Skip to main content

The Pillars of Creation look spooky in new James Webb image

Following on from the recent release of a stunning image of the Pillars of Creation, researchers using the James Webb Space Telescope have released another image of the pillars — and it’s a spooky one. Taken in the mid-infrared range using Webb’s Mid-Infrared Instrument (MIRI), the new image shows the enormous clouds of dust that form the famous structure of the pillars.

The previous Webb image of the pillars was taken in the near-infrared range using the Near-Infrared Camera (NIRCam) and showed off the thousands of stars that glow brightly in that range. By looking at the same target in different wavelengths, astronomers can see different features and get a new view of a familiar sight.

NASA’s James Webb Space Telescope’s mid-infrared view of the Pillars of Creation.
NASA’s James Webb Space Telescope’s mid-infrared view of the Pillars of Creation strikes a chilling tone. Thousands of stars that exist in this region disappear – and seemingly endless layers of gas and dust become the centerpiece. SCIENCE: NASA, ESA, CSA, STScI IMAGE PROCESSING: Joseph DePasquale (STScI), Alyssa Pagan (STScI)

The beautiful pillars, which are located 6,500 light-years away in the Eagle Nebula, look rather sinister in this wavelength as James Webb scientists explain: “Why does mid-infrared light set such a somber, chilling mood in Webb’s Mid-Infrared Instrument (MIRI) image? Interstellar dust cloaks the scene. And while mid-infrared light specializes in detailing where dust is, the stars aren’t bright enough at these wavelengths to appear. Instead, these looming, leaden-hued pillars of gas and dust gleam at their edges, hinting at the activity within.”

Recommended Videos

MIRI is the only Webb instrument that operates in the mid-infrared, which means it has different sensors and different temperature requirements from the other three instruments which operate in the near-infrared. The mid-infrared range is excellent for studying dust, which plays a vital role in the formation of new stars. The pillars are a hotbed of star formation and the dust and gas form into knots that gather material toward them before collapsing under gravity and forming protostars.

However, few stars are visible here as stars don’t give off much light in this wavelength. The few stars which are visible are the younger stars that are still cloaked in dust, which appear in red, and a handful of older stars that have shed their layers and are shown in blue.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
One galaxy, two views: see a comparison of images from Hubble and Webb
The peculiar galaxy NGC 3256 takes centre stage in this image from the NASA/ESA Hubble Space Telescope. This distorted galaxy is the wreckage of a head-on collision between two spiral galaxies which likely occurred 500 million years ago, and it is studded with clumps of young stars which were formed as gas and dust from the two galaxies collided.

It might not seem obvious why astronomers need multiple different powerful space telescopes. Surely a more powerful telescope is better than a less powerful one? So why are there multiple different telescopes in orbit, either around Earth or around the sun?

The answer is to do with two main factors. One is the telescope's field of view, meaning how much of the sky it looks at. Some telescopes are useful for looking at large areas of the sky in less detail, working as survey telescopes to identify objects for further research or to look at the universe on a large scale -- like the recently launched Euclid mission. While others, like the Hubble Space Telescope, look at small areas of the sky in great detail, which is useful for studying particular objects.

Read more
James Webb spots the most distant active supermassive black hole ever discovered
Crop of Webb's CEERS Survey image.

As well as observing specific objects like distant galaxies and planets here in our solar system, the James Webb Space Telescope is also being used to perform wide-scale surveys of parts of the sky. These surveys observe large chunks of the sky to identify important targets like very distant, very early galaxies, as well as observe intriguing objects like black holes. And one such survey has recently identified the most distant active supermassive black hole seen so far.

While a typical black hole might have a mass up to around 10 times that of the sun, supermassive black holes are much more massive, with a mass that can be millions or even billions of times the mass of the sun. These monsters are found at the heart of galaxies and are thought to play important roles in the formation and merging of galaxies.

Read more
Saturn as you’ve never seen it before, captured by Webb telescope
Saturn captured by the James Webb Space Telescope

NASA has shared a gorgeous image of Saturn captured recently by the James Webb Space Telescope (JWST).

Webb’s first near-infrared observations of the second largest planet in our solar system also show several of Saturn’s moons: Dione, Enceladus, and Tethys.

Read more