Skip to main content

James Webb snapped a picture of an exoplanet for the first time

The James Webb Space Telescope has directly imaged an exoplanet for the first time. This is exciting because it is very rare for exoplanets to be directly imaged, as usually, their existence has to be inferred from other data. By taking an image of a planet outside our solar system, Webb demonstrates how we’ll be able to gather more information than ever before about distant worlds.

There are over 5,000 known exoplanets, but the vast majority of these have been detected using techniques like the transit method, in which the light from a host star dips slightly when a planet passes in front of it, or radial velocity, in which a star is slightly tugged around by the gravity of a planet. In these methods, the existence of a planet is inferred because of the effect that can be observed on a star, so the planet itself isn’t directly observed. In rare cases, however, an exoplanet can be observed directly, particularly if it is a large planet located relatively nearby.

This image shows the exoplanet HIP 65426 b in different bands of infrared light.
This image shows the exoplanet HIP 65426 b in different bands of infrared light, as seen from the James Webb Space Telescope: purple shows the NIRCam instrument’s view at 3.00 micrometers, blue shows the NIRCam instrument’s view at 4.44 micrometers, yellow shows the MIRI instrument’s view at 11.4 micrometers, and red shows the MIRI instrument’s view at 15.5 micrometers. These images look different because of the ways the different Webb instruments capture light. NASA/ESA/CSA, A Carter (UCSC), the ERS 1386 team, and A. Pagan (STScI)

Webb made one such direct observation of the exoplanet HIP 65426 b, and was able to capture an image of the planet using four different filters. Each of these filters corresponds to a different wavelength of light, capturing different features of the planet and its environment. The planet is a big one at between six and 12 times the mass of Jupiter, and it is a relative youngster at just 15 to 20 million years old.

“This is a transformative moment, not only for Webb but also for astronomy generally,” said leader of the observations Sasha Hinkley in a statement.

To observe the planet, the researchers needed to block out the light coming from the planet’s host star. As the star is so much brighter than the planet, this light has to be blocked to make it possible to see the planet. This is done with an instrument called a coronagraph, which is a mask that blocks light from a bright source.

“It was really impressive how well the Webb coronagraphs worked to suppress the light of the host star,” Hinkley said.

“Obtaining this image felt like digging for space treasure,” said another of the researchers, Aarynn Carter. “At first all I could see was light from the star, but with careful image processing I was able to remove that light and uncover the planet.”

This finding demonstrates some of Webb’s abilities when it comes to finding and investigating exoplanets. “I think what’s most exciting is that we’ve only just begun,” Carter said. “There are many more images of exoplanets to come that will shape our overall understanding of their physics, chemistry, and formation. We may even discover previously unknown planets, too.”

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Psyche spacecraft sends data back to Earth using lasers for the first time
NASA’s Psyche spacecraft is shown in a clean room at the Astrotech Space Operations facility near the agency’s Kennedy Space Center in Florida on Dec. 8, 2022. DSOC’s gold-capped flight laser transceiver can be seen, near center, attached to the spacecraft.

NASA's experimental laser communication system, riding along with the Psyche spacecraft, has hit another milestone. The system was recently used to transmit Psyche data from over 140 million miles (226 million kilometers) away.

The system, called Deep Space Optical Communications, or DSOC, has previously been used to send test data and even to send a video of a cat, to test whether using laser communications in addition to the usual radio communications is possible. But as this is technology is experimental, the Psyche spacecraft has its own radio communications system it has been using to transmit its science data. Now, though, DSOC has been able to interface with the Psyche systems and send Psyche engineering data back to Earth as well.

Read more
First indications of a rare, rainbow ‘glory effect’ on hellish exoplanet
For the first time, potential signs of the rainbow-like ‘glory effect’ have been detected on a planet outside our Solar System. Glory are colourful concentric rings of light that occur only under peculiar conditions. Data from ESA’s sensitive Characterising ExOplanet Satellite, Cheops, along with several other ESA and NASA missions, suggest this delicate phenomenon is beaming straight at Earth from the hellish atmosphere of ultra-hot gas giant WASP-76b, 637 light-years away.

Just from looking at our own solar system, we can see that planets come in a wide variety of colors -- from the dusty red of Mars to the bright blues of Uranus and Neptune. Planets like Jupiter have beautiful bands of color caused by variations in the atmosphere, while it's hard to even see the surface of Venus because its atmosphere is so thick. But there are other variations in color which planets can display, like a stunning rainbow-hued set of circular rings called a glory.

Glories are observed on Earth, and have been seen just once on another planet, Venus. But now, researchers believe they may have identified a glory on a planet outside our solar system for the first time. The extreme exoplanet WASP-76b could be host to the first known extrasolar glory, observed by the European Space Agency (ESA)'s Characterising ExOplanet Satellite (Cheops).

Read more
James Webb images capture the galactic winds of newborn stars
A team of astronomers used the NASA/ESA/CSA James Webb Space Telescope to survey the starburst galaxy Messier 82 (M82), which is located 12 million light-years away in the constellation Ursa Major. M82 hosts a frenzy of star formation, sprouting new stars 10 times faster than the Milky Way galaxy. Webb’s infrared capabilities enabled scientists to peer through curtains of dust and gas that have historically obscured the star formation process. This image from Webb’s NIRCam (Near-Infrared Camera) instrument shows the centre of M82 with an unprecedented level of detail. With Webb’s resolution, astronomers can distinguish small, bright compact sources that are either individual stars or star clusters. Obtaining an accurate count of the stars and clusters that compose M82’s centre can help astronomers understand the different phases of star formation and the timelines for each stage.

A stunning new pair of images from the James Webb Space Telescope show a new view of a familiar galaxy. Messier 82 is a famous starburst galaxy, full of bright and active star formation, and scientists are using Webb to study how stars are being born in the busy conditions at the center of the galaxy.

Astronomers used Webb's NIRCam instrument to observe the galaxy, and by splitting the resulting data into shorter and longer wavelengths, you can see different features which are picked out in the bustling, active region where stars are forming.

Read more