These are the sharpest images yet of planets being born around distant stars
ALMA observations of carbon monoxide emission from 15 protoplanetary disks reveal a stunning variety of gas structures, including gaps, rings and spirals.
Get the world’s most fascinating discoveries delivered straight to your inbox.
You are now subscribed
Your newsletter sign-up was successful
Want to add more newsletters?
Delivered Daily
Daily Newsletter
Sign up for the latest discoveries, groundbreaking research and fascinating breakthroughs that impact you and the wider world direct to your inbox.
Once a week
Life's Little Mysteries
Feed your curiosity with an exclusive mystery every week, solved with science and delivered direct to your inbox before it's seen anywhere else.
Once a week
How It Works
Sign up to our free science & technology newsletter for your weekly fix of fascinating articles, quick quizzes, amazing images, and more
Delivered daily
Space.com Newsletter
Breaking space news, the latest updates on rocket launches, skywatching events and more!
Once a month
Watch This Space
Sign up to our monthly entertainment newsletter to keep up with all our coverage of the latest sci-fi and space movies, tv shows, games and books.
Once a week
Night Sky This Week
Discover this week's must-see night sky events, moon phases, and stunning astrophotos. Sign up for our skywatching newsletter and explore the universe with us!
Join the club
Get full access to premium articles, exclusive features and a growing list of member rewards.
Astronomers have captured the sharpest, most detailed images yet of young solar systems where planets are just beginning to take shape.
Exquisite snapshots released on April 28 provide a rare glimpse into the earliest stages of planet formation in more than a dozen star systems, revealing where planets emerge, how quickly they form and what materials they're made from. Scientists say the data could help refine computer models of planetary formation and evolution, as well as shed new light on how these infant systems compare to the myriad of mature exoplanets already discovered.
The high-resolution, science-packed images come thanks to advanced imaging techniques courtesy of the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile. These techniques reduce distortions and sharpen clarity, boosting astronomers' ability to map out the planet formation process with greater precision by revealing finer structures within the protoplanetary disks — the swirling gas and dust surrounding young stars, according to a statement.
The newly developed techniques "are like switching from reading glasses to high-powered binoculars," Richard Teague of the Massachusetts Institute of Technology, who serves as the principal investigator of the project, said in the statement. "They reveal a whole new level of detail in these planet-forming systems."
Using ALMA, Teague's team captured images of 15 young star systems sprinkled in space between a few hundred to 1,000 light-years from Earth. Rather than rely on direct detection of a young planet's faint light, Teague's team looked for the subtle clues these infant worlds imprint on their surroundings — such as gaps and rings in dusty disks, swirling gas motions caused by a planet's gravity, and other physical disturbances that hint at a planet's presence. To uncover these signatures, the researchers used ALMA to map the motion of gas within over a dozen protoplanetary disks.
"It's like trying to spot a fish by looking for ripples in a pond, rather than trying to see the fish itself," Christophe Pinte, an astrophysicist at the Institute for Planetary sciences and Astrophysics in France, who was also a principal investigator of the project, said in the statement.
Initial analysis of the images, detailed in 17 newly published papers, clearly shows that these protoplanetary disks with still-forming planets are highly dynamic, chaotic places that already harbor complex structures, the team says.
Get the world’s most fascinating discoveries delivered straight to your inbox.
Among the key findings are fresh insights into how large dust grains are gathered into rings — precursors to planets — and subtle signs of the disks' gravitational influence, providing astronomers with a new way to gauge the mass available for forming planets.
"We're seeing evidence of hugely perturbed and dynamic disks, highly suggestive of young planets shaping the disks they're born in," Teague said.A particularly notable aspect of the project, according to the research team, is that early-career scientists took the lead — authoring 12 of the 17 published papers, with more expected to follow later this year.
Originally posted on Space.com.

Sharmila Kuthunur is an independent space journalist based in Bengaluru, India. Her work has also appeared in Scientific American, Science, Astronomy and Space.com, among other publications. She holds a master's degree in journalism from Northeastern University in Boston. Follow her on BlueSky @skuthunur.bsky.social
You must confirm your public display name before commenting
Please logout and then login again, you will then be prompted to enter your display name.
