Research news on Circumstellar dust

Circumstellar dust as a research area focuses on the physical, chemical, and dynamical properties of solid particles in the immediate environments of stars, including protoplanetary disks, debris disks, and evolved-star envelopes. Studies address dust grain composition, size distributions, formation and destruction processes, and radiative transfer effects that govern spectral energy distributions and polarization signatures. The field integrates observations from infrared to submillimeter wavelengths with laboratory astrochemistry and dust analog experiments, as well as hydrodynamic and magnetohydrodynamic simulations. It is central to understanding planet formation, disk evolution, stellar mass loss, and the feedback of stellar systems on the interstellar medium.

Webb provides crash course on planet-shattering collisions

In the early history of our solar system, scientists theorize that a Mars-sized object called Theia smashed into the infant Earth, vaporizing massive amounts of rock and blasting it into space. Some of that material coalesced ...

Webb telescope discovers hidden planet in famous star system

Astronomers using NASA's James Webb Space Telescope have discovered a giant planet outside our solar system, called an exoplanet, hiding within one of the most intensely studied planetary systems in the Milky Way galaxy.

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, ...

page 1 from 5