REVIEW 3 cited by
Lecture notes on the formation and early evolution of planetary systems
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
These notes provide an introduction to the theory of the formation and early evolution of planetary systems. Topics covered include the structure, evolution and dispersal of protoplanetary disks; the formation of planetesimals, terrestrial and gas giant planets; and orbital evolution due to gas disk migration, planetesimal scattering, planet-planet interactions, and tides.
Forward citations
Cited by 3 Pith papers
-
Re-evaluating solar irradiance reconstructions: No evidence for large secular trends
Recalibrating the CHRONOS and Penza et al. (2024) solar irradiance models against satellite-era TSI removes their claimed 2.1–5.9 W/m² secular trend, leaving changes of roughly 0.1–0.4 W/m².
-
Three-dimensional transport of solids in a protoplanetary disk containing a growing giant planet
3D particle tracking in hydrodynamic disk simulations shows that small dust can cross a giant planet's gap in both directions via meridional gas advection, with the crossing fraction depending on grain size, disk visc...
-
Numerical modeling the mass feeding rates onto accretion-modified stars embedded within AGN disks
Numerical shearing-box simulations provide a broken power-law formula for the suppression of mass feeding onto stars in AGN disks, with a plateau at 88% of the Bondi rate at low thermal mass.
Discussion (0). Continue with ORCID to comment.