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.

Recommended Videos

“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 has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb image shows two galaxies in the process of colliding
This composite image of Arp 107, created with data from the James Webb Space Telescope’s NIRCam (Near-InfraRed Camera) and MIRI (Mid-InfraRed Instrument), reveals a wealth of information about the star formation taking place in these two galaxies and how they collided hundreds of million years ago. The near-infrared data, shown in white, show older stars, which shine brightly in both galaxies, as well as the tenuous gas bridge that runs between them. The vibrant background galaxies are also brightly illuminated at these wavelengths.

A new image from the James Webb Space Telescope shows one of the universe's most dramatic events: the colliding of two galaxies. The pair, known as Arp 107, are located located 465 million light-years away and have been pulled into strange shapes by the gravitational forces of the interaction, but this isn't a purely destructive process. The collision is also creating new stars as young stars are born in swirling clouds of dust and gas.

The image above is a composite, bringing together data from Webb's NIRCam (Near-InfraRed Camera) and MIRI (Mid-InfraRed Instrument). These two instruments operate in different parts of the infrared, so they can pick up on different processes. The data collected in the near-infrared range is seen in white, highlighting older stars and the band of gas running between the two galaxies. The mid-infrared data is shown in orange and red, highlighting busy regions of star formation, with bright young stars putting out large amounts of radiation.

Read more
Crew Dragon is about to fly with empty seats for the first time. Here’s why
A Falcon 9 rocket launches from California.

NASA and SpaceX are making final preparations for the Crew-9 astronaut flight to the International Space Station (ISS), which is set to launch from the Kennedy Space Center in Florida on Thursday, September 26.

But this will be the first of SpaceX’s 13 crewed flights to the ISS since the first one in 2020 where there will be two empty seats on the Crew Dragon spacecraft. And there’s a very good reason for that. Let us explain.

Read more
James Webb trains its sights on the Extreme Outer Galaxy
The NASA/ESA/CSA James Webb Space Telescope has observed the very outskirts of our Milky Way galaxy. Known as the Extreme Outer Galaxy, this region is located more than 58 000 light-years from the Galactic centre.

A gorgeous new image from the James Webb Space Telescope shows a bustling region of star formation at the distant edge of the Milky Way. Called, dramatically enough, the Extreme Outer Galaxy, this region is located 58,000 light-years away from the center of the galaxy, which is more than twice the distance from the center than Earth is.

Scientists were able to use Webb's NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument) instruments to capture the region in sparkling detail, showing molecular clouds called Digel Clouds 1 and 2 containing clumps of hydrogen, which enables the formation of new stars.

Read more