Research news on Protoplanetary disks

Protoplanetary disks as a research area encompass the observational, theoretical, and computational study of gas- and dust-rich disks surrounding young stellar objects, which serve as the birthplaces of planets. This field investigates disk structure, composition, thermochemistry, angular momentum transport, and disk evolution through processes such as accretion, turbulence, magnetohydrodynamic effects, dust growth, and planet–disk interactions. Research integrates multiwavelength observations (e.g., ALMA, infrared spectroscopy) with radiative transfer, hydrodynamical, and chemical modeling to constrain disk lifetimes, mass budgets, and conditions for planet formation, as well as to link disk properties to emerging planetary system architectures and demographics.

Young giant gas planet Beta Pic B refuses to reveal its origin

The young planetary system of the 23-million-year-old star Beta Pictoris (short: Beta Pic) is regarded as an iconic circumstellar dust disk, which hosts at least three giant gas planets. Discovered in 2008 by direct imaging, ...

Nautilus array to track missing exoplanet atmospheres

Exoplanet atmospheres have become prime targets for astrobiologists in the search for life beyond Earth. This is because exoplanet surfaces can't be directly imaged yet, so astronomers must get creative in how they search ...

Longest-period young transiting exoplanets discovered

It's 2234, you're on your annual class field trip touring exoplanets, and your teacher informs everyone they can pick one more exoplanetary system to explore before heading back to Earth. You and your classmates are exhausted ...

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