Skip to main content

See the universe in stunning detail in first James Webb image

After years of planning and months in space, the James Webb Space Telescope has inaugurated a new era in astronomy. NASA today released the first science image from the world’s most powerful space telescope, showing the infrared universe in a depth never seen before.

“From the beginning of history, humans have looked up to the night sky with wonder,” Vice President Kamala Harris said in a briefing. “Now, we enter a new phase of scientific discovery. Building on the legacy of Hubble, the James Webb Space Telescope allows us to see deeper into space than ever before and in stunning clarity.” Harris also acknowledged the contributions of international partners in the building of Webb, which included NASA, the European Space Agency, and the Canadian Space Agency: “This telescope is one of humanity’s great engineering achievements,” she said.

Known as Webb’s First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail.
This first image from NASA’s James Webb Space Telescope is the deepest and sharpest infrared image of the distant universe to date. Known as Webb’s First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail. Thousands of galaxies – including the faintest objects ever observed in the infrared – have appeared in Webb’s view for the first time. This slice of the vast universe covers a patch of sky approximately the size of a grain of sand held at arm’s length by someone on the ground. NASA, ESA, CSA, and STScI

The image shows galaxy cluster SMACS 0723 and is the deepest infrared image of the distant universe to date. It shows the cluster as it would have been 4.6 billion years ago, and because the mass of the cluster is so great it bends spacetime and allows us to see even more distant galaxies behind it. As they are so distant the light is very faint, and these thousands of galaxies are among the faintest objects ever observed in infrared — captured thanks to Webb’s NIRCam instrument in a composite of observations taken over 12.5 hours to pick up this level of detail.

Unlike telescopes like Hubble which look primarily in the visible light range, equivalent to what would be seen by the human eye, Webb’s instruments operate in the infrared. This enables the telescope to look through opaque targets like clouds of dust to see what lies beneath, and it will be used to study nebulae, stars, black holes, and more.

Webb’s instruments are so sensitive that they can observe extremely distant targets, which — because of the time it takes for light to travel from these great distances to Earth — is like looking back in time. Webb will search out some of the earliest galaxies in the universe, helping to elucidate a period called the Epoch of Reionization when the earliest stars spread light through the universe for the first time.

Deep field images like the one shown above help in the quest to find the earliest galaxies by identifying extremely distant galaxies in dim patches of the sky. Similar images will be produced by deep and wide surveys made using Webb, such as the upcoming COSMOS-Webb program.

The image released today is just a teaser of all that is to come from Webb. More images will be released tomorrow, including images of nebulae and a galaxy group, as well as a spectrum showing the composition of the atmosphere of an exoplanet. And there will be plenty more topics that Webb will study in its first year as well, giving astronomers glimpses into topics as wide-ranging as how stars are formed, the composition of comets in our solar system, and how the first black holes formed.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Stunning image shows the magnetic fields of our galaxy’s supermassive black hole
The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of our Milky Way black hole released in 2022, has captured a new view of the massive object at the center of our Galaxy: how it looks in polarized light. This is the first time astronomers have been able to measure polarization, a signature of magnetic fields, this close to the edge of Sagittarius A*. This image shows the polarized view of the Milky Way black hole. The lines mark the orientation of polarization, which is related to the magnetic field around the shadow of the black hole.

The Event Horizon Telescope collaboration, the group that took the historic first-ever image of a black hole, is back with a new stunning black hole image. This one shows the magnetic fields twirling around the supermassive black hole at the heart of our galaxy, Sagittarius A*.

Black holes are hard to image because they swallow anything that comes close to them, even light, due to their immensely powerful gravity. However, that doesn't mean they are invisible. The black hole itself can't be seen, but the swirling matter around the event horizon's edges glows brightly enough to be imaged. This new image takes advantage of a feature of light called polarization, revealing the powerful magnetic fields that twirl around the enormous black hole.

Read more
See the stunning Vela supernova remnant in exquisite detail in expansive image
This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the US National Science Foundation's Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF’s NOIRLab. The striking reds, yellows, and blues in this image were achieved through the use of three DECam filters that each collect a specific color of light. Separate images were taken in each filter and then stacked on top of each other to produce this high-resolution image that contains 1.3 gigapixels and showcases the intricate web-like filaments snaking throughout the expanding cloud of gas.

A new image of the ghostly Vela supernova remnant shows off the fascinating and elaborate structure of this striking cosmic object. Taken using the Dark Energy Camera (DECam), this enormous image is 1.3 gigapixels, making it DECam's largest image to date.

This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the U.S. National Science Foundation's Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile. CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab)

Read more
The expansion rate of the universe still has scientists baffled
This image of NGC 5468, a galaxy located about 130 million light-years from Earth, combines data from the Hubble and James Webb space telescopes. This is the most distant galaxy in which Hubble has identified Cepheid variable stars. These are important milepost markers for measuring the expansion rate of the Universe. The distance calculated from Cepheids has been cross-correlated with a Type Ia supernova in the galaxy. Type Ia supernovae are so bright they are used to measure cosmic distances far beyond the range of the Cepheids, extending measurements of the Universe’s expansion rate deeper into space.

The question of how fast the universe is expanding continues to confound scientists. Although it might seem like a fairly straightforward issue, the reality is that it has been perplexing the best minds in physics and astronomy for decades -- and new research using the James Webb Space Telescope and the Hubble Space Telescope doesn't make the answer any clearer.

Scientists know that the universe is expanding over time, but what they can't agree on is the rate at which this is happening -- called the Hubble constant. There are two main methods used to estimate this constant: one that looks at how fast distant galaxies are moving away from us, and one that looks at leftover energy from the Big Bang called the cosmic microwave background. The trouble is, these two methods give different results.

Read more