JWST has spotted the birth of a star like never before in the Carina Nebula, and it’s amazing

The powerful James Webb Space Telescope is a powerful technological tool. It was first conceived by astrophysicists over 20 years ago, and after many twists and turns, it was launched on December 25, 2021. It is now in a halo orbit at the Sun-Earth point L2, where it will hopefully continue to operate for the next 20 years.

It’s only been a few months since his first images were released, and he’s already made progress in answering some of the universe’s most pressing questions.

In a newly released image, JWST peers deep inside huge clouds of gas and dust to watch young stars come to life in their stellar cocoons.

One of the first images of JWST was “Cosmic Ramps”. The cosmic slopes are the edge of an active star-forming region in NGC 3324, a star cluster near the Carina Nebula.

The image shows intense ultraviolet energy from hot young stars forming the region, carving cavernous cavities and leaving towers of gas that resist radiation.

We were all amazed by that image in July, but scientists delved into it to learn more about the region and the star-forming activity taking place there. the Monthly Notices of the Royal Astronomical Society (MNRAS) Publish a paper presenting the results of their work.

It’s titled “Deep Diving” in Cosmic Slope: Previously Hidden Outflows in NGC 3324 and Revealed by JWST. The lead author is astronomer Megan Reiter of Rice University in Houston, Texas.

The researchers closely examined Webb’s image and found more than two dozen outflows of hot young stars that had not been seen before. There’s everything from “tiny fountains to pesky giants,” according to a press release announcing the findings. Some outflows extend several light years from their star.

New features found by JWST in the cosmic slopes of the Carina Nebula. (NASA, ESA, CSA, and STScI, J. DePasquale STScI Image Processing)

“What Webb gives us is a snapshot in time of how much star formation is going on in what might be a typical corner of the universe that we haven’t been able to see before,” Reiter said.

The powerful infrared capabilities of JWST fueled this study. It can focus on molecular hydrogen, the main ingredient in stars. It’s an excellent tracker of star formation activity because as young stars grow, they take in hydrogen and eject some of it in polar jets and outflows. They’re called stellar feedback, and these jets carve out caverns in the clouds of gas and dust pictured.

Young protostars that are still forming are obscured by the dense molecular clouds spawned by protostars. But JWST has the ability to see inside these clouds. One of the telescope’s four main science goals is examining young stars within the clouds.

“Webb will be able to see through and into huge clouds of dust that are opaque to visible-light observatories like Hubble, where stars and planetary systems are born,” NASA’s website explained long before the telescope’s completion and launch.

Now we are seeing all these words come true.

“Jeters like these are markers of the most exciting part of the star formation process. We only see them over a short period of time when the protostar is actively accreting,” explained co-author Nathan Smith of the University of Arizona in Tucson.

The more astronomers learn about young stars that formed elsewhere, the more they’ll learn about how our sun formed and how our solar system came to be. The JWST broadens and deepens our understanding of the complex mechanisms behind their formation.

“It opens the door to what would be possible in terms of looking at these clusters of infant stars in fairly typical environments of the universe that were invisible until the James Webb Space Telescope,” Reiter added.

“Now we know where to look next to explore the variables important for the formation of sun-like stars.”

Outflows are difficult to observe in the early stages of star formation because they occur within a dense mantle of gas and last only for a short time. The jets could only flow for a few thousand years, maybe ten thousand. Using JWST’s powerful filters, astronomers have screened some of the jets and jets streaming outward from the original Cosmic Cliffs image that was hinted at.

β€œIn the image first released in July, you see hints of this activity, but these jets are only visible when you embark on that deep dive β€” dissecting the data from each of the different filters and analyzing each area individually,” said a member Lieutenant General John Morse. from the California Institute of Technology in Pasadena.

“It’s like finding buried treasure.”

Close-up of the cosmic slopes with a bright spot indicating the presence of a star cluster
The star cluster NGC 3324 and the two bright stars responsible for ionizing the surrounding gaseous region. (NASA/ESA/CSA/JWST Reiter et al. 2022)

Understanding how young stars form is one of the primary tasks in astrophysics today. The collective light from the first stars helped re-ionize the early universe. Before the era of reionization, a thick haze of primordial gas shrouded the universe. During reionization, the light from the young stars helped clear the haze from the universe and allow the light to travel.

But astrophysicists don’t know how these first stars formed, and addressing this question is one of JWST’s main science goals. The JWST can see highly redshifted objects from the early days of the universe, but it cannot form individual stars.

This is why these newly released images are a must. Astrophysicists can’t study the formation of the first stars, but they can watch young stars form today and work their way toward a stronger understanding of the age of reionization.

Side-by-side images of the gas flow with the raw images to the left and the color image to the right
MHO 1643, the brightest outflow in NGC 3324. Left: filtered science image and just bright colors. MHO 1643 has two prominent bow shocks and several additional nodes. (NASA/ESA/CSA/JWST Reiter et al. 2022)

This isn’t the first time astronomers have studied the formation of young stars in this region. Hubble looked at it 16 years ago.

And although Hubble can’t discern details like James Webb, it did reveal enough for the study’s authors to compare how jets and outflows have changed in the intervening years.

The measurements show the speed and direction in which the jets are moving, details essential to understanding young stars.

These are the early launch (ERO) images and are just the beginning of JWST and its study of star formation.

“Future observations will allow quantitative analysis of the excitations, mass loss rates, and velocities of these new jets,” the authors write.

“As a relatively modest region of massive star formation, NGC 3324 provides a preview of what studies of star formation with the JWST may provide.”

Future notes will be more comprehensive and detailed. They will help shed more light on one of the hottest topics in astronomy: how young stars drive planet formation.

Feedback mechanisms characterize young stars. They are still growing, and as they accumulate gas from the clouds into which they merge, they emit some of it back into their surroundings with their jets. Outflows of gas help shape protoplanetary disks and form planets like ours.

A better understanding of these outflows leads to a better understanding of the planets and, through complex expansion, the potential for life to emerge elsewhere.

Our solar system likely formed in a cluster similar to the one in this study. Astronomers aren’t sure yet, but by revealing details in NGC 3324, they may shed some light on our origins.

A red glow of clouds representing NGC 3324
Intense radiation from NGC 3324’s many blue-white massive stars creates a hole in the surrounding gas and dust. (ESO)

We live in the “stellar age” of the universe, according to the book “The Five Ages of the Universe.” At this age, matter is mainly arranged into stars, galaxies, and galaxy clusters. Stars produce most of the energy in the universe and will last for a long time. Since the stars provide energy for life, the stellar age may easily be called the age of life.

JWST can collect ancient light from the first stars and galaxies and peer deep inside stellar cocoons to show us how stars are born. The results are great scientific understandings, but along with answering our scientific questions, JWST does something else. It gives context for humanity’s existence in the age of the life of the universe.

The sun is no different from other stars. The same forces gave rise to its formation and evolution, and the Sun would have emitted the same polar outflows and jets as the young stars in this image. These feedback mechanisms would have shaped the protoplanetary disk in which the Earth formed.

So every time we see photos of young stars elsewhere, we learn something about our origins. We are fortunate to have the James Webb Space Telescope to show us such clear and vast horizons of star birth. Exquisite and exquisite details convey the mind as well as the eye. We can sit back and wonder if every single one, life, or even another civilization, might have arisen.

This article was originally published by Universe Today. Read the original article.

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