Galaxies Spotted by Webb Space Telescope Rewrite Prior Understanding of Universe

Observations by NASA’s James Webb Space Telescope are upending the understanding of the early universe, indicating the presence of large and mature but remarkably compact galaxies teeming with stars far sooner than scientists had considered possible.

Astronomers said data obtained by the telescope reveals what appear to be six big galaxies as mature as our Milky Way existing about 540 million to 770 million years after the explosive Big Bang that kicked off the universe 13.8 billion years ago. The universe was roughly 3 percent of its current age at the time.

These galaxies, one of which appears to have a mass rivaling our Milky Way but 30 times more densely packed, seem to differ in fundamental ways from those populating the universe today.

“Oh, they are radically different — truly bizarre creatures,” said astrophysicist Ivo Labbe of Swinburne University of Technology in Australia, lead author of the study published in the journal Nature. “If the Milky Way were a regular-sized average adult, say about 5 feet, 9 inch (1.75 meters) and 160 pounds (70 kg), these would be 1-year-old babies weighing about the same but standing just under 3 inches (7 cm) tall. The early universe is a freak show.”

Webb was launched in 2021 and began collecting data last year. The findings were based upon the first dataset released by NASA last July from Webb, a telescope boasting infrared-sensing instruments able to detect light from the most ancient stars and galaxies.

“This is an astounding discovery and unexpected. We thought that galaxies form over much longer periods of time,” said Penn State astrophysicist and study co-author Joel Leja. “No one expected to find these. These galaxy candidates are simply too evolved for our expectations. They seem to have evolved faster than allowed by our standard models.”

Leja called them galaxy candidates because further observations are needed to confirm that they all are galaxies rather than some other source of light like a supermassive black hole.

“The exciting part is that even if only some turn out to be massive galaxies, these things are so massive that they alone would upend our measurements of the total mass in stars at this time. It would suggest 10 to 100 times more mass in stars existing at this epoch than expected and would imply that galaxies form way, way faster in the universe than anyone thought.”

The galaxies appear to contain mass equivalent to 10 billion to 100 billion times that of our sun. The latter figure is similar to the Milky Way’s mass.

The journey to galaxy formation following the Big Bang apparently hinged on mysterious material called dark matter that is invisible to us but is known to exist because of the gravitational influence it exerts on normal matter.

“The leading theory is that an ocean of dark matter filled the early universe after the Big Bang,” Labbe said.

“This dark matter — we don’t know what it is actually is — started out really smooth, with only the tiniest of ripples. These ripples grew over time due to gravity and eventually the dark matter started to collect in concentrated clumps, dragging hydrogen gas along for the ride. It’s that hydrogen gas that will eventually turn into stars. Clumps of dark matter, gas and stars is what we call a galaxy,” Labbe added.

Astronomers suspect the first stars began forming 100 million to 200 million years after the Big Bang, each perhaps 1,000 more massive than our sun but much shorter-lived.

“Their explosion set off the chain of events that formed subsequent generations of stars,” Labbe said.

“Webb continuous to amaze and surprise us,” Labbe added. “So yes, the early universe was a lot richer and lot more diverse — monsters and dragons. And the curtain is still being lifted.”

© Thomson Reuters 2023


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NASA’s Webb Captures Pillars of Creation Filled With New Stars, Dense Cloud of Dust

NASA’s James Webb Space Telescope has captured a lush, highly detailed landscape the iconic Pillars of Creation where new stars are forming within dense clouds of gas and dust. The three-dimensional pillars look like majestic rock formations but are far more permeable. These columns are made up of cool interstellar gas and dust that appear at times semi-transparent in near-infrared light.

Webb’s new view of the Pillars of Creation, which were first made famous when imaged by NASA’s Hubble Space Telescope in 1995, will help researchers revamp their models of star formation by identifying far more precise counts of newly formed stars, along with the quantities of gas and dust in the region. Over time, they will begin to build a clearer understanding of how stars form and burst out of these dusty clouds over millions of years.

Newly formed stars are the scene-stealers in this image from Webb’s Near-Infrared Camera (NIRCam). These are the bright red orbs that typically have diffraction spikes and lie outside one of the dusty pillars. When knots with sufficient mass form within the pillars of gas and dust, they begin to collapse under their own gravity, slowly heat up, and eventually form new stars.

What about those wavy lines that look like lava at the edges of some pillars? These are ejections from stars that are still forming within the gas and dust. Young stars periodically shoot out supersonic jets that collide with clouds of material, like these thick pillars. This sometimes also results in bow shocks, which can form wavy patterns like a boat does as it moves through water. The crimson glow comes from the energetic hydrogen molecules that result from jets and shocks. This is evident in the second and third pillars from the top — the NIRCam image is practically pulsing with their activity. These young stars are estimated to be only a few hundred thousand years old.

Although it may appear that near-infrared light has allowed Webb to “pierce through” the clouds to reveal great cosmic distances beyond the pillars, there are no galaxies in this view. Instead, a mix of translucent gas and dust known as the interstellar medium in the densest part of our Milky Way galaxy’s disk blocks our view of the deeper universe.

This scene was first imaged by Hubble in 1995 and revisited in 2014, but many other observatories have also stared deeply at this region. Each advanced instrument offers researchers new details about this region, which is practically overflowing with stars.

This tightly cropped image is set within the vast Eagle Nebula, which lies 6,500 light-years away.

The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA.


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NASA’s James Webb Telescope Captures Colourful Cartwheel Galaxy: Details

The James Webb Space Telescope has peered through time and huge amounts of dust to capture a new image of the Cartwheel Galaxy, revealing the spinning ring of colour in unprecedented clarity, NASA and the European Space Agency said Tuesday. Located around 500 million light-years from Earth in the constellation Sculptor, the Cartwheel gained its shape during a spectacular head-on collision between two galaxies.

The impact sent two rings expanding from the galaxy’s centre, “like ripples in a pond after a stone is tossed into it”, NASA and the ESA said in a joint statement.

A smaller white ring remains closer to the galaxy’s centre, while the outer ring, with its spokes of colour, has been expanding into the universe for around 440 million years, the statement added.

As the outer ring expands it runs into gas, sparking the formation of new stars.

The Hubble telescope had previously captured images of the rare ring galaxy, which is believed to have been a spiral galaxy like our own Milky Way before it was hit by a smaller intruder galaxy.

But the Webb telescope, which launched in December 2021 and revealed its first images to global fanfare last month, has a far greater reach.

Webb’s ability to detect infrared light allowed it to see through the “tremendous amount of hot dust” obscuring the view of the Cartwheel Galaxy, NASA and the ESA said.

This revealed new details about star formation in the galaxy, as well as the behaviour of the supermassive black hole at its heart, they said.

It was also able to detect regions rich in hydrocarbons and other chemicals, as well as dust that is similar to dust on Earth.

Behind the Cartwheel, two smaller galaxies shine brightly, while even more galaxies can be seen behind them.

The observations show that the Cartwheel Galaxy is still in “very transitory stage”, the space agencies said.

“While Webb gives us a snapshot of the current state of the Cartwheel, it also provides insight into what happened to this galaxy in the past and how it will evolve in the future.”


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NASA’s James Webb Space Telescope Almost Set to Go for Solar System Exploration, Find Universe’s Deepest Secrets

Our wait seems to be nearing its end as NASA’s James Webb Space Telescope is in its final stages of completion before being launched to explore the solar system. The Webb team is undertaking the final stages of commissioning the essential instruments aboard the observatory. Technical operations have also begun to test these instruments. The team is running a final test to check how precisely the Webb telescope can find distant stars and galaxies and acquire their images and spectra. The observatory is also equipped to keep a check on satellites, asteroids, and comets in the solar system.

The task of the Webb telescope is to lock its observing tools on the objects that are swiftly moving against a background of stars of our Milky Way galaxy. In order to check the observatory’s capabilities to undertake such complex tasks, the team ran the first test to track a moving object and Webb succeeded in the test. Scientists, now, aim to test different objects, which will move at varying speeds, to test the precision of Webb’s instruments.

Heidi Hammel, Webb’s interdisciplinary scientist for solar system observations, shares, “Webb can detect the faint light of the earliest galaxies, but my team will be observing much closer to home. They will use Webb to unravel some of the mysteries that abound in our own solar system.”

But, isn’t Webb meant to observe the deepest corners of outer space? Do we really need such a powerful tool to study our solar system? The answers lie in a statement by Ms Hammel, “We planetary scientists use telescopes to complement our in situ missions (missions that we send to fly by, orbit, or land on objects). One example of this is how Hubble was used to find the post-Pluto target for the New Horizons mission, Arrokoth. We also use telescopes when we don’t have in situ missions planned — like for the distant ice giants Uranus and Neptune or to make measurements of large populations of objects, such as hundreds of asteroids or Kuiper Belt Objects (small ice worlds beyond the orbits of Neptune, including Pluto) since we can only send missions to just a few of these.”

“Our solar system has far more mysteries than my team had time to solve. Our programs will observe objects across the solar system,” said Hammel.

Her team is planning to observe the giant planets, Saturn‘s rings, the atmosphere of Mars and Kuiper Belt Objects, among other mysteries.


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