There is a powerful technological tool. After many twists and turns, it was launched on December 25th, 2011. It is currently in a halo at the Sun-Earth L2 point, which will hopefully last for 20 years.

It's only been a few months since its first images were released, and it's already answering some of the Universe's most compelling questions.

The JWST peered into huge clouds of gas and dust to see young stars come to life.

The 'cosmic cliffs' was one of the first images to be taken. The edges of an active star-forming region are known as the Cosmic Cliffs.

The hot young stars that shape the region carve out cavernous gaps and leave towers of gas that resist the radiation in the image.

The results of their work were presented in a paper in the Monthly Notices.

The title is " Deep diving off the'Cosmic Cliffs': previously hidden outflows revealed by JWST." The lead author is an astronomer.

Over two dozen outflows from hot young stars that weren't previously seen were discovered by the researchers. According to a press release announcing the results, there is more than one type of fountain. The outflows can be seen several light years from their star.

annotated image of the cosmic cliffs
New features the JWST found in the Carina Nebula's Cosmic Cliffs. (NASA, ESA, CSA, and STScI, Image processing J. DePasquale STScI)

"Webb gives us a snapshot in time to see how much star formation is going on in what may be a more typical corner of the universe that we haven't been able to see before."

The study was made possible by the power of the JWST. The main ingredient in stars ismolecular hydrogen. As young stars grow, they excrete some of the hydrogen in jets and polar outflows. The jets carve out caverns in the clouds of gas and dust in the picture.

The young stars are obscured from view by the dense clouds. The power of the JWST can be seen in the clouds. One of the telescope's main objectives is to scrutinize young stars in the clouds.

According to a NASA website, "Webb will be able to see right through and into massive clouds of dust that are opaque to visible-light observatories like Hubble, where stars and planetary systems are being born."

All of those words are coming true.

The most exciting part of the star formation process can be seen in the jets. Nathan Smith of the University of Arizona in Tucson said that they only see them during a brief window of time when the Protostar is active.

The astronomer learns more about how our own Sun formed and how our Solar System came to be as a result. Our understanding of the complex mechanisms behind their formation is getting deeper by the day.

"It opens the door for what's going to be possible in terms of looking at these populations of newborn stars in fairly typical environments of the Universe that have been invisible up until now."

We know where to look next to find out what variables are important for the formation of Sun- like stars.

The outflow jets are difficult to observe because they happen inside a thick cloak of gas and only last a short time. For a long time, the jets can only flow for a short time. Astronomers looked at some of the jets and outflows from the original image.

"In 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 - analyzing data from each of the different filters and analyzing each area alone," shared team member Jon Morse.

It is similar to finding buried treasure.

close up image of the cosmic cliffs with a bright spot indicating a star cluster
Star cluster NGC 3324 and the two bright young stars responsible for ionizing the region of gas surrounding them. (NASA/ESA/CSA/JWST Reiter et al. 2022)

Understanding how young stars form is one of the main goals in astrophysics. Light from the first stars helped drive the reionization of the Universe. The universe was obscured by a dense fog of primordial gas. Light from young stars helped clear the haze from the Universe.

One of the main objectives of the JWST is to find out how the first stars formed. The Universe's early days can be seen by the JWST, but it can't make out individual stars.

These new images are essential. Astrophysicists can't study the formation of the first stars, but they can watch young stars form and work on a better understanding of the Epoch of Reionization.

side-by-side images of a gas outflow with raw imagery to left and colorized image to the right
MHO 1643, the brightest outflow in NGC 3324. Left: science image filtered and stripped of vivid color. MHO 1643 has two prominent bow shocks and several additional knots. (NASA/ESA/CSA/JWST Reiter et al. 2022)

Astronomers have looked at the young stars in this area before. Sixteen years ago, the Hubble looked at it.

The study authors were able to compare how the jets and outflows have changed in the intervening years because of the Hubble's revelations.

The speed and direction of the jets are shown in the measured data.

The early release images are the start of the study of stellar formation.

Future observations will allow analysis of the mass-loss rates and velocities of new flows.

"NGC 3324 is a relatively modest region of massive star formation and offers a glimpse of what star formation studies may provide."

Future observations will be more detailed One of the hottest topics in astronomy is how young stars drive planetary formation.

Young stars are marked by feedback. As they grow, they emit some of the gas from the clouds into their surroundings with their jets. The formation of planets like ours can be traced back to the gas outflows.

A better understanding of the outflows leads to a better understanding of the planets.

The cluster in this study is similar to the one that formed our solar system. Astronomers may be able to shed some light on our origins if they uncover the details in NGC 3324.

red glow of clouds depicting NGC 3324
The intense radiation from several of NGC 3324's massive, blue-white stars carving out a cavity in the surrounding gas and dust. (ESO)

The book " The Five Ages of the Universe" states that we live in the universe's "Stelliferous Era" Matter is mostly arranged into stars, galaxies, and clusters. Most of the energy in the universe is produced by stars. The Life Era is thought to be the result of stars providing the energy for life.

We can see how stars are born with the help of the JWST. Along with answering our scientific questions, the results are fascinating. Context to humanity's existence in the universe's life era is given.

Other stars are no different than the Sun. The Sun would have produced the same outflows and polar jets as the young stars in this image if it had been created by the same forces. The Earth's formation would've been influenced by those feedback mechanisms.

We learn a lot when we see young stars elsewhere. We are fortunate to have a space telescope that can show us the stars. The mind is transported along with the eye. We can ponder if life or another civilization might come into being.

This article was published in the past. The original article is worth a read.