Stunning Close-Up of Arp 4 Captured by Hubble Space Telescope

Discover the latest stunning image captured by the NASA/ESA Hubble Space Telescope, showcasing Arp 4, an intriguing visual pair of galaxies located in the constellation Cetus.



The Hubble image captures the galaxy pair Arp 4. Image credits: NASA / ESA / Hubble / J. Dalcanton, Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA.

For more details, explore Arp 4, which features the bright spiral galaxy MCG-02-05-050a alongside the larger spiral galaxy MCG-02-05-050.

Located within the constellation Cetus, this galaxy pair was first discovered by Dutch-Canadian astronomer Sidney van den Bergh in 1959.

Arp 4 stands as the fourth entry in Halton Arp’s Atlas of Peculiar Galaxies and belongs to the section focusing on “Galaxies with Low Surface Brightness.”

“The term ‘Arp 4’ derives from the Atlas of Peculiar Galaxies compiled by astronomer Halton Arp during the 1960s,” Hubble astronomers explained.

“These ‘unusual galaxies’ were chosen for photography to illustrate their distinct and non-standard shapes, providing insights into galaxy evolution.”

Hubble’s mission has transformed our understanding of galaxies, revealing captivating examples from Arp’s Atlas, including Arp 4.

The initial galaxies in this catalog, including Arp 4, exhibit low surface brightness, rendering them faint and challenging to observe.

“The larger galaxy, cataloged as MCG-02-05-050, features fragmented arms and a dim disk, perfectly fitting this description,” the astronomers noted.

“In contrast, its smaller counterpart, MCG-02-05-050a, is considerably brighter and more dynamic as a spiral galaxy.”

“Crucially, these galaxies are not in close proximity,” the researchers emphasized.

“The prominent blue galaxy, MCG-02-05-050, lies 65 million light-years from Earth.”

“Meanwhile, the brighter, smaller galaxy MCG-02-05-050a is positioned at an impressive 675 million light-years, over ten times farther away.”

This positioning likely suggests that MCG-02-05-050a is the more substantial of the two, while MCG-02-05-050 is relatively smaller.

“This visual pairing is simply an unlikely coincidence,” the astronomers added.

“Despite the absence of a physical connection, we can enjoy the unique sight of Arp 4 as an enthralling duo adorning our night sky.”

Source: www.sci.news

ARP 105: Hubble Captures Ongoing Merger of Two Massive Galaxies

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

New Images of Arp 142 Captured by Webb Show Stunning Detail

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have captured new infrared images of two interacting galaxies. Alp 142.



This Webb image shows two interacting galaxies known as Arp 142. On the left is NGC 2937, nicknamed “The Egg” because of its appearance, and on the right is NGC 2936, nicknamed “The Penguin” because of its appearance. Image courtesy of NASA/ESA/CSA/Webb/STScI.

The interacting pair, Arp 142, is located about 326 million light-years away in the southern constellation Hydra.

This system is ARP Catalog of Peculiar Galaxies It was observed by astronomer Halton C. Earp in the 1960s.

It contains the star-forming spiral galaxy NGC 2936 and its elliptical companion galaxy NGC 2937 at the lower left, which bears a striking resemblance to a penguin guarding its eggs.

The “penguin” part of the pair, NGC 2936, was probably once a relatively ordinary-looking spiral galaxy – flat like a pancake, with smoothly symmetrical spiral arms.

Because of the abundance of newly formed, hot stars, its shape is twisted and distorted by the gravitational forces of nearby stars.

The twin “egg,” NGC 2937, is a collection of much older stars and, in contrast, is largely featureless.

The absence of glowing red dust features indicates that it long ago lost its reservoir of gas and dust from which new stars could form.

“The two asteroids first came close to each other between 25 million and 75 million years ago, triggering 'fireworks' – the formation of new stars – in the constellation of Penguin,” astronomer Webb said in a statement.

“In the most extreme cases, galaxy mergers could result in the formation of thousands of new stars every year for millions of years.”

“In the case of penguins, studies have found that they form around 100-200 stars per year. By comparison, in our own Milky Way galaxy (which is not interacting with a galaxy of a similar size), around six to seven new stars form per year.”

“This gravitational rocking also changed the penguins' appearance,” they noted.

“The spiral arms uncoiled, pulling gas and dust in different directions like confetti.”

“When galaxies interact, it's rare for individual stars to collide (the universe is huge), but the intermingling of galaxies disrupts the orbits of stars.”

“Currently, the centre of the Penguin's galaxy looks like an eye inside its head, and the galaxy has a prominent star trail in the shape of a beak, spine and fanned-out tail. A faint but noticeable dust ribbon stretches from the beak to the tail.”

“Although the Penguin Galaxy appears much larger than the Egg Galaxy, the two galaxies have roughly the same mass,” the astronomers said.

“This is one of the reasons why the tiny looking egg hasn't merged with the penguin yet.”

“Because the elliptical egg is filled with old stars and contains very little gas or dust, it doesn't emit its own 'streams' or tidal tails, and instead maintains its compact elliptical shape.”

“If you look closely, the Egg has four noticeable diffraction spikes – it's glowing because of a high concentration of stars from the galaxy.”

“Now, find the bright, edge-on galaxy in the upper right. It may look like it's crashing the party, but it’s not close by.”

Cataloging No. 1237172It lies nearly 100 million light-years from Earth. It is relatively young and not covered by dust, making it virtually invisible in Webb's mid-infrared images.”

Source: www.sci.news

Close-up of Arp 140 captured by Hubble Space Telescope

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Hubble captures the stunning collision of two spiral galaxies in Arp 122

This cosmic encounter is known as Arp 122, and here: NASA/ESA Hubble Space Telescope.


Two spiral galaxies, NGC 6040 and NGC 6039, have merged on the right side of this Hubble image. NGC 6039 is circular when viewed from the front. NGC 6040 appears to be before the first one. In the lower left corner of the frame, elliptical galaxy NGC 6041, the central member of the galaxy cluster in which Arp 122 resides, is visible as light emanating from a point. This color image was created in both the visible and infrared regions of the spectrum using Hubble's Altitude Survey Camera (ACS) and the Dark Energy Camera mounted on NSF's Victor M. Blanco 4-meter Telescope at Cerro Tololo Inter. Created from separate exposures taken in the area. -American Observatory of Chile. Four filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: NASA / ESA / Hubble / J. Dalcanton / Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA / L. Shatz.

Alp 122 It is located in the constellation Hercules, approximately 570 million light years from Earth.

This system consists of two galaxies: a tilted and distorted spiral galaxy; NGC6040 and the spiral galaxy in front of me NGC6039.

“Galaxy collisions and mergers are highly energetic and dramatic events, but they occur on very slow timescales,” Hubble astronomers said in a statement.

“For example, our Milky Way galaxy is on a colliding orbit with its nearest galactic neighbor, the Andromeda galaxy, but it will still be four billion years before these two galaxies actually meet. ”

“The process of collision and fusion will not end soon either; it may take hundreds of millions of years to unfold.”

“These collisions take a very long time because they have very long distances.”

“Galaxies are composed of stars and their solar systems, dust and gas,” the researchers added.

“Over time, the structures of two (or more) colliding galaxies may change completely, eventually forming a single, merged galaxy.”

“That could be the result of the collision seen in this image.”

“Galaxies resulting from mergers are thought to have regular or elliptical structures because the merger process destroys more complex structures (such as those observed in spiral galaxies).”

“It will be interesting to see what Arp 122 will look like once this collision is complete, but that won't happen for a long time.”

Source: www.sci.news