NGC 5042 Under Observation by Hubble Space Telescope

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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

After days of observation, scientists confirm a 650-foot-high tsunami formed in Greenland.

summary

  • Seismologists detected unusual vibrations and determined that a 650-foot-high tsunami had occurred in Greenland.
  • The tsunami was caused by melting glacial ice that triggered landslides and washed away water in Greenland's fjords.
  • The waves it created continued to travel back and forth across the fjord for nine days.

Last September, seismologists around the world detected vibrations never before observed.

The monotony seemed to come from Greenland and continued for nine days.

“We saw some very strange signals at some stations in the north that we'd never seen before,” said Karl Ebeling, a seismologist at the Scripps Institution of Oceanography at the University of California, San Diego.

Shortly after the vibrations began, a cruise ship sailing near a Greenland fjord noticed that a key landmark on the remote island of Ella, a scientific research and Danish military dog ​​sled patrol base, had been destroyed.

The event drew an international group of seismologists, the Danish military and oceanographers into the mystery: what struck the island, and where did it come from?

On Thursday, the researchers They published their findings in the journal Science.The island was hit by one of the largest tsunamis on record, leaving a scar about 650 feet high.

It was the result of a rare series of cascading events caused by climate change.

The researchers traced the initial trigger to the collapse of a glacier tongue that had been thinned by rising temperatures. This destabilized the steep mountainside, sending an avalanche of rock and ice into Greenland's deep Dikson Fjord. Massive amounts of water were displaced, causing towering waves to move across the narrow fjord, about a mile and a half wide.

The tsunami, at least as high as the Statue of Liberty, surged up the steep rock faces along the fjord and, because the landslide struck the waterway at a nearly 90-degree angle, sent waves circling the channel for nine days — a phenomenon scientists call a seiche.

“No one has ever seen anything like this,” said Christian Svennevig, lead author of the study and a geologist and senior research scientist at the Geological Survey of Denmark and Greenland.

The findings are the result of a complex year-long investigation. The team determined that Ella Island, about 45 miles from the landslide site, was hit by a tsunami at least 13 feet high.

Tourists visit the island from time to time.

“The cruise ship had been docked off the coast just a few days before,” Svennevig said. “We were really lucky that no one was there when it happened.”

The seiche was the longest scientists had ever observed: Until now, tsunamis generated by landslides have typically produced waves that dissipate within a few hours.

“This is really a cascade of events that has never been observed before,” said Alice Gabriel, co-author of the study. “The Earth is a very dynamic system, and we're currently at a stage where this very delicate balance is being disrupted pretty dramatically by climate change.”

Tsunamis triggered by landslides occur more frequently than many people realize and are a danger to people living and working in some Arctic and sub-Arctic regions.

In 2017, a landslide triggered a tsunami that killed four people and destroyed 11 homes. Attacked the village of Ngaatsiaq in West GreenlandThe tsunami was estimated to be at least 300 feet high. Two villages were abandoned in the aftermath of the tsunami due to fears of further landslides, and Svennevig said hundreds of people remain evacuated.

Bretwood “Higg” Higman, an Alaska geologist who studies landslide tsunamis but was not involved in the new study, said evidence suggests landslide tsunamis are a growing problem, but more research is needed.

“I'm pretty confident that these events are becoming more and more frequent,” he said. “Exactly how frequent these events are and can we predict the future? We're not there yet.”

Higman said he thought the Greenland study's researchers were “spot on” and that the research was an important example of how dangerous landslide-induced tsunamis could be.

The Arctic and sub-Arctic regions are warming two to three times faster than the rest of the Earth. As the ice melts, the exposed, dark surface absorbs more sunlight. Warming is triggering three dynamics that could make landslides more frequent in glacial regions, Higman said.

First, rising temperatures are eroding the permafrost within rock formations, weakening slopes and making them more susceptible to collapse. Second, warming is thinning the glaciers that support the rock slopes. Without the ice, sudden collapses could occur. Third, climate change is increasing the likelihood of heavy rains, which are the biggest risk factor for landslides because saturated rocks and soils become more slippery.

Higman has compiled a list of Alaska's slopes that are at risk for landslides that could trigger tsunamis. He said there are dozens of sites of concern that need further study, some of which are near populated areas where a landslide could be catastrophic.

“We're in an awkward position: Scientists know something, but they don't know enough to provide certainty to take action,” Higman said.

Last month, the U.S. Geological Survey reported a 56-foot-high landslide tsunami in Alaska's Pedersen Lagoon. Higman visited the site and believes the tsunami was larger than initially predicted.

Globally, risks are growing due to expanding development in some polar regions and increased visitation by miners, shippers and tourists, Svennevig said.

“At the same time as the population increases, the risk of landslides, geological hazards also increases,” he said. “It's an unfortunate combination.”

Source: www.nbcnews.com

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

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



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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Observation by Hubble of the central region of the Trigonum Galaxy

Astronomers have used the NASA/ESA Hubble Space Telescope to capture a detailed image of the spectacular centre of the Triangulum Galaxy.



The Triangulum Galaxy is the third largest galaxy in our galaxy group. Image credit: NASA/ESA/M. Boyer, STScI/J. Dalcanton, University of Washington/Gladys Kober, NASA and The Catholic University of America.

The Triangulum Galaxy, also known as Messier 33, M33, and NGC 598, is a spiral galaxy located about 3 million light-years away.

Under very dark sky conditions, the galaxy can be seen with the naked eye as a faint, fuzzy object in the constellation Triangulum, and its ethereal glow makes it a fascination for amateur astronomers.

The galaxy is a notable member of the Local Group, a collection of more than 50 galaxies bound together by gravity. It is the third largest galaxy in the Local Group, but it is also the smallest spiral galaxy in the group.

The Triangulum Galaxy is only about 60,000 light years in diameter, and the Andromeda Galaxy is 200,000 light years in diameter. The Milky Way Galaxy is about 100,000 light years in diameter, placing it halfway between these two extremes.

“The Triangulum Galaxy is a known hotbed of star birth, forming stars at an average rate ten times higher than in the neighboring Andromeda Galaxy,” Hubble astronomers said in a statement.

“Interestingly, its well-ordered spiral arms indicate that it has few interactions with other galaxies, so galactic collisions are not driving rapid star formation as they do in many other galaxies.”

“The galaxy has an abundance of dust and gas to produce stars, and it also has many clouds of ionized hydrogen, also known as HII regions, that give rise to phenomenal star formation.”

“Researchers present evidence that high-mass stars form in collisions between giant molecular clouds in the Triangulum Galaxy.”

This new image from the Hubble Space Telescope shows a reddish cloud of ionized hydrogen dotted with dark dust bands that make the image look grainy but are actually a swarm of stars.

“The Triangulum Galaxy is one of fewer than 100 galaxies close enough that a telescope like Hubble can resolve individual stars, as revealed here,” the astronomers write.

“It is known that this galaxy does not have a central bulge, and there is no evidence of a supermassive black hole at its center. This is odd, given that most spiral galaxies have a central bulge made of densely packed stars, and most large galaxies have supermassive black holes at their centers.”

“Galaxies with this type of structure are called pure disk galaxies, and studies suggest that they make up about 15-18 percent of galaxies in the universe.”

“The Triangulum Galaxy could lose its streamlined appearance and peaceful state in a dramatic way, potentially colliding with both the Andromeda and Milky Way galaxies.”

“The image was taken as part of an investigation of the Triangulum Galaxy to refine theories on topics such as the physics of the interstellar medium, star formation processes and stellar evolution.”

Source: www.sci.news

Physicists Witness the First Observation of Antihyperhydrogen 4

Physicists from the STAR Collaboration have observed an antimatter hypernucleus, antihyperhydrogen-4, consisting of an antihypernucleus, an antiproton, and two antineutrons, in nuclear collisions at the Relativistic Heavy Ion Collider (RHIC) at the U.S. Department of Energy's Brookhaven National Laboratory.

Artistic representation of antihyperhydrogen-4 produced in the collision of two gold nuclei. Image courtesy of the Institute of Modern Physics.

“What we know in physics about matter and antimatter is that, apart from the opposite charge, antimatter has the same properties as matter – the same mass, the same lifetime before decaying, and the same interactions,” said Junlin Wu, a graduate student at Lanzhou University and the China Institute of Modern Physics.

“But in reality, our universe is made up of antimatter rather than matter, even though equal amounts of matter and antimatter are thought to have been created during the Big Bang about 14 billion years ago.”

“Why our universe is populated with matter remains a question, and we don't yet have a complete answer.”

“The first step in studying the asymmetry between matter and antimatter is to discover new antimatter particles. This is the basic idea of ​​this research,” added Dr Hao Qiu, a researcher at the Institute of Modern Physics.

STAR physicists had previously observed atomic nuclei made of antimatter produced in RHIC collisions.

In 2010, they detected an antihypertriton, the first example of an antimatter nucleus containing a hyperon, a particle that contains at least one strange quark rather than just the light up and down quarks that make up ordinary protons and neutrons.

Just a year later, STAR physicists broke that massive antimatter record by detecting antihelium-4, the antimatter equivalent of a helium nucleus.

Recent analysis suggests that antihyperhydrogen 4 may also be feasible.

But detecting this unstable antihypernucleus is a rare event: all four components (one antiproton, two antineutrons and one antilambda) need to be ejected from the quark-gluon soup produced in the RHIC collision in just the right place, in the same direction and at just the right time, briefly becoming bound together.

“It's just a coincidence that these four component particles appear close enough together in the RHIC collision that they can combine to form an antihypernucleus,” said Brookhaven National Laboratory physicist Lijuan Luan, one of the STAR collaboration's co-spokespeople.

To find antihyperhydrogen-4, STAR physicists studied the trajectories of particles produced when this unstable antihypernucleus decays.

One of these decay products is the previously detected antihelium-4 nucleus, and the other is a simple positively charged particle called a pion (pi+).

“Antihelium-4 had already been discovered with STAR, so we used the same methods as before to pick up those events and reconstruct them with the π+ track to find these particles,” Wu said.

“It is simply by chance that these four component particles emerge from the RHIC collision close enough together to combine to form an antihypernucleus,” said Dr. Lijuan Luan, a research scientist at Brookhaven National Laboratory.

RHIC's collisions produce huge amounts of pions, and physicists have been sifting through billions of collision events to find the rare antihypernuclei.

The antihelium-4 produced by the collision can pair up with hundreds or even a thousand pi+ particles.

“The key was to find an intersection point where the trajectories of the two particles had a particular characteristic – a collapse vertex,” Dr. Luan said.

“That is, the collapse apex must be far enough away from the collision point that the two particles could have originated from the decay of an antihypernucleus that formed shortly after the collision of the particle originally produced in the fireball.”

STAR researchers worked hard to eliminate the background of all other potential collapse pair partners.

Ultimately, their analysis found 22 candidate events with an estimated background count of 6.4.

“That means that about six of what appear to be antihyperhydrogen-4 decays could just be random noise,” said Emily Duckworth, a doctoral student at Kent State University.

Subtracting that background count from the 22, physicists can be confident that they have detected about 16 actual antihyperhydrogen-4 nuclei.

The results were significant enough to allow scientists to make a direct comparison between matter and antimatter.

They compared the lifespan of antihyperhydrogen 4 to that of hyperhydrogen 4, which is made from normal matter variants of the same building blocks.

They also compared the lifetimes of another matter-antimatter pair, antihypertritons and hypertritons.

Neither difference was significant, but the authors were not surprised.

“This experiment tested a particularly strong form of symmetry,” the researchers said.

“Physicists generally agree that this symmetry breaking is extremely rare and is not an answer to the imbalance of matter and antimatter in the universe.”

“If we saw this particular breaking of symmetry, we would basically have to throw a lot of what we know about physics out the window,” Duckworth said.

“So in a way it was reassuring that symmetry still worked in this case.”

“We agree that this result provides further confirmation that our model is correct and marks a major step forward in the experimental study of antimatter.”

Team work Published in a journal Nature.

_____

STAR Collaboration. Observation of the antimatter hypernucleus antihyperhydrogen 4. NaturePublished online August 21, 2024, doi: 10.1038/s41586-024-07823-0

This article is based on an original release from Brookhaven National Laboratory.

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

Webb’s Observation of a Massive Star-Forming Complex in the Large Magellanic Cloud

Use of Mid-infrared measuring instrument With (MIRI) aboard the NASA/ESA/CSA James Webb Space Telescope, astronomers have captured stunning images of N79, a region of interstellar ionized hydrogen in the Large Magellanic Cloud.

This Hubble image shows star-forming region N79 located 163,000 light-years away in the constellation Sera. Image credit: NASA / ESA / CSA / Webb / M. Meixner.

N79 is a massive star-forming complex spanning about 1,630 light-years in the generally unexplored southwestern region of the Large Magellanic Cloud, a neighboring dwarf galaxy about 163,000 light-years from us.

This region is usually considered a younger version of the 30 Doradus, also known as the Tarantula Nebula.

N79 has a star formation efficiency more than twice that of Doradas 30 over the past 500,000 years.

This particular image centers on one of three giant molecular cloud complexes called N79 South (S1 for short).

The distinctive “starburst” pattern surrounding this bright object is a series of diffraction spikes.

“All telescopes that use mirrors to collect light, like Webb, have this form of artifact resulting from the design of the telescope,” Webb astronomers said.

“For Webb, the six largest starburst spikes appear due to the hexagonal symmetry of Webb's 18 primary mirror segments.”

“Such patterns are only noticeable around very bright and compact objects, where all the light comes from the same place.”

“Most galaxies appear very small to our eyes, but we don't see this pattern because they are dimmer and more spread out than a single star.”

“At the longer wavelengths of light captured by MIRI, Webb's view of N79 shows glowing gas and dust in the region.”

“This is because mid-infrared light can reveal what's going on deep within the cloud (whereas shorter wavelength light is absorbed or scattered by dust particles within the nebula). Still embedded Some protostars also appear in this region.”

Star-forming regions such as N79 are of interest to astronomers because their chemical composition is similar to that of giant star-forming regions observed in the early universe.

“The star-forming regions of our Milky Way galaxy are not producing stars at the same ferocious rate as N79 and have a different chemical composition,” the astronomers said.

“Webb now offers us the opportunity to compare and contrast observations of star formation in N79 with deep telescopic observations of distant galaxies in the early universe.”

“These observations of N79 are part of the Webb program to study the evolution of circumstellar disks and envelopes of forming stars over a wide range of masses and at different evolutionary stages.”

“Webb's sensitivity allows us to detect for the first time disks of planet-forming dust around stars of the same mass as the Sun at distances in the Large Magellanic Cloud.”

Source: www.sci.news