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Gorgeous images show off James Webb telescope’s remarkable abilities

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If yesterday’s deep field image got you excited for the James Webb Space Telescope, there’s a veritable feast of space images on offer today. NASA has released four more images showing off the capabilities of the world’s most powerful space telescope and giving a taster of what science it will be able to perform in the future.

First up is a stunning image of the Carina Nebula, nicknamed the Cosmic Cliffs for its mountainous shapes. This cloud of dust and gas is a star-forming region that is lit up by bright young stars. These huge, hot young stars give off stellar winds which shape the gas into these stunning structures, and studying the region can help to learn about how common these young stars are and how they influence star formation around them. The nebula is located 7,600 light-years away and was captured using two of Webb’s cameras, NIRCam and MIRI.

This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula.
This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. NASA, ESA, CSA, and STScI / NASA, ESA, CSA, and STScI

The second image is a quintet of galaxies locked into a cosmic dance. Four of the five members of the galaxy group Stephan’s Quintet are extremely close together and are in the process of merging, giving scientists information about how galaxies grow larger and evolve over time. This is Webb’s largest image so far, covering a huge area in an image of over 150 million pixels. The closest galaxy of the group is located 40 million light-years away, while the other four are much more distant at 290 million light-years away.

Stephan’s Quintet, imaged by the James Webb Space Telescope.
Stephan’s Quintet, a visual grouping of five galaxies, is best known for being prominently featured in the holiday classic film, “It’s a Wonderful Life.” Today, NASA’s James Webb Space Telescope reveals Stephan’s Quintet in a new light. This enormous mosaic is Webb’s largest image to date, covering about one-fifth of the Moon’s diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The information from Webb provides new insights into how galactic interactions may have driven galaxy evolution in the early universe. NASA, ESA, CSA, and STScI

This striking structure is called the Southern Ring Nebula and is a type of nebula that is formed by a dying star throwing off layers of dust and gas. This dust and gas spreads out into space and forms a huge shell, which makes it hard to see the structure of the nebula in the visible light range. But in the infrared wavelength, where Webb operates, it is possible to peer inside the dusty shell and see the nebula beneath. This image shows how imaging the same structure in different wavelengths can bring out different features of an object, as the image on the left was taken in the near-infrared by Webb’s NIRCam, and the image on the right was taken in the mid-infrared by Webb’s MIRI instrument.

Two stars imaged by the James Webb telescope. The stars – and their layers of light – are prominent in the image from Webb’s Near-Infrared Camera (NIRCam) on the left, while the image from Webb’s Mid-Infrared Instrument (MIRI) on the right shows for the first time that the second star is surrounded by dust.
Two stars, which are locked in a tight orbit, shape the local landscape. Webb’s infrared images feature new details in this complex system. The stars – and their layers of light – are prominent in the image from Webb’s Near-Infrared Camera (NIRCam) on the left, while the image from Webb’s Mid-Infrared Instrument (MIRI) on the right shows for the first time that the second star is surrounded by dust. The brighter star is in an earlier stage of its stellar evolution and will probably eject its own planetary nebula in the future. NASA, ESA, CSA, and STScI

Finally, the last treat from Webb today is not an image but a spectrum, or an analysis of the light coming from a distant planet. Using spectroscopy, Webb was able to determine that water is present in the atmosphere of the superhot planet WASP-96 b. This gas giant orbits so close to its star that a year there lasts just three and a half Earth days, and it is estimated to have a surface temperature of over 1000°F. Before Webb, it was extremely difficult to analyze the atmospheres of exoplanets so the ability to detect gas molecules in an exoplanet atmosphere is a major step forward in planetary science.

A chart demonstrating the atmospheric composition of Hot Gas Giant Exoplanet WASP-96b.
NASA’s James Webb Space Telescope has captured the distinct signature of water, along with evidence for clouds and haze, in the atmosphere surrounding a hot, puffy gas giant planet orbiting a distant Sun-like star. NASA, ESA, CSA, and STScI

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Georgina Torbet
Georgina Torbet
Space Writer
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
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