scholarly journals Planet Formation in the Outer Solar System

2002 ◽  
Vol 114 (793) ◽  
pp. 265-283 ◽  
Author(s):  
Scott J. Kenyon

Science ◽  
2021 ◽  
Vol 371 (6527) ◽  
pp. 365-370
Author(s):  
Tim Lichtenberg ◽  
Joanna Dra̧żkowska ◽  
Maria Schönbächler ◽  
Gregor J. Golabek ◽  
Thomas O. Hands

Geochemical and astronomical evidence demonstrates that planet formation occurred in two spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We use numerical models to investigate how the evolution of the solar protoplanetary disk influenced the timing of protoplanet formation and their internal evolution. Migration of the water snow line can generate two distinct bursts of planetesimal formation that sample different source regions. These reservoirs evolve in divergent geophysical modes and develop distinct volatile contents, consistent with constraints from accretion chronology, thermochemistry, and the mass divergence of inner and outer Solar System. Our simulations suggest that the compositional fractionation and isotopic dichotomy of the Solar System was initiated by the interplay between disk dynamics, heterogeneous accretion, and internal evolution of forming protoplanets.





1997 ◽  
Author(s):  
R. Lewis ◽  
G. Smith ◽  
B. Dundore ◽  
J. Fulmer ◽  
S. Chakrabarti ◽  
...  


2016 ◽  
Author(s):  
Orkan Umurhan ◽  
◽  
Oliver Luke White ◽  
Alan D. Howard ◽  
Jeffrey Moore


2006 ◽  
Vol 2 (S236) ◽  
pp. 31-34
Author(s):  
E. L. Kiseleva ◽  
V. V. Emel'yanenko

AbstractThe dynamical interrelation between resonant trans-Neptunian objects and short-period comets is studied. Initial orbits of resonant objects are based on computations in the model of the outward transport of objects during Neptune's migration in the early history of the outer Solar system. The dynamical evolution of this population is investigated for 4.5 Gyr, using a symplectic integrator. Our calculations show that resonant trans-Neptunian objects give a substantial contribution to the planetary region. We have estimated that the relative fraction of objects captured per year from the 2/3 resonance to Jupiter-family orbits with perihelion distances q<2.5 AU is 0.4×10−10 near the present epoch.



1969 ◽  
Vol 163 (1 Second Confer) ◽  
pp. 442-452
Author(s):  
J. N. Smith ◽  
C. W. Mead


2016 ◽  
Vol 205 (1-4) ◽  
pp. 213-230 ◽  
Author(s):  
Brenda C. Matthews ◽  
JJ Kavelaars


2001 ◽  
Vol 122 (1) ◽  
pp. 474-481 ◽  
Author(s):  
T. A. Michtchenko ◽  
S. Ferraz-Mello


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