Results 81 to 90 of about 505 (181)
β Pictoris's well-studied debris disk and two known giant planets, in combination with the stability of the Hubble Space Telescope’s Space Telescope Imaging Spectrograph (HST/STIS) (and now also JWST), offers a unique opportunity to test planet–disk ...
Arin M. Avsar +4 more
doaj +1 more source
Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Wang W +4 more
europepmc +1 more source
Debris disks or exo-Kuiper belts, detected through their thermal or scattered emission from their dusty components, are ubiquitous around main-sequence stars.
Antranik A. Sefilian
doaj +1 more source
Convective Overstability in Radially Global Protoplanetary Disks. I. Pure Gas Dynamics
Protoplanetary disks are prone to several hydrodynamic instabilities. One candidate, convective overstability (COS), can drive radial semiconvection that may influence dust dynamics and planetesimal formation.
Marius Lehmann, Min-Kai Lin
doaj +1 more source
Energy dissipation caused by impact or slow compression of dust aggregates consisting of fibers
In the process of planetesimal formation, the mechanical properties of highly porous dust aggregates play a key role. However, it has not been easy to form highly porous dust aggregates in laboratory experiments.
Shiori Iwano +2 more
doaj +1 more source
GANBISS: a new GPU accelerated N-body code for binary star systems. [PDF]
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
Being one of the most populated mean motion resonances (MMRs) with Neptune and lying close to the inner boundary of the present-day cold classical disk, observations of the orbital and surface class distributions of the plutinos in the 3:2 MMR provide ...
Cameron Collyer +8 more
doaj +1 more source
Simulations of Multiple Dust Ring Formation in a Subsolar-metallicity Protoplanetary Disk
Super-Earths exist around subsolar-metallicity host stars with a frequency comparable to that around solar-metallicity stars, suggesting efficient assembly of dust grains even in metal-deficient environments.
Ryoki Matsukoba +2 more
doaj +1 more source
Organic Matter in the Asteroid Ryugu: What We Know So Far. [PDF]
Potiszil C +8 more
europepmc +1 more source
Imaging of the Vega Debris System Using JWST/MIRI
We present images of the Vega planetary debris disk obtained at 15.5, 23, and 25.5 μ m with the Mid-Infrared Instrument on JWST. The debris system is remarkably symmetric, smooth, and centered accurately on the star.
Kate Y. L. Su +8 more
doaj +1 more source

