Impact of planetesimal eccentricities and material strength on the appearance of eccentric debris disks [PDF]
, 2018 M. Kim +4 more
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Planetesimal formation in turbulent circumstellar disks [PDF]
, 2010 David Robert Kirsh, Ralph E. Pudritz
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Argon in β Pictoris–Entrapment and Release of Volatile in Disks
The Astrophysical JournalChemical compositions of planets reveal much about their formation environments. Such information is well sought-after in studies of solar system bodies and extrasolar ones.
Yanqin Wu +3 more
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Vom Staubkorn zum Planetesimal [PDF]
Physik in unserer Zeit, 2019 ZusammenfassungDurch astronomische Beobachtungen, numerische Simulationen und Laborexperimente sind wir erstmals in der Lage, ein in sich geschlossenes Bild der Entstehung der ersten größeren Körper in jungen Planetensystemen zu zeichnen. Mikroskopisch kleine Staubpartikel verklumpen durch haftende Stöße zu millimeter‐ bis zentimetergroßen Agglomeraten.
openaire +1 more source
Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall
The Astrophysical JournalThere is growing evidence that planet formation begins early, within the ≲1 Myr Class 0/I phase, when infall dominates disk dynamics. Our goal is to determine if Class 0/I disks reach the conditions needed to form planetesimals (∼100 km planet building ...
Daniel Carrera +7 more
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Thermal evolution and sintering of chondritic planetesimals IV. Temperature dependence of heat conductivity of asteroids and meteorites [PDF]
, 2018 H. P. Gail, M. Trieloff
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Interstellar planetesimals – II. Radiative instability in dense molecular clouds [PDF]
, 1986 W. M. Napier, C. M. Humphries
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Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion [PDF]
, 2017 S. Raymond, A. Izidoro
semanticscholar +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
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