Page 4: 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.

Ring around Tabby's star

This illustration shows a hypothetical uneven ring of dust orbiting KIC 8462852, also known as Boyajian's Star or Tabby's Star. The star has experienced unusual dips in brightness over a matter of days, as well as much subtler ...

Learning more about supernovae through stardust

Most of the diverse elements in the universe come from supernovae. We are, quite literally, made of the dust of those long-dead stars and other astrophysical processes. But the details of how it all comes about are something ...

Dying stars could seed interstellar medium with carbon nanotubes

Evidence suggests that carbon nanotubes, tiny tubes consisting of pure carbon, could be forged in the envelopes of dust and gas surrounding dying stars. The findings propose a simple, yet elegant mechanism for the formation ...

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