Results 111 to 120 of about 832 (184)

Stochastic accretion of the Earth. [PDF]

Nat Astron, 2022
Sossi PA, Stotz IL, Jacobson SA, Morbidelli A, O'Neill HSC.   +4 more
europepmc   +1 more source

Petrologic evidence for core sulfur degassing in partially differentiated planetesimals. [PDF]

Sci Adv
Wang SZ, Zhang AC, Du TT, Chen J, Wen Y, Lu X.   +5 more
europepmc   +1 more source

Planetary population synthesis and the emergence of four classes of planetary system architectures. [PDF]

Eur Phys J Plus, 2023
Emsenhuber A, Mordasini C, Burn R.
europepmc   +1 more source

Experimental evidence for granular shear-flow instability in the Epstein regime. [PDF]

Commun Phys
Capelo HL, Bodénan JD, Jutzi M, Kühn J, Surville C, Mayer L, Schönbächler M, Alibert Y, Thomas N, Pommerol A.   +9 more
europepmc   +1 more source

Interstellar ices as carriers of supernova material to the early solar system. [PDF]

Nat Commun
Bizzarro M, Schiller M, Holst J, Bouvier L, Groen M, Moynier F, van Kooten EMME, Schönbächler M, Haugbølle T, Watson D, Johansen A, Connelly JN, Bizzarro E.   +12 more
europepmc   +1 more source

Models and observational predictions of dust traps in protoplanetary discs. [PDF]

Astrophys Space Sci
Pinilla P.
europepmc   +1 more source

Occultation constraints on solar system formation models. [PDF]

Philos Trans A Math Phys Eng Sci
Buie MW, Keller JM, Nesvorný D, Porter SB.   +3 more
europepmc   +1 more source

Initial Conditions of Planet Formation: Time Constraints from Small Bodies and the Lifetime of Reservoirs in the Solar Protoplanetary Disk. [PDF]

Space Sci Rev
Schönbächler M, Bouvier A, Kita NT, Kruijer TS.   +3 more
europepmc   +1 more source

Provenance and distribution of zinc in terrestrial planets. [PDF]

Sci Rep
Martins R, Morton EM, Huang Y, Williams HM, Rehkämper M.   +4 more
europepmc   +1 more source

Density of planetesimals

Density of planetesimals
Pressure density relation of powder near the percolation threshold is investigated from percolation theory to find the density of planetesimal. It is shown that the density of a planetesimal is estimated to be 0.2 g/cu cm.
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