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Planets Forming in Disk Around Young Star

· By Josh Universe · 5 min read

A solar system in the making? Two planets spotted forming in disk around young star

by ESO

edited by Stephanie Baum, reviewed by Robert Egan

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A Solar System in the making? Two planets spotted forming in disc around young star
These images, taken with ESO's Very Large Telescope (VLT), show a planetary system being born around the young star WISPIT 2. The star is surrounded by a disc of gas and dust –– the raw material out of which planets form and grow. In 2025 a team of astronomers detected a young planet, called WISPIT 2b, carving out a gap in the disc around the star. Now the same team has confirmed the presence of a second planet, WISPIT 2c, orbiting even closer to the star, as shown in the inset. Both planets are gas giants, similar to Jupiter. WISPIT 2b is almost five times as massive as Jupiter, and orbits the star at a distance 60 times larger than the separation between Earth and the Sun. WISPIT 2c is twice as massive as 2b and orbits the star four times closer. The images shown here were taken with the SPHERE instrument at the VLT. SPHERE can correct the blur caused by atmospheric turbulence, as well as block the light of the central star, revealing the faint disc and planets around it in great detail. A different instrument, GRAVITY+ on the VLT Interferometer, was also used in the discovery, helping confirm the planetary nature of the observed object. Credit: ESO/C. Lawlor, R. F. van Capelleveen et al.

Astronomers have observed two planets forming in the disk around a young star named WISPIT 2. Having previously detected one planet, the team has now employed European Southern Observatory (ESO) telescopes to confirm the presence of another. These observations, and the unique structure of the disk around the star, indicate that the WISPIT 2 system could resemble a young solar system.

"WISPIT 2 is the best look into our own past that we have to date," says Chloe Lawlor, Ph.D. student at the University of Galway, Ireland, and lead author of the study published in The Astrophysical Journal Letters.

The system is only the second known, after PDS 70, where two planets have been directly observed in the process of forming around their host star. Unlike PDS 70, however, WISPIT 2 has a very extended planet-forming disk with distinctive gaps and rings.

"These structures suggest that more planets are currently forming, which we will eventually detect," Lawlor says.

"WISPIT 2 gives us a critical laboratory not just to observe the formation of a single planet but an entire planetary system," says Christian Ginski, study co-author and researcher at the University of Galway.

With such observations, astronomers aim to better understand how baby planetary systems develop into mature ones, like our own.

The first newborn planet found in the system—named WISPIT 2b—was detected last year, with a mass almost five times that of Jupiter and orbiting the central star at around 60 times the distance between Earth and the sun.

"This detection of a new world in formation really showed the amazing potential of our current instrumentation," said Richelle van Capelleveen, Ph.D. student at Leiden Observatory, the Netherlands, and leader of the previous study.

After an additional object was identified near the star, measurements made with ESO's Very Large Telescope (VLT) and the VLT Interferometer (VLTI) confirmed its planetary nature. The new planet—WISPIT 2c—is four times closer to the central star and is twice as massive as WISPIT 2b. Both planets are gas giants, like the outer planets in our solar system.

To confirm the existence of WISPIT 2c, the team employed the SPHERE instrument on ESO's VLT, which captured an image of the object. The team then used the GRAVITY+ instrument on the VLTI to confirm that the object was indeed a planet.

"Critically, our study made use of the recent upgrade to GRAVITY+, without which we would not have been able to get such a clear detection of the planet so close to its star," says Guillaume Bourdarot, study co-author and researcher at the Max Planck Institute for Extraterrestrial Physics, Garching, Germany.

Both planets in WISPIT 2 appear in clear gaps within the disk of dust and gas circling the young star. These gaps result from each planet's development: particles in the disk accumulate, their gravity pulling in more material until an embryo planet forms. The remaining material, around each gap, creates distinctive dust rings in the disk.

Besides the gaps in which the two planets were found, there is at least one smaller gap farther out in the WISPIT 2 disk.

"We suspect there may be a third planet carving out this gap," says Lawlor, "potentially of Saturn mass, owing to the gap being much narrower and shallower."

The team is eager to make follow-up observations, with Ginski noting, "With ESO's upcoming Extremely Large Telescope, we may be able to directly image such a planet."

Publication details

Chloe Lawlor et al, Direct spectroscopic confirmation of the young embedded proto-planet WISPIT 2c, The Astrophysical Journal Letters (2026). www.eso.org/public/archives/re … eso2604/eso2604a.pdf

Journal information: Astrophysical Journal Letters

Key concepts

Exoplanet systems Protoplanetary disks

Provided by ESO

Citation: A solar system in the making? Two planets spotted forming in disk around young star (2026, March 24) retrieved 24 March 2026 from https://phys.org/news/2026-03-solar-planets-disk-young-star.htmlThis document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.0 shares

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Updated on Mar 24, 2026