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Comets may have transported water to a young planetary system

Today’s Picture of the Week tells a story of redemption for one lonely star. The young star MP Mus (PDS 66) was thought to be all alone in the Universe, surrounded by nothing but a featureless band of gas and dust called a protoplanetary disc. In most cases, the material inside a protoplanetary disc condenses to form new planets around the star, leaving large gaps where the gas and dust used to be. These features are seen in almost every disc — but not in MP Mus’s. When astronomers first observed it with the Atacama Large Millimeter/submillimeter Array (ALMA), they saw a smooth, planet-free disc, shown here in the right image. The team, led by Álvaro Ribas, an astronomer at the University of Cambridge, UK, gave this star another chance and re-observed it with ALMA at longer wavelengths that probe even deeper into the protoplanetary disc than before. These new observations, shown in the left image, revealed a gap and a ring that had been obscured in previous observations, suggesting that MP Mus might have company after all. Meanwhile, another piece of the puzzle was being revealed in Germany as Miguel Vioque, an astronomer at ESO, studied this same star with the European Space Agency’s (ESA’s) Gaia mission. Vioque noticed something suspicious — the star was wobbling. A bit of gravitational detective work, together with insights from the new disc structures revealed by ALMA, showed that this motion could be explained by the presence of a gas giant exoplanet.  Both teams presented their joint results in a new paper published in Nature Astronomy. In what they describe as “a beautiful merging of two groups approaching the same object from different angles”, they show that MP Mus isn’t so boring after all. Link Research paper in Nature Astronomy

Astronomers at Lund University in Sweden have found evidence of exocomets – comets in other solar systems – orbiting a young star similar to our Sun. The observations point to a possible mechanism for how water might be transported from the cold outer regions of the planetary system to regions where planets form.

The PDS 70 planetary system is just over five million years old and lies around 370 light-years from Earth. The system has at least two gas giants and orbits a star that is slightly cooler than the Sun. Water vapour was detected near the star as early as 2023. Researchers in Lund have now shown that variations in sodium gas in front of the star may be a sign of comets passing through the inner parts of the system.

“Our study suggests that comets may be responsible for transporting water to the inner parts of the planetary system, where planets can form, in the same way as in the early Solar System,” says Aline Novais, an astronomy researcher at Lund University.

The researchers have analysed observations from 2018 and detected sodium gas moving at several kilometres per second relative to the star. The gas appears and disappears over the course of several nights – a pattern consistent with what one would expect when comets pass in front of a star. When a comet approaches its star, it heats up and the ice on its surface turns directly into gas – a process known as sublimation. The gas can then leave a measurable imprint in the star’s light.

“This is the first time we have seen evidence of exocomets orbiting a star that is relatively cool, much like our Sun. Furthermore, this system is the youngest in which exocomet activity has been proposed,” says Aline Novais.

The researchers have also simulated the comets’ orbits. The results show that objects far out in the planetary system can be affected by the gravitational pull of the gas giants and flung towards the star. This is particularly interesting because comets form in the cold outer regions of the planetary system, where water may exist as ice. If they are then channelled inwards, they can transport water and other volatile substances to the region where planets form.

“It is reminiscent of a possible process in the early Solar System, in which comets may have helped to deliver water to the young Earth,” says Alexandra Stockwell Murphy, an astronomer at Lund University.

Where the Earth’s water originally came from remains an open question. Water-rich asteroids and comets are two possible sources. PDS 70 gives researchers the opportunity to study a similar process whilst a planetary system is still in its early stages of development.

“And when the Extremely Large Telescope, which is currently being built in Chile, becomes operational in the coming years, we will be able to find out whether there are any further planets in the system and thus gain an even clearer picture of how water and other building blocks of planets are transported,” concludes Jens Hoeijmakers, an astronomy researcher at Lund University.


Journal: Nature Communications
DOI: 10.1038/s41467-026-76880-y
Article Title: Potential sublimating exocomets around the young star PDS 70
Publication Date: 24-Aug-2026
Institution: Lund University

Source: EurekAlert | Featured image credit: ALMA (ESO/NAOJ/NRAO)/A. Ribas et al.

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