Results 131 to 140 of about 11,561 (252)
Two-source Terrestrial Planet Formation with a Sweeping Secular Resonance
The models that most successfully reproduce the orbital architecture of the solar system terrestrial planets start from a narrow annulus of material that grows into embryos and then planets.
Max Goldberg +2 more
doaj +1 more source
Gas giant formation with small cores triggered by envelope pollution by icy planetesimals [PDF]
Y. Hori, M. Ikoma
openalex +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
A Smoking Gun for Planetesimal Formation: Charge-driven Growth into a New Size Range [PDF]
Jens Teiser +3 more
openalex +1 more source
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
Organic Matter in the Asteroid Ryugu: What We Know So Far. [PDF]
Potiszil C +8 more
europepmc +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
The Composition Of A Disrupted Extrasolar Planetesimal At SDSS\n J0845+2257 (Ton 345) [PDF]
David J. Wilson +6 more
openalex +1 more source
Observing planetesimal formation under streaming instability in the rings of HD 163296 [PDF]
Francesco Zagaria +4 more
openalex +1 more source

