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Interacting galaxies are more than they seem, JWST shows

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It was only two years ago that JWST’s first science images were released.

This view showcases the difference between the JWST’s NIRCam and MIRI views, with NIRCam’s being far sharper and revealing more objects. The MIRI view reveals dusty details that no other wavelength can, however, including the abundance and composition of dust inside, which relates to a galaxy’s star-forming and life-forming potentials. In the MIRI view, red = gas-rich; blue = gas-poor (but still present); green = organic molecules, especially polycyclic aromatic hydrocarbons.

Credit: NASA, ESA, CSA, and STScI

They combined high resolution with unprecedented sensitivity in infrared light.

Overlaid with (older) Hubble data, the JWST NIRCam image of the Southern Ring Nebula is clearly superior in a variety of ways: resolution, the details revealed, the extent of the outer gas, etc. It truly is a spectacular reveal of how stars like the Sun end their lives, as well as how, very slightly, the nebula has expanded in between the acquisition of the Hubble and JWST images.

Credit: NASA, ESA, CSA, and STScI

Many surprises abounded early on.

This image is the first mid-infrared image of Stephan’s Quintet ever taken by the James Webb Space Telescope. The galaxy at the topmost-right of the image displays a brilliant spiky pattern: evidence of a supermassive black hole that had never been revealed prior.

Credit: NASA, ESA, CSA, STScI

New features within planetary systems were discovered.

This image of the dusty debris disk surrounding the young star Fomalhaut is from Webb’s Mid-Infrared Instrument (MIRI). It reveals three nested belts extending out to 14 billion miles (23 billion kilometers) from the star. The inner belts – which had never been seen before – were revealed by Webb for the first time. Labels at left indicate the individual features. At right, a great dust cloud is highlighted and pullouts show it in two infrared wavelengths: 23 and 25.5 microns.

Credit: NASA, ESA, CSA; Processing: A. Gáspár (University of Arizona) &Alyssa Pagan (STScI)

Distance records were shattered, both for individual galaxies,

JADES-GS-z14-0, in the top inset box, is found behind (and just to the right of) a closer, brighter, bluer galaxy. It was only through the power of spectroscopy with incredible resolution, capable of separating the two sources, that the nature of this record-breakingly distant object could be determined. Its light comes to us from when the Universe was only 290 million years old: just 2.1% of its current age.

Credit: S. Carniani et al. (JADES collaboration), arXiv:2405.18485, 2024

as well as the earliest galaxy clusters.

The galaxies that are members of the identified proto-cluster A2744z7p9OD are shown here, outlined atop their positions in the JWST view of galaxy cluster Abell 2744. At just 650 million years after the Big Bang, it’s the oldest proto-cluster of galaxies ever identified. This is early, but is consistent with simulations of when the earliest proto-clusters should emerge from the most initially overdense regions.

Credit: NASA, ESA, CSA, Takahiro Morishita (IPAC); Processing: Alyssa Pagan (STScI)

But spectacular features also emerged within interacting galaxies.

The stellar streams being ripped from one of the interacting member galaxies of Stephan’s Quintet glitters in this image, while background galaxies shine from much farther away. The new stars that form may not remain gravitationally bound and undisturbed for long, but for as long as they persist, will form collections of stars (or galaxies) that have no dark matter within them at all.

Credit: NASA, ESA, CSA, and STScI

With near-infrared NIRCam and mid-infrared MIRI views, optically invisible features shone brilliantly.

The pair of interacting galaxies in the process of a merger, known as IC 1623, is imaged here by JWST. Data from a trio of JWST’s instruments, MIRI, NIRSpec, and NIRCam, were used in the construction of this image. The ongoing starburst at the center produces intense infrared emissions.

Credit: ESA/Webb, NASA & CSA, L. Armus & A. Evans; Acknowledgement: R. Colombari

Previously, the galactic pair Arp 142 — the Penguin and the Egg — was viewed by Hubble.

This interacting pair of galaxies, cataloged as Arp 142, was dubbed “the Penguin and the Egg” after the Hubble Space Telescope revealed this view of the two member galaxies: the extended NGC 2936 and the compact NGC 2937.

Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA)

To celebrate its second anniversary, JWST released a NIRCam image,

This NIRCam view of the Penguin and the Egg displays a smoke-like appearance, while the “eye” of the Penguin shines brilliantly: corresponding to the center of what was, up until perhaps 75 million years ago, just a normal-appearing spiral galaxy. The gravitational encounter with the “Egg” galaxy has distorted and distended the less massive spiral galaxy into the shape now seen here.

Credit: NASA, ESA, CSA, STScI

a MIRI image,

In mid-infrared light, the Penguin looks more like a seahorse, with cool dust dominating the galaxy’s appearance, while the Egg appears smaller and more compact: illuminated largely by the cooler, older stars present within it. At much longer wavelengths than the NIRCam image, MIRI’s resolution is much lower, but still reveals spectacularly sharp features.

Credit: NASA, ESA, CSA, STScI

and also a composite image of this galactic encounter, occurring 326 million light-years away.

In this composite image, NIRCam and MIRI data are combined together to produce this image, which is more detail-rich than either the NIRCam or MIRI images on their own. While both MIRI and NIRCam features are clearly present throughout the Penguin, only the central core of the Egg has a MIRI contribution.

Credit: NASA, ESA, CSA, STScI

The larger galaxy, the Penguin, exhibits severely extended features: knotted gas, which triggers new star-forming episodes.

This three-panel animation shows Hubble (visible light), NIRCam (near-infrared light), and NIRCam+MIRI composite (all JWST light) images superimposed atop one another, highlighting the various features present within the Penguin component of Arp 142.

Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); NASA, ESA, CSA, STScI; Processing: E. Siegel

The Egg, meanwhile, is relatively undisturbed: a more massive, compact elliptical galaxy, with very little gas remaining.

This three-panel animation shows Hubble (visible light), NIRCam (near-infrared light), and NIRCam+MIRI composite (all JWST light) images superimposed atop one another, highlighting the various features present within the Egg component of Arp 142. Note how only background galaxies and the absolute center of the Egg are impacted by MIRI’s imagery.

Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); NASA, ESA, CSA, STScI; Processing: E. Siegel

Nearby, the edge-on galaxy PGC 1237172 lies 100 million light-years closer: dust-poor and nearly invisible to MIRI.

This three-panel animation shows Hubble (visible light), NIRCam (near-infrared light), and NIRCam+MIRI composite (all JWST light) images superimposed atop one another, highlighting the various features present within the edge-on galaxy PGC 1237172. The galaxy itself is nearly invisible to MIRI’s eyes.

Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); NASA, ESA, CSA, STScI; Processing: E. Siegel

The Penguin, once a spiral, stretches out into a seahorse-like appearance in infrared light.

These three views show the visible light (left), near-infrared (middle), and mid-infrared (right) views of the Penguin galaxy that’s part of Arp 142. The galaxy takes on a seahorse-like appearance in mid-infrared light, as polycyclic aromatic hydrocarbons, old, cool stars, and cold dust are highlighted.

Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); NASA, ESA, CSA, STScI; Composition: E. Siegel

The smoke-like appearance reveals polycyclic aromatic hydrocarbons: complex organic molecules that may be life’s precursors.

This annotated composite view from JWST shows both NIRCam and MIRI data together, highlighting the longer-wavelength features in redder colors and the shorter-wavelength ones in bluer colors. The Penguin, in particular, exhibits a great diversity of gaseous and stellar features, showcasing just how severely it is being disrupted by this gravitational encounter.

Credit: NASA, ESA, CSA, STScI

Eventually, and ironically, the Egg will subsume the Penguin.

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Mostly Mute Monday tells an astronomical story in images, visuals, and no more than 200 words.

 

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Here’s how Helene and other storms dumped a whopping 40 trillion gallons of rain on the South

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More than 40 trillion gallons of rain drenched the Southeast United States in the last week from Hurricane Helene and a run-of-the-mill rainstorm that sloshed in ahead of it — an unheard of amount of water that has stunned experts.

That’s enough to fill the Dallas Cowboys’ stadium 51,000 times, or Lake Tahoe just once. If it was concentrated just on the state of North Carolina that much water would be 3.5 feet deep (more than 1 meter). It’s enough to fill more than 60 million Olympic-size swimming pools.

“That’s an astronomical amount of precipitation,” said Ed Clark, head of the National Oceanic and Atmospheric Administration’s National Water Center in Tuscaloosa, Alabama. “I have not seen something in my 25 years of working at the weather service that is this geographically large of an extent and the sheer volume of water that fell from the sky.”

The flood damage from the rain is apocalyptic, meteorologists said. More than 100 people are dead, according to officials.

Private meteorologist Ryan Maue, a former NOAA chief scientist, calculated the amount of rain, using precipitation measurements made in 2.5-mile-by-2.5 mile grids as measured by satellites and ground observations. He came up with 40 trillion gallons through Sunday for the eastern United States, with 20 trillion gallons of that hitting just Georgia, Tennessee, the Carolinas and Florida from Hurricane Helene.

Clark did the calculations independently and said the 40 trillion gallon figure (151 trillion liters) is about right and, if anything, conservative. Maue said maybe 1 to 2 trillion more gallons of rain had fallen, much if it in Virginia, since his calculations.

Clark, who spends much of his work on issues of shrinking western water supplies, said to put the amount of rain in perspective, it’s more than twice the combined amount of water stored by two key Colorado River basin reservoirs: Lake Powell and Lake Mead.

Several meteorologists said this was a combination of two, maybe three storm systems. Before Helene struck, rain had fallen heavily for days because a low pressure system had “cut off” from the jet stream — which moves weather systems along west to east — and stalled over the Southeast. That funneled plenty of warm water from the Gulf of Mexico. And a storm that fell just short of named status parked along North Carolina’s Atlantic coast, dumping as much as 20 inches of rain, said North Carolina state climatologist Kathie Dello.

Then add Helene, one of the largest storms in the last couple decades and one that held plenty of rain because it was young and moved fast before it hit the Appalachians, said University of Albany hurricane expert Kristen Corbosiero.

“It was not just a perfect storm, but it was a combination of multiple storms that that led to the enormous amount of rain,” Maue said. “That collected at high elevation, we’re talking 3,000 to 6000 feet. And when you drop trillions of gallons on a mountain, that has to go down.”

The fact that these storms hit the mountains made everything worse, and not just because of runoff. The interaction between the mountains and the storm systems wrings more moisture out of the air, Clark, Maue and Corbosiero said.

North Carolina weather officials said their top measurement total was 31.33 inches in the tiny town of Busick. Mount Mitchell also got more than 2 feet of rainfall.

Before 2017’s Hurricane Harvey, “I said to our colleagues, you know, I never thought in my career that we would measure rainfall in feet,” Clark said. “And after Harvey, Florence, the more isolated events in eastern Kentucky, portions of South Dakota. We’re seeing events year in and year out where we are measuring rainfall in feet.”

Storms are getting wetter as the climate change s, said Corbosiero and Dello. A basic law of physics says the air holds nearly 4% more moisture for every degree Fahrenheit warmer (7% for every degree Celsius) and the world has warmed more than 2 degrees (1.2 degrees Celsius) since pre-industrial times.

Corbosiero said meteorologists are vigorously debating how much of Helene is due to worsening climate change and how much is random.

For Dello, the “fingerprints of climate change” were clear.

“We’ve seen tropical storm impacts in western North Carolina. But these storms are wetter and these storms are warmer. And there would have been a time when a tropical storm would have been heading toward North Carolina and would have caused some rain and some damage, but not apocalyptic destruction. ”

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‘Big Sam’: Paleontologists unearth giant skull of Pachyrhinosaurus in Alberta

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It’s a dinosaur that roamed Alberta’s badlands more than 70 million years ago, sporting a big, bumpy, bony head the size of a baby elephant.

On Wednesday, paleontologists near Grande Prairie pulled its 272-kilogram skull from the ground.

They call it “Big Sam.”

The adult Pachyrhinosaurus is the second plant-eating dinosaur to be unearthed from a dense bonebed belonging to a herd that died together on the edge of a valley that now sits 450 kilometres northwest of Edmonton.

It didn’t die alone.

“We have hundreds of juvenile bones in the bonebed, so we know that there are many babies and some adults among all of the big adults,” Emily Bamforth, a paleontologist with the nearby Philip J. Currie Dinosaur Museum, said in an interview on the way to the dig site.

She described the horned Pachyrhinosaurus as “the smaller, older cousin of the triceratops.”

“This species of dinosaur is endemic to the Grand Prairie area, so it’s found here and nowhere else in the world. They are … kind of about the size of an Indian elephant and a rhino,” she added.

The head alone, she said, is about the size of a baby elephant.

The discovery was a long time coming.

The bonebed was first discovered by a high school teacher out for a walk about 50 years ago. It took the teacher a decade to get anyone from southern Alberta to come to take a look.

“At the time, sort of in the ’70s and ’80s, paleontology in northern Alberta was virtually unknown,” said Bamforth.

When paleontogists eventually got to the site, Bamforth said, they learned “it’s actually one of the densest dinosaur bonebeds in North America.”

“It contains about 100 to 300 bones per square metre,” she said.

Paleontologists have been at the site sporadically ever since, combing through bones belonging to turtles, dinosaurs and lizards. Sixteen years ago, they discovered a large skull of an approximately 30-year-old Pachyrhinosaurus, which is now at the museum.

About a year ago, they found the second adult: Big Sam.

Bamforth said both dinosaurs are believed to have been the elders in the herd.

“Their distinguishing feature is that, instead of having a horn on their nose like a triceratops, they had this big, bony bump called a boss. And they have big, bony bumps over their eyes as well,” she said.

“It makes them look a little strange. It’s the one dinosaur that if you find it, it’s the only possible thing it can be.”

The genders of the two adults are unknown.

Bamforth said the extraction was difficult because Big Sam was intertwined in a cluster of about 300 other bones.

The skull was found upside down, “as if the animal was lying on its back,” but was well preserved, she said.

She said the excavation process involved putting plaster on the skull and wooden planks around if for stability. From there, it was lifted out — very carefully — with a crane, and was to be shipped on a trolley to the museum for study.

“I have extracted skulls in the past. This is probably the biggest one I’ve ever done though,” said Bamforth.

“It’s pretty exciting.”

This report by The Canadian Press was first published Sept. 25, 2024.

The Canadian Press. All rights reserved.

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The ancient jar smashed by a 4-year-old is back on display at an Israeli museum after repair

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TEL AVIV, Israel (AP) — A rare Bronze-Era jar accidentally smashed by a 4-year-old visiting a museum was back on display Wednesday after restoration experts were able to carefully piece the artifact back together.

Last month, a family from northern Israel was visiting the museum when their youngest son tipped over the jar, which smashed into pieces.

Alex Geller, the boy’s father, said his son — the youngest of three — is exceptionally curious, and that the moment he heard the crash, “please let that not be my child” was the first thought that raced through his head.

The jar has been on display at the Hecht Museum in Haifa for 35 years. It was one of the only containers of its size and from that period still complete when it was discovered.

The Bronze Age jar is one of many artifacts exhibited out in the open, part of the Hecht Museum’s vision of letting visitors explore history without glass barriers, said Inbal Rivlin, the director of the museum, which is associated with Haifa University in northern Israel.

It was likely used to hold wine or oil, and dates back to between 2200 and 1500 B.C.

Rivlin and the museum decided to turn the moment, which captured international attention, into a teaching moment, inviting the Geller family back for a special visit and hands-on activity to illustrate the restoration process.

Rivlin added that the incident provided a welcome distraction from the ongoing war in Gaza. “Well, he’s just a kid. So I think that somehow it touches the heart of the people in Israel and around the world,“ said Rivlin.

Roee Shafir, a restoration expert at the museum, said the repairs would be fairly simple, as the pieces were from a single, complete jar. Archaeologists often face the more daunting task of sifting through piles of shards from multiple objects and trying to piece them together.

Experts used 3D technology, hi-resolution videos, and special glue to painstakingly reconstruct the large jar.

Less than two weeks after it broke, the jar went back on display at the museum. The gluing process left small hairline cracks, and a few pieces are missing, but the jar’s impressive size remains.

The only noticeable difference in the exhibit was a new sign reading “please don’t touch.”

The Canadian Press. All rights reserved.

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