Young Star HD 135344B: Newborn planet sculpting dust around it | ESO
This image shows the dusty disc around the young star HD 135344B. It is a combination of data taken with two facilities: the Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) instrument at the European Southern Observatory’s VLT in red, and the Atacama Large Millimeter/submillimeter Array (ALMA) in orange and blue. The original SPHERE and ALMA images were released in 2016 and 2015 respectively and did not show evidence for the presence of a planet in this disc, first revealed in 2025.
This image, taken with the Atacama Large Millimeter/submillimeter Array (ALMA), and first released in 2015, shows a planet-forming disc around the young star HD 135344B. The image combines a view of the gas (blue) and the dust (orange) around the star. The star itself is invisible at these wavelengths, and is located in the central gap of the disc.
This image from the Digitized Sky Survey (DSS) shows the region of the sky around the star HD 135344B. Right at the center of the image there are two bright stars close to each other; HD 135344B is the one at the bottom.
Astronomers may have caught a still-forming planet in action, carving out an intricate pattern in the gas and dust that surrounds its young host star. Using the European Southern Observatory’s Very Large Telescope (VLT), they observed a planetary disc with prominent spiral arms, finding clear signs of a planet nestled in its inner regions. This is the first time astronomers have detected a planet candidate embedded inside a disc spiral.
“We will never witness the formation of Earth, but here, around a young star 440 light-years away, we may be watching a planet come into existence in real time,” says Francesco Maio, a doctoral researcher at the University of Florence, Italy, and lead author of this study, published today in Astronomy & Astrophysics.
The potential planet-in-the-making was detected around the star HD 135344B within a disc of gas and dust around it called a protoplanetary disc. The budding planet is estimated to be twice the size of Jupiter and as far from its host star as Neptune is from the Sun. It has been observed shaping its surroundings within the protoplanetary disc as it grows into a fully formed planet.
Protoplanetary discs have been observed around other young stars, and they often display intricate patterns, such as rings, gaps or spirals. Astronomers have long predicted that these structures are caused by baby planets that sweep up material as they orbit around their parent star. However, until now, they had not caught one of these planetary sculptors in the act.
In the case of HD 135344B’s disc, swirling spiral arms had previously been detected by another team of astronomers using Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE), an instrument on ESO’s VLT. However, none of the previous observations of this system found proof of a planet forming within the disc.
Now, with observations from the new VLT’s Enhanced Resolution Imager and Spectrograph (ERIS) instrument, the researchers say they may have found their prime suspect. The team spotted the planet candidate right at the base of one of the disc’s spiral arms, exactly where theory had predicted they might find the planet responsible for carving such a pattern.
“What makes this detection potentially a turning point is that, unlike many previous observations, we are able to directly detect the signal of the protoplanet, which is still highly embedded in the disc,” says Maio, who is based at the Arcetri Astrophysical Observatory, a centre of Italy’s National Institute for Astrophysics (INAF). “This gives us a much higher level of confidence in the planet’s existence, as we’re observing the planet’s own light.”
A star’s companion is born
Another team of astronomers have also recently used the ERIS instrument to observe another star, V960 Mon, one that is still in the very early stages of its life. In a study published on July 18, 2025, in The Astrophysical Journal Letters, the team report that they have found a companion object to this young star. The exact nature of this object remains a mystery.
The new study, led by Anuroop Dasgupta, a doctoral researcher at ESO and at the Diego Portales University in Chile, follows up observations of V960 Mon made a couple of years ago. Those observations, made with both SPHERE and the Atacama Large Millimeter/submillimeter Array (ALMA), revealed that the material orbiting V960 Mon is shaped into a series of intricate spiral arms. They also showed that the material is fragmenting, in a process known as ‘gravitational instability’, when large clumps of the material around a star contract and collapse, each with the potential to form a planet or a larger object.
“That work revealed unstable material but left open the question of what happens next. With ERIS, we set out to find any compact, luminous fragments signalling the presence of a companion in the disc—and we did,” says Dasgupta. The team found a potential companion object very near to one of the spiral arms observed with SPHERE and ALMA. The team say that this object could either be a planet in formation, or a ‘brown dwarf’—an object bigger than a planet that did not gain enough mass to shine as a star.
If confirmed, this companion object may be the first clear detection of a planet or brown dwarf forming by gravitational instability.
Credit: ESO/T. Stolker et al./ALMA (ESO/NAOJ/NRAO)/N. van der Marel et al./ESO/Digitized Sky Survey 2
Acknowledgement: D. De Martin
Release Date: July 21, 2025
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