slowly over time, but the black hole jets act like space furnaces, preventing new star formation despite the abundant star-building materials present.

The authors also found that J2345-0449 contains 10 times the dark matter as the Milky Way.

“Understanding these rare galaxies could provide important clues about the invisible forces that govern the universe, such as the nature of dark matter, the long-term fate of the galaxy, and the origin of life,” says Ph.D. A student at the University of Christ.

“In the end, this research brings us one step closer to solving the mystery of the Cosmos and reminds us that the universe holds surprise beyond our imagination.”

Survey results It was published in Monthly Notices from the Royal Astronomical Society.

____

Joydeep Bagchi et al. 2025. Announcing bulge disk structures, AGN feedback and baryon landscapes in a large helical galaxy with MPC-scale radio jets. mnras 538(3): 1628-1652; doi: 10.1093/mnras/staf229

Source: www.sci.news

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble’s Observation of a Spiral Galaxy Hosting a Supernova

NASA has released a beautiful photo of spiral galaxy LEDA 22057 taken by the NASA/ESA Hubble Space Telescope.

This Hubble image shows spiral galaxy LEDA 22057 about 650 million light-years away in the constellation Gemini. Image credits: NASA/ESA/Hubble/RJ Foley, University of California, Santa Cruz.

Leda 22057 It is located in the constellation Gemini, about 650 million light years away from Earth.

Also known as AGC 170923, MaNGA 11743-12703, or 2MASX J07524264+1450263, this galaxy is the site of a supernova explosion.

“This special supernova… SN2024piwas discovered by automated research in January 2024,” Hubble team members said in a statement.

“This survey covered the entire northern half of the night sky every two days and cataloged more than 10,000 supernovae.”

New images of LEDA 22057 consist of observations from. Hubble’s Wide Field Camera 3 (WCF3) Located in the infrared part of the spectrum.

“SN 2024pi is visible in this image,” the astronomers said.

“SN 2024pi’s pale blue dot, located just below and to the right of the galactic nucleus, stands out against the galaxy’s ghostly spiral arms.”

“This image was taken about a month and a half after the supernova was discovered, so the supernova appears many times fainter here than at its peak brightness.”

According to the researchers, SN 2024pi supernova belongs to type Ia.

“This type of supernova requires a remarkable object called a white dwarf, which is the crystallized core of a star with a mass less than about eight times the mass of the Sun,” the researchers said.

“When a star of this size runs out of hydrogen in its core, it expands into a red giant, becoming colder, swollen, and brighter.”

“Over time, pulsations and stellar winds strip away the star’s outer layers, leaving behind a white dwarf and a colorful planetary nebula.”

“White dwarfs can have surface temperatures of over 100,000 degrees Celsius and are extremely dense, packing almost the mass of the Sun into a sphere the size of Earth.”

“Nearly all stars in the Milky Way will someday evolve into white dwarfs, a fate that awaits our Sun in about 5 billion years, but not all of them will explode as Type Ia supernovae.”

“For that to happen, the white dwarf must be part of a binary star system.”

“If a white dwarf siphons material from its stellar partner, it could become too massive to support itself.”

“The resulting runaway fusion explosion destroys the white dwarf in a supernova explosion visible many galaxies away.”

Source: www.sci.news

Hubble Captures Stunning Image of Barred Spiral Galaxy NGC 2566

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

The Hubble Space Telescope captures an off-center spiral galaxy

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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

Hubble Captures Mysterious Spiral Galaxy Edge-On

NASA has released a surprising image of the unusual edge-on spiral galaxy UGC 10043 taken by the Hubble Space Telescope.

This Hubble image shows UGC 10043, an unusual spiral galaxy located about 150 million light-years away in the constellation Serpens. Image credits: NASA / ESA / Hubble / R. Windhorst / W. Kiel.

UGC 10043 It is located in the constellation Serpens, about 150 million light years from Earth.

Also known as IRAS 15464+2201 or LEDA 56094, this galaxy is one of the somewhat rarer spiral galaxies. Viewed from the side.

“We see galactic disks as sharp lines through space, with pronounced dust lanes along them,” Hubble astronomers said in a statement.

“This dust is spread throughout UGC 10043's spiral arm, but when viewed from the side it appears very thick and cloudy.”

“I can see some lights, too.” Active star forming region In your arms, shining from behind the dust. ”

“Surprisingly, we can also see that the center of the galaxy has a bright, almost egg-shaped bulge that towers far above and below the disk.”

“All spiral galaxies have such a bulge as part of their structure, containing stars that orbit the center of the galaxy in paths above and below the spiral disk.”

“This is a feature that isn't usually obvious in pictures of galaxies.”

“The unusually large size of this bulge compared to the galaxy's disk is likely due to UGC 10043 sucking up material from nearby dwarf galaxies.”

“This may also be why the disc warps, causing one end to bend up and the other end to bend down.”

The color image of UGC 10043 was created from separate exposures taken in the visible and near-infrared regions of the spectrum. Hubble's advanced survey camera (ACS) and Wide field planetary camera 2 (WFPC2).

Two filters were used to sample different wavelengths.

Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

“Like most full-color images published by Hubble, this image is a composite of multiple individual snapshots taken by Hubble at different times and capturing different wavelengths of light,” the astronomers said. Explained.

“What is remarkable about this image is that the two sets of Hubble data used were collected 23 years apart, in 2000 and 2023.”

“Hubble's longer lifespan not only allows us to generate new and better images of old targets.”

“It also provides a long-term archive of data, making it increasingly useful to astronomers.”

Source: www.sci.news

Hubble revisits NGC 4414: The Majestic Spiral Galaxy

Astronomers using the NASA/ESA Hubble Space Telescope have captured stunning new images of unobstructed spiral galaxy NGC 4414.



This Hubble image shows the unobstructed spiral galaxy NGC 4414 located 51 million light-years away in the constellation of Coma. Image credits: NASA / ESA / Hubble / O. Graur / SW Jha / A. Filippenko.

NGC4414 It is located approximately 51 million light years from Earth in the constellation Coma.

The galaxy, also known as the Dusty Spiral Galaxy, Ark 365, IRAS 12239+3129, LEDA 40692, or UGC 7539, has a diameter of approximately 56,000 light years.

NGC 4414 was first discovered on March 13, 1785 by German-born British astronomer William Herschel.

galaxy belong to It belongs to the Coma I group, a group of galaxies close to the Virgo cluster.

NGC 4414 was previously observed It was studied by Hubble in 1995 and 1999 as part of its research efforts. Cepheid variable star.



This collage features the supernova observed by Hubble in NGC 4414. In the upper left, a large spiral galaxy can be seen tilted diagonally. Each subsequent panel shows a close-up of the galaxy in 1999, 2021, and 2023 to highlight the galaxy's supernovae. Image credits: NASA / ESA / Hubble / O. Graur / SW Jha / A. Filippenko.

“Cepheid stars are a special type of variable star with very stable and predictable brightness changes,” Hubble astronomers said in a statement.

“The period of these fluctuations is determined by the star's physical properties, such as its mass and true brightness.”

“This means that astronomers can learn about the physical properties of Cepheids just by looking at their light fluctuations, and can use that very effectively to determine their distances.”

“For this reason, cosmologists refer to Cepheids as 'standard candles.'”

“Astronomers used Hubble to observe Cepheids like those in NGC 4414, and the results were surprising.”

“Cepheids were then used as a stepping stone to measure distances to supernovae, which in turn gave us a measure of the size of the universe.”

“Today we can tell the age of the universe with much greater precision than before Hubble: about 13.7 billion years.”

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

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

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.

Source: www.sci.news

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.”

Source: www.sci.news

Twisted Spiral Arms Galaxy Hosting Supernova Discovered by Hubble Space Telescope

Astronomers used the NASA/ESA Hubble Space Telescope to capture this image of the barred spiral galaxy LEDA 857074.

This Hubble image shows the barred spiral galaxy LEDA 857074. The color image was created from observations in the near-infrared part of the spectrum with Hubble’s Wide Field Camera 3 (WFC3). Four filters were used to sample different wavelengths. Color is produced by assigning a different hue to each monochromatic image associated with an individual filter. Image courtesy of NASA / ESA / Hubble / RJ Foley.

LEDA857074 It is a barred spiral galaxy located in the constellation Eridanus.

“Hubble has observed a wide range of celestial objects, from galaxies, nebulae and star clusters to planets in our solar system and beyond,” Hubble astronomers said in a statement.

“Observing programs typically aim to collect data that will enable astronomers to answer specific questions.”

“Naturally, this means that most of the planned observations will be directed at objects that astronomers have already studied.”

“Some are well-known, such as the Crab Nebula and the globular cluster Omega Centauri, while others, such as the Spider Galaxy and NGC 4753, are less well known to the public but have been featured in hundreds of scientific papers.”

“This galaxy is not like that: LEDA 857074 has been named in fewer than five papers, one of which is the Lyon-Meudon extragalactic database itself.”

“Apart from its location, virtually no data has been recorded about this object. It has never been studied since it was discovered. So why did it attract the attention of the legendary Hubble telescope?”

In 2022, an automated survey observed a supernova event in LEDA 857074 called SN 2022ADQZ.

“Although astronomers have catalogued millions of galaxies and tens of thousands of supernovae are detected annually today, the probability of discovery in any particular galaxy is low,” the researchers said.

“We don’t know how actively LEDA 857074 is forming stars, and therefore how frequently it will undergo supernova explosions.”

“The spotlight from this supernova made this galaxy an unexpected and lucky target for Hubble!”

“This object joins the ranks of many other well-known celestial objects thanks to its unique imaging by the Hubble Space Telescope.”

Source: www.sci.news

Observation of Spiral Galaxy NGC 3430 by Hubble

In this new image, the NASA/ESA Hubble Space Telescope focuses its lens on the center of spiral galaxy NGC 3430.



This Hubble image shows NGC 3430, a spiral galaxy about 100 million light-years away in the constellation Cygnus Minor. The color image was created from separate exposures taken with Hubble’s Advanced Camera for Surveys (ACS) in the visible and near-infrared spectral regions. The image is based on data acquired through two filters. Color is produced by assigning a different hue to each monochromatic image associated with an individual filter. Image courtesy of NASA / ESA / Hubble / C. Kilpatrick.

NGC 3430 It is located about 100 million light years away in the constellation Cygnus Minor.

Also known as IC 2613, LEDA 32614 and UGC 5982, the galaxy has a diameter of about 85,000 light-years.

NGC 3430 First discovered It was discovered on December 7, 1785 by German-born British astronomer William Herschel.

“Several other galaxies lie relatively close to this one, just outside the frame,” the Hubble astronomers said.

“One of them is close enough that gravitational interactions could drive star formation in NGC 3430.”

“NGC 3430 is such an excellent example of a galactic spiral that it may be the reason it became part of the sample Edwin Hubble used to define the classification of galaxies.”

“The NASA/ESA Hubble Space Telescope was named after him in 1926. Wrote the paper The project classifies about 400 galaxies according to their appearance: spiral, barred spiral, lenticular, elliptical, and irregular.”

“This easy-to-understand typology was highly influential, and the modern, more detailed systems used by astronomers today are still based on it.”

“NGC 3430 itself is a SAc galaxy, i.e. a spiral galaxy with no central bar and open, well-defined arms,” ​​the researchers added.

“At the time Hubble’s paper was published, the study of galaxies themselves was still in its infancy.”

“Thanks to Henrietta Levitt’s work on Cepheid variables, Hubble had only two years earlier settled the debate over whether these ‘nebulae’, as they were then called, were located within our galaxy or whether they were distant, separate stars.”

“He himself refers to an ‘extragalactic nebula’ in his paper, suggesting that it is outside the Milky Way galaxy.”

“Once it became clear that these distant objects were very different from real nebulae, the highly poetic term ‘island universe’ became popular for a time.”

“NGC 3430 may still seem worthy of this moniker, but today we refer to it and objects like it simply as a galaxy.”

Source: www.sci.news

New Hubble Space Telescope Images Reveal Classic Spiral Structure in NGC 3810

Astronomers have used the NASA/ESA Hubble Space Telescope to create a stunningly detailed image of NGC 3810, a spiral galaxy hosting a supernova.

This Hubble Space Telescope image shows NGC 3810, a spiral galaxy about 50 million light-years away in the constellation Leo. The color image is composed of infrared, visible, and ultraviolet observations from both the Hubble Space Telescope's Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) instruments. Nine filters were used to sample different wavelengths. Color is achieved by assigning a different hue to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / D. Sand / RJ Foley.

NGC 3810 It is located in the constellation Leo, about 50 million light years from Earth.

Also known as IRAS 11383+1144, LEDA 36243 and UGC 6644, the galaxy has a diameter of 60,000 light years.

NGC 3810 discovered It was discovered on March 15, 1784 by German-born British astronomer William Herschel.

The galaxy belongs to a small group of galaxies called the NGC 3810 group.

The bright central region of NGC 3810 thought Many new stars are forming and outshining the outer regions of the galaxy by a significant amount.

Even more distant galaxies show surprisingly abundant dust clouds along their spiral arms.

Far from the center, hot, young blue stars appear in huge clusters, with bright red giants scattered throughout the arms.

In 2022, a Type Ia supernova event called SN 2022zut was observed in NGC 3810.

“In early 2023, the Hubble Space Telescope will focus on this and several other galaxies to take a closer look at recent Type Ia supernovae,” Hubble astronomers said in a statement.

“These types of supernovae are produced by the explosion of a white dwarf star, and all of them maintain a very stable brightness.”

“This allows us to measure distances. We know how bright a Type Ia supernova is, so we can tell from how faint it appears how far away it is.”

“One uncertainty with this method is that intergalactic dust between Earth and the supernova will block some of the light.”

“How do we know how much of the light reduction is due to distance and how much is due to dust?”

“With the help of Hubble, we have a clever workaround: we can image the same Type Ia supernova in ultraviolet light, which is almost completely blocked by the dust, and in infrared light, which passes through the dust almost unaffected.”

“By carefully recording how much light is transmitted at each wavelength, we can calibrate the relationship between the supernova's brightness and distance, and take dust into account.”

“Hubble can observe both of these wavelengths of light in incredible detail with the same instrument.”

“That makes it the perfect tool for this experiment. In fact, some of the data used to create this beautiful image of NGC 3810 was focused on the SN 2022zut supernova, which you can see as a point of light just below the galactic nucleus.”

Source: www.sci.news

Hubble directly observes a barred spiral galaxy from a head-on perspective

This new image from the NASA/ESA Hubble Space Telescope shows the barred spiral galaxy NGC 3059 in the constellation Carina.

This Hubble Space Telescope image shows NGC 3059, a barred spiral galaxy about 57 million light-years away in the constellation Carina. Image courtesy of NASA / ESA / Hubble / D. Thilker.

NGC 3059 It is located in the constellation Carina, about 57 million light years away.

Also known as ESO 37-7, IRAS 09496-7341, and LEDA 28298, the galaxy has a diameter of 55,000 light years.

it was discovered It was discovered on February 22, 1835 by British astronomer John Herschel.

This new image of NGC 3059 shows Hubble's Wide Field Camera 3 (WFC3) is present in the ultraviolet, near infrared, and visible light portions of the spectrum.

Six 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 was collected by Hubble in May 2024 as part of an observing program studying a large number of galaxies,” Hubble astronomers explained.

“All observations were made using the same range of filters – partially transparent materials that only let certain wavelengths of light through.”

“Filters are widely used in observational astronomy and can be adjusted to let through a very narrow range of light, or a somewhat broader range of light.”

“Narrowband filters are invaluable from a scientific perspective because specific wavelengths of light are associated with specific physical and chemical processes.”

“For example, under certain conditions, hydrogen atoms are known to emit red light with a wavelength of 656.46 nm.”

“Red light of this wavelength H-alpha radiationor “H-alpha radiation.”

“Their presence is extremely useful to astronomers as they serve as indicators of certain physical processes and conditions. For example, they are often a telltale sign that a new star is forming.”

“Thus, narrow-band filters tuned to pass H-alpha radiation can be used to identify regions of the universe where stars are forming.”

For this image of NGC 3059, a narrowband filter called the F657N or H-alpha filter was used.

“F stands for filter and N stands for narrow,” the astronomers said.

“The numbers represent the peak wavelength that the filter passes. 657 is very close to the wavelength of the 656.46 H-alpha line.”

“Data collected using five other filters also contributed to the image, and they are all broadband filters, meaning they let through a wider range of wavelengths of light.”

“This isn't very useful for identifying very specific lines (such as H-alpha), but it still allows us to explore relatively unusual parts of the electromagnetic spectrum.”

“And by integrating the information from multiple filters, we're able to create beautiful images like this.”

Source: www.sci.news

Hubble Space Telescope Shines Light on Stunning Spiral Galaxy NGC 4731

The NASA/ESA Hubble Space Telescope captured this stunning image of a barred spiral galaxy called NGC 4731.

This Hubble Space Telescope image shows NGC 4731, a barred spiral galaxy about 43 million light-years away in the constellation Virgo. Image courtesy of NASA / ESA / Hubble / D. Thilker.

NGC 4731 It is located in the constellation Virgo, about 43 million light years from Earth.

Also known as IRAS 12484-0607, LEDA 43507, and UGCA 302, it is classified as a barred spiral galaxy.

“Barred spiral galaxies outnumber regular spiral and elliptical galaxies combined, making up about 60 percent of all galaxies,” the Hubble astronomers said.

“The bar-like structure we see is the result of the orbits of stars and gas in our galaxy aligning, forming dense regions where individual stars move in and out over time.”

“This is the same process that maintains the spiral arms of our galaxy, but in the case of barred galaxies it's a bit more mysterious. As spiral galaxies mature they seem to form a bar at their centre, which explains the large number of bar structures we see today. But later on the bar can also be lost if the accumulated mass along it becomes unstable.”

“The orbital patterns and gravitational interactions of galaxies support the bar-like structure of the galaxy, transporting matter and energy and promoting star formation.”

“Indeed, the observing program studying NGC 4731 seeks to investigate this flow of matter within the galaxy,” they added.

beginning discovered Discovered on April 25, 1784 by German-born British astronomer William Herschel, NGC 4731 has a diameter of about 80,000 light years.

With LEDA 43526 Galaxy, Forms Holm 472, a pair of interacting galaxies.

NGC 4731 is also a member of the NGC 4697 galaxy group. Located Near the Virgo Supercluster.

“Beyond the bar, NGC 4731's spiral arms extend far beyond the scope of this close-up Hubble image,” the astronomers said.

“The galaxy's elongated arms are thought to be the result of gravitational interactions with other nearby galaxies in the Virgo Cluster.”

The color image of NGC 4731 includes ultraviolet, near-infrared, and optical observations. Hubble's Wide Field Camera 3 (WFC3).

Six 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 richness of color reveals the galaxy's swirling gas clouds, dark dust bands, bright pink star-forming regions, and most notably, its long, luminous arms stretching out behind it,” the researchers said.

Source: www.sci.news

Stunning images of small spiral galaxies captured by Hubble

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble Photographs Stunning Barred Spiral Galaxy: NGC 3783

Astronomers using the NASA/ESA Hubble Space Telescope have taken photos of NGC 3783, a bright barred spiral galaxy in the constellation Centaurus.



This Hubble image shows NGC 3783, a barred spiral galaxy about 135 million light-years away in the constellation Centaurus. The color images consist of infrared and optical observations from Hubble’s Wide Field Camera 3 (WFC3). Based on data obtained through five filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: NASA / ESA / Hubble / MC Benz / DJV Rosario.

NGC 3783 is located about 135 million light years It is located beyond the constellation Centauri.

Also known as ESO 378-14, LEDA 36101, or 2XMM J113901.7-374418, this galaxy was first discovered It was announced by British astronomer John Herschel on April 21, 1835.

NGC 3783 is home to a rapidly rotating black hole of 2.8 million solar masses.

It is a major member of the NGC 3783 galaxy group, which is a collection of 47 galaxies.

“Like galaxy clusters, galaxy groups are gravitationally bound collections of galaxies,” the Hubble astronomers said.

“However, galaxy groups are smaller and contain fewer members than galaxy clusters. Galaxy clusters can contain hundreds or even thousands of member galaxies, whereas galaxy groups typically contain fewer than 50. It does not include galaxies that exceed

“The Milky Way is actually part of a group of galaxies known as the Local Group, which includes two other large galaxies (Andromeda and the Triangular Galaxy) and dozens of satellite galaxies. Contains dwarf galaxies.

“On the other hand, the NGC 3783 galaxy group contains 47 galaxies,” they added.

“It also appears to be at a fairly early stage in its evolution, making it an interesting subject to study.”

“Although the focus of this image is spiral galaxy NGC 3783, your eye is equally focused on a very bright object in the lower right-hand portion of this image. This is the star. HD 101274” said the researchers.

“The perspective of this image makes the stars and galaxies appear to be close companions, but this is an illusion.”

“HD 101274 is only about 1,530 light-years from Earth, which means it is about 85,000 times closer than NGC 3783.”

“This explains how a single star can appear to outshine an entire galaxy.”

According to scientists, NGC 3783 type I Seyfert galaxy — A galaxy with a bright central region.

“In this image, thanks to five separate images taken at different wavelengths of light, Hubble shows incredible detail, from the glowing central bar to the thin, winding arms and the dust that passed through them. ,” the researchers said.

“In fact, the center of the galaxy is bright enough for Hubble to exhibit diffraction spikes that are normally only seen in stars such as HD 101274.”

Source: www.sci.news

Hubble Space Telescope Captures Stunning Image of the Magellanic Spiral Galaxy

NASA has released a surprising new image of the little-known dwarf galaxy LEDA 42160 taken by the NASA/ESA Hubble Space Telescope.

This Hubble image shows dwarf galaxy LEDA 42160 located 53.5 million light-years away in the constellation Virgo. Image credit: NASA / ESA / Hubble / M. Sun.

LEDA 42160 Located approximately at 53.5 million light years It is located in the constellation Virgo, far from Earth.

Also known as MCG+02-32-161, VCC 1725, ALFALFA 3-327, or AGC 220849, this galaxy is a member of a massive galaxy cluster called the Virgo Cluster.

“LEDA 42160 is one of many astronomers to force their way through the relatively dense gas in the Virgo cluster,” Hubble astronomers said.

“The pressure exerted by this intergalactic gas, known as the Ram pressure, has a dramatic effect on star formation in LEDA 42160, which is currently being studied using Hubble.”

“LEDA 42160 falls into the following categories.” magellanic spiral galaxyIn the de Vaucouleurs galaxy classification system, it is abbreviated as Sm. ”

“Magellanic spiral galaxies can be further classified as barred galaxies (SBm), barred galaxies (SAm), and weakly barred galaxies (SABm), where the ‘bar’ refers to the elongated bar at the center of the galaxy. ”

“Generally speaking, the Magellanic Spiral Galaxy is a dwarf galaxy with only one spiral arm.”

“They are named after their prototype SBm galaxy, the Large Magellanic Cloud.”

“The Magellanic Spiral Galaxy is an interesting example of how the classification of galaxies is actually more nuanced than just spiral, elliptical, irregular, etc.”

Color images of LEDA 42160 consist of observations from. Hubble’s advanced survey camera (ACS) in the near-infrared and optical portions of the spectrum.

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

Source: www.sci.news

The Hubble Space Telescope observes a small spiral galaxy from an edge-on perspective

NASA has released a beautiful photo of spiral galaxy NGC 4423 taken by the Hubble Space Telescope.



This Hubble image shows spiral galaxy NGC 4423 about 55 million light-years away in the constellation Virgo. Image credit: NASA / ESA / Hubble / M. Sun.

NGC4423 It is located in the constellation Virgo, about 55 million light years away.

Also known as IRAS 12246+0609, LEDA 40801, or VCC 971, this spiral galaxy is approximately 35,000 light-years in diameter.

beginning spotted Discovered on April 13, 1784 by German-born British astronomer William Herschel, NGC 4423 is a member of the Virgo cluster.

“In the new image, NGC 4423 appears to have a highly irregular, tubular shape, so it may be surprising to learn that it is actually a spiral galaxy,” Hubble astronomers said in a statement.

“Knowing this, we can distinguish between the galaxy's denser central bulge and the less dense surrounding disk, which makes up the spiral arms.”

“If you looked at NGC 4423 head-on, it would resemble the shape we most associate with spiral galaxies: a spectacular curve spreading out from a bright center and interspersed with darker, dimmer, less populated regions. This is the arm you are drawing.”

“However, when observing the sky, we are constrained by the relative position of the earth and the object we are observing. We cannot simply change the position of the earth to get a better view of NGC 4423 head-on. .”

“Of course, celestial bodies are not stationary in space; they often move at very high speeds relative to each other.”

“This may suggest that even if the galaxy is moving in a coincidental direction relative to Earth, if you travel far enough you may be able to see it from a substantially different perspective. I don’t know.”

“While this is theoretically possible, in reality the distances in the universe are too long and human lifespans are too short for significant differences in relative alignment to occur.”

“In other words, this is more or less the view of NGC 4423 that we will always have.”

New images of NGC 4423 consist of observations from. Hubble's advanced survey camera (ACS) in the near-infrared and optical portions of the spectrum.

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

Source: www.sci.news

Hubble’s Discovery: Dwarf Spiral Galaxy Found in the Coma Constellation

Astronomers using the NASA/ESA Hubble Space Telescope have captured stunning images of the dwarf spiral galaxy IC 3476 in the constellation of Coma.


This Hubble image shows IC 3476, a dwarf spiral galaxy located 54 million light-years away in the constellation Coma. This image consists of observations made by Hubble's Altitude Survey Camera (ACS) in the near-infrared and optical parts of the spectrum. This is based on data obtained through his two filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / M. Sun.

IC 3476 It is located in the constellation Coma, approximately 54 million light-years from Earth.

This galaxy is first discovered It was proposed by German astronomer Arnold Schwassmann on November 22, 1900.

IC 3476, also known as IRAS 12301+1419 or LEDA 41608, is a member of the Virgo Cluster.

On the other hand, new Hubble images of the galaxy don't look quite as dramatic. The actual physical events occurring in IC 3476 are highly energetic.

“IC 3476 is undergoing a process known as ram pressure stripping, which promotes unusually high levels of star formation within the region of the galaxy itself,” the Hubble astronomers said.

“We tend to associate the letter 'ram' with the acronym RAM, which refers to random access memory in computing.”

“But ram pressure has a perfectly clear definition in physics: it is the pressure exerted on an object by the overall resistance of the fluid as it moves through some form of fluid.”

“If the entire galaxy is under ram pressure, then the galaxy is a 'celestial body', and the intergalactic medium or the intracluster medium (dust and gas that permeates the space between galaxies, in the latter case the intergalactic space) becomes a “celestial body”. fluid'. “

“Lamb pressure stripping occurs when gas is stripped from a galaxy by ram pressure,” the astronomers explained.

“Gas is absolutely key to star formation, so removing this gas could lead to reduced levels of star formation or even a complete cessation.”

“But the ram's pressure could also compress other parts of the galaxy, which could actually promote star formation.”

“This is what appears to be happening in IC 3476: no star formation appears to be occurring at the edges of the galaxy, which are bearing the brunt of the ram pressure separation, but in deeper regions of the galaxy, the rate of star formation slows down. It seems to be clearly above average. ”

Source: www.sci.news

The Potential Harmful Effects of Spiral Scratches on Contact Lenses

Contact lenses with a spiral design

Laurent Galinier

Lenses featuring a trippy spiral design could be an alternative to traditional multifocal lenses. It seems to produce clearer images than standard multifocal lenses, even in dimly lit areas.

The lens was created by the inventor Laurent Galinier.when bertrand simon He met Galinier through a scientific collaboration at the Institute of Optics Graduate School in France, and he immediately wanted to test lenses in the lab.

They are round lenses like traditional contact lenses, but the surface is carefully turned into a spiral using a lathe. This spiral shape changes the path that light rays take through the lens. That is, the lens does not have a single focal point, but several focal points, some closer to the lens and some farther from it.

It's unclear exactly how the spiral shape does this, but Simon said it appears to twist the light rays and create vortexes of light (like small tornadoes of light) that somehow influence each other. ing.

In the lab, Simon and his colleagues analyzed laser light passed through a spiral lens and simulated the process on a computer. In direct comparison with traditional multifocal lenses, the spiral lenses provided more clarity and detail when more light passed through them, and performed better in dim light conditions.

Therefore, spiral lenses may be suitable under various lighting conditions. For example, it could be useful for people who use multifocal lenses while driving at night, Simon said. He tried the spiral contact lenses himself and said that while the hard material was uncomfortable in contact with his eyes, it saved him the hassle of removing his glasses to look at his cell phone. With the spiral lens, I could see the screen clearly.

james wolfthorn According to researchers at Aston University in the UK, many people experience problems focusing on nearby objects, even if their distance vision is corrected. Innovations like spiral lenses are promising, but only clinical trials can prove how much of a difference new technology will actually make for people, he says.

Simon says it's possible to create a more compact camera by replacing part of the lens with a spiral lens version, but the team will first investigate the science behind spiral light. We would like to do further testing.

topic:

Source: www.newscientist.com

The Hubble Space Telescope captures a distorted spiral galaxy

Astronomers using the NASA/ESA Hubble Space Telescope have obtained a surprising new perspective of spiral galaxy UGC 3912.

This Hubble image shows UGC 3912, a small spiral galaxy located 63 million light-years away in the constellation Canis Major. Image credit: NASA / ESA / C. Kilpatrick, Northwestern University / Gladys Kober, NASA and The Catholic University of America.

UGC 3912also known as IRAS 07315+0439 or LEDA 21303, lies. 19.3 megaparsecs It is located in the constellation Canis Minor (63 million light years) from Earth.

“UGC 3912 is classified as a spiral galaxy, but you wouldn't know it from this detailed Hubble image,” said Hubble astronomers.

“This galaxy's distorted shape typically indicates a gravitational encounter with another galaxy.”

“When galaxies interact, meaning they bump into or collide with each other's gravitational fields, their stars, dust, and gas can be pulled into new paths.”

“UGC 3912 may have once been an organized-looking spiral, but now it appears to have been bent out of shape by a giant thumb.”

“Fortunately, when galaxies interact, individual stars and objects orbiting them remain intact, even though their orbits change dramatically and the shape of the galaxy as a whole changes.”

“That's because the distances between stars in galaxies are so great that they simply keep moving along new orbits without colliding with each other.”

Astronomers are studying UGC 3912 as part of their investigation into supernova activity. Supernova activity is when a star at least eight times the size of the Sun explodes at the end of its life.

“Hubble studies hydrogen-rich phenomena known as supernovae, one of several types of supernovae. Type II supernova” they explained.

“Although enough Type II supernovae have been observed, they exhibit highly variable properties in brightness and spectroscopy and are not well understood.”

Source: www.sci.news

The Hubble Space Telescope Observes Stunning Spiral Galaxies

The Hubble team has released a stunning photo of the face-on spiral galaxy ESO 420-13 taken by the NASA/ESA Hubble Space Telescope.



This Hubble image shows spiral galaxy ESO 420-13 facing forward. Image credit: NASA / ESA / University of Virginia A. Evans / Gladys Kober, NASA and The Catholic University of America.

ESO420-13 It is a spiral galaxy located south of the constellation Eridanus.

This galaxy, also known as LEDA 14702, IRAS 04118-3207, or 2MASX J04134969-3200252, Seyfert Galaxy.

“Dark dust lanes are visible against the backdrop of the glow of the galaxy's many stars,” Hubble astronomers said in a statement.

“About 10% of all galaxies in the universe are thought to be Seyfert galaxies.”

“They are typically spiral galaxies and have very bright nuclei, the result of a supermassive black hole at their center accreting large amounts of radiation-emitting material.”

“The centers of these active galaxies are the brightest when observed with light outside the visible spectrum.”

“Galaxies containing active galactic nuclei of this type are often so bright that the glow of the nucleus washes out the host galaxy itself.”

“But the Seyfert galaxy is unique because the galaxy itself is also visible.”

“In the case of ESO 420-13, we can enjoy the galaxy's almost perfectly round disk, brighter core, and swirling dark dust filaments.”

Astronomers observed ESO 420-13 as part of their research. bright infrared galaxy (LIRG).

“These galaxies are known to be very bright in the infrared part of the spectrum,” the researchers said.

“Galaxy interactions trigger new star-forming regions in LIRG that become extremely bright in infrared light.”

Source: www.sci.news