Results 161 to 170 of about 4,639 (216)
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.
openaire +1 more source
Models and observational predictions of dust traps in protoplanetary discs. [PDF]
Pinilla P.
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]
Schönbächler M +3 more
europepmc +1 more source
Provenance and distribution of zinc in terrestrial planets. [PDF]
Martins R +4 more
europepmc +1 more source
Understanding the Formation of Saturn's Regular Moons in the Context of Giant Planet Moons Formation Scenarios. [PDF]
Blanc M +9 more
europepmc +1 more source
Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]
Lagrange AM +28 more
europepmc +1 more source
Origin of compact exoplanetary systems during disk infall. [PDF]
Rufu R, Canup RM.
europepmc +1 more source
Improvement of merging processes in N-body simulations in circumstellar disks
Zimmermann M, Pilat-Lohinger E.
europepmc +1 more source
Earth's core-mantle differentiation shaped by water. [PDF]
Luo H, Zheng D, Deng J.
europepmc +1 more source

