The first deep-field image from the James Webb Space Telescope

NASA, ESA, CSA, STScI

NASA’s James Webb Space Telescope (JWST) has released its first full-resolution images in a preview of the science soon to come. These five images, showing two sparkling nebulas, a group of doomed galaxies and the chemical composition of a giant exoplanet, are the culmination of decades of work by scientists and engineers – and they are just the beginning.

After its December 2021 launch, JWST beamed down its very first images in February, but those were part of the telescope testing process, and they didn’t yet demonstrate JWST’s full power. But these science images do.

Advertisement

The JWST deep field

The first image, released on 11 July and seen above, is the deepest image of the cosmos ever taken. JWST was designed to take such images to help us understand the first galaxies. The faint galaxies in this image include the most distant galaxy whose composition we have ever been able to measure.

“The previous record-holder, the Hubble Extreme Deep Field, was two weeks of continuous work with Hubble,” said JWST scientist Jane Rigby during the image release event at NASA’s Goddard Space Flight Center in Maryland. “With Webb, we took that image before breakfast… We’re going to be doing discoveries like this every week.”

WASP-96b

New Scientist Default Image

Light spectrum from exoplanet WASP-96b

NASA, ESA, CSA, STScI

This image showcases one of JWST’s other key capabilities: examining the light shining through the atmosphere of an exoplanet. It is the spectrum of light coming from a planet called WASP-96b, a gas giant about 1150 light years from Earth. Its mass is about half that of Jupiter, but it is much closer to its star – and therefore far hotter – orbiting once every 3.4 days while Jupiter takes 12 Earth years to circle the sun. This particular planet has almost no clouds whatsoever, making it far easier to examine the chemistry of its atmosphere without anything to block the starlight shining through.

“It’s extremely hot, extremely close in, nothing like our solar system planets – but it’s okay,” said Knicole Colon at Goddard. “This is just the beginning. We’re going to start pushing down to further, smaller planets and being able to take measurements just like this.”

Southern Ring Nebula

This side-by-side comparison shows observations of the Southern Ring Nebula in near-infrared light, at left, and mid-infrared light, at right, from NASA???s Webb Telescope. This scene was created by a white dwarf star ??? the remains of a star like our Sun after it shed its outer layers and stopped burning fuel though nuclear fusion. Those outer layers now form the ejected shells all along this view. In the Near-Infrared Camera (NIRCam) image, the white dwarf appears to the lower left of the bright, central star, partially hidden by a diffraction spike. The same star appears ??? but brighter, larger, and redder ??? in the Mid-Infrared Instrument (MIRI) image. This white dwarf star is cloaked in thick layers of dust, which make it appear larger. The brighter star in both images hasn???t yet shed its layers. It closely orbits the dimmer white dwarf, helping to distribute what it???s ejected. Over thousands of years and before it became a white dwarf, the star periodically ejected mass ??? the visible shells of material. As if on repeat, it contracted, heated up ??? and then, unable to push out more material, pulsated. Stellar material was sent in all directions ??? like a rotating sprinkler ??? and provided the ingredients for this asymmetrical landscape. Today, the white dwarf is heating up the gas in the inner regions ??? which appear blue at left and red at right. Both stars are lighting up the outer regions, shown in orange and blue, respectively. The images look very different because NIRCam and MIRI collect different wavelengths of light. NIRCam observes near-infrared light, which is closer to the visible wavelengths our eyes detect. MIRI goes farther into the infrared, picking up mid-infrared wavelengths. The second star more clearly appears in the MIRI image, because this instrument can see the gleaming dust around it, bringing it more clearly into view. The stars ??? and their layers of light ??? steal more attention in the NIRCam image, while dust pl

Side-by-side observations of the Southern Ring Nebula in near-infrared light, at left, and mid-infrared light, at right

This cloud of dust and gas surrounding two stars is called the Southern Ring Nebula, or the Eight-Burst Nebula. Both of these images show the nebula in infrared, but the one on the right was taken using longer wavelengths than the one at left.

The Southern Ring Nebula is about 2000 light years away and nearly half a light year across. The bright cloud that makes up the ring came from the outer layers of one of the stars at the centre of the nebula, which expanded when it reached the end of its lifetime and transformed from a sun-like star into a white dwarf. The image on the right has revealed the two stars in extraordinary detail, showing that the dimmer, redder star – the one that spawned this nebula – is surrounded by dust, whereas the brighter star may puff out its own nebula in the future.

Stephan’s Quintet

New Scientist Default Image

Stephan’s Quintet galaxy cluster

NASA, ESA, CSA, STScI

These five galaxies, called Stephan’s Quintet, are about 290 million light years away in the direction of the constellation Pegasus. Four of the five are engaged in a deadly game of chicken, swooping past one another closer and closer until, someday in the distant cosmic future, they will most likely smash together and merge. We have seen them before – in fact, the group of four is the most thoroughly studied compact group of galaxies – but this image is far more detailed than any of the previous ones. It is a mosaic of almost 1000 pictures, making it JWST’s biggest image to date.

That detail allows us to see the area around a supermassive black hole, the brightest part of the top galaxy. “We cannot see the black hole itself, but we see the material sort of swirling around and being swallowed by this cosmic monster,” said JWST researcher Giovanna Giardino. This area is 40 billion times as bright as the sun, she said.

Carina Nebula

New Scientist Default Image

The Carina Nebula

NASA, ESA, CSA, STScI

One of the brightest nebulas in the sky, the Carina Nebula is a huge cloud of gas and nascent stars. It is about 7600 light years away in the direction of the constellation Carina. The top part of the image is full of huge, hot stars, shining onto the stellar nursery at the bottom of the picture.

“Today, for the first time, we’re seeing brand new stars that were completely hidden from our view,” said JWST scientist Amber Straughn. “We see examples of bubbles and cavities and jets that are being blown out by these newborn stars. We even see some galaxies sort of lurking in the background up here. We see examples of structures that honestly we don’t even know what they are. The data is just so rich.”

Read more: 7 big questions the James Webb Space Telescope is about to answer

Now that we have the first full-resolution images from JWST, the next step is getting more detailed data so that researchers can start digging into the science. This includes not only the data behind these images, but even deeper observations of the cosmos, from the most distant stars to a bevy of alien worlds to asteroids in our own solar system.

“This day gives a new meaning to ‘as far as the eye can see’,” said US Congressman Steny Hoyer during the image release event. Over the coming months and years, JWST is expected to continue pushing the limits of astronomy. It has enough fuel to continue observing for at least 20 years, and the release of these new images marks the beginning of year one.

Sign up to our free Launchpad newsletter for a voyage across the galaxy and beyond, every Friday

More on these topics: