Results 1 to 10 of about 546,735 (346)
Planet Formation in the Outer Solar System [PDF]
This paper reviews coagulation models for planet formation in the Kuiper Belt, emphasizing links to recent observations of our and other solar systems.
Augereau J. C. +20 more
core +7 more sources
Evidence from stable isotopes and 10Be for solar system formation triggered by a low-mass supernova. [PDF]
Banerjee P, Qian YZ, Heger A, Haxton WC.
europepmc +3 more sources
The birth environment of planetary systems [PDF]
Star and planet formation are inextricably linked. In the earliest phases of the collapse of a protostar, a disc forms around the young star and such discs are observed for the first several million years of a star’s life.
Richard J. Parker
doaj +1 more source
Cylindrical molecular filaments are observed to be the main sites of Sunlike star formation, while massive stars form in dense hubs at the junction of multiple filaments.
Doris Arzoumanian +9 more
doaj +1 more source
Magnetic fields in the early solar system may have driven the inward accretion of the protoplanetary disk (PPD) and generated instabilities that led to the formation of planets and ring and gap structures.
Roger R. Fu +5 more
doaj +1 more source
Ocean worlds, or icy bodies in the outer solar system that have or once had subsurface liquid water oceans, are among the most compelling topics of astrobiology.
Kathleen Mandt +3 more
doaj +1 more source
Multiple formation pathways for amino acids in the early Solar System based on carbon and nitrogen isotopes in asteroid Bennu samples. [PDF]
Baczynski AA +11 more
europepmc +2 more sources
Evidence for Enrichment of Niobium-92 in the Outer Protosolar Disk
The short-lived radionuclide, niobium-92 ( ^92 Nb), has been used to estimate the site of nucleosynthesis for p- nuclei and the timing of planetary differentiation, assuming that it was uniformly distributed in the early solar system.
Yuki Hibiya +3 more
doaj +1 more source
The formation and subsequent migration of gas giants could significantly affect the material mixing in the solar system. In this study, we use N -body simulations to investigate how much water is transported into the region of the terrestrial planet ...
Masahiro Ogihara +2 more
doaj +1 more source
We model the early stages of planet formation in the solar system, including continual planetesimal formation, and planetesimal and pebble accretion onto planetary embryos in an evolving disk driven by a disk wind.
John Chambers
doaj +1 more source

