Results 101 to 110 of about 14,974 (190)

Carbon to oxygen ratios in extrasolar planetesimals [PDF]

, 2016
David J. Wilson, B. T. Gänsicke, Jay Farihi, D. Koester   +3 more
openalex   +1 more source

Efficiency of coherent vortices to trap dust particles in the solar nebula

EPJ Web of Conferences, 2013
We develop the idea proposed by Barge & Sommeria (1995) that large-scale vortices present in the solar nebula can concentrate dust particles and facilitate the formation of planetesimals and planets.
Chavanis Pierre-Henri
doaj   +1 more source

Impact of planetesimal eccentricities and material strength on the appearance of eccentric debris disks [PDF]

, 2018
M. Kim, S. Wolf, T. Löhne, Florian Kirchschlager, A. V. Krivov   +4 more
openalex   +1 more source

Conditions of core melt segregation in planetesimals [PDF]

, 2022
Hidenori Terasaki, Takumi Miura, Takashi Yoshino, Tadashi Kondo   +3 more
openalex   +1 more source

Planetesimal Formation in the Warm, Inner Disk: Experiments with Tempered Dust [PDF]

, 2017
Caroline de Beule, Joachim Landers, Soma Salamon, Heiko Wende, Gerhard Wurm   +4 more
openalex   +1 more source

Interstellar planetesimals – II. Radiative instability in dense molecular clouds [PDF]

, 1986
W. M. Napier, C. M. Humphries
openalex   +1 more source

Considering Contact Forces during the Formation of Planetesimals by Gravitational Collapse: Mutual Orbits, Spin States, and Shapes

The Astrophysical Journal
In this work, we apply a soft-sphere discrete element method (SSDEM) within the PKDGRAV N -body integrator to investigate the formation of planetesimal systems through the gravitational collapse of clouds of superparticles. Previously published numerical
Jackson T. Barnes, Stephen R. Schwartz, Seth A. Jacobson   +2 more
doaj   +1 more source

New Evidence for Wet Accretion of Inner Solar System Planetesimals from Meteorites Chelyabinsk and Benenitra

, 2021
Ziliang Jin, Maitrayee Bose, Tim Lichtenberg, Gijs D. Mulders   +3 more
openalex   +1 more source

Gas Pressure Driven Screening Forces and Pebble Aggregation: A Pathway for Growth in Planet Formation

The Astrophysical Journal
The formation of planetesimals from centimeter-sized pebbles in protoplanetary disks faces significant barriers, including fragmentation and radial drift.
Mukesh Kumar Vyas
doaj   +1 more source

Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]

Sci Adv, 2023
Wang W, Walter MJ, Brodholt JP, Huang S, Petaev MI.   +4 more
europepmc   +1 more source