Linking planetesimal and dust content in protoplanetary disks via a local toy model [PDF]
Konstantin Gerbig +2 more
openalex +1 more source
Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Wang W +4 more
europepmc +1 more source
Thousands of planetesimals: Simulating the streaming Instability in very large computational domains [PDF]
Urs Schäfer +3 more
openalex +1 more source
Rapid Timescales for Accretion and Melting of Differentiated Planetesimals Inferred from 26 Al- 26 Mg Chronometry [PDF]
Martin Bizzarro +3 more
openalex +1 more source
Ureilite meteorites provide a new model of early planetesimal formation and destruction [PDF]
Nachiketa Rai, Hilary Downes, CL Smith
openalex +1 more source
Effects of Dust Coagulation on Streaming Instability
Streaming instability (SI) in dust has long been thought to be a promising process in triggering planetesimal formation in the protoplanetary disks (PPDs).
Ka Wai Ho, Hui Li, Shengtai Li
doaj +1 more source
Formation of Super-Earths and Mini-Neptunes from Rings of Planetesimals
The solar system's planetary architecture has been proposed to be consistent with the terrestrial and giant planets forming from material rings at ∼1 au and ∼5 au, respectively.
Sho Shibata, Andre Izidoro
doaj +1 more source
Aqueous breakdown of aspartate and glutamate to n-ω-amino acids on the parent bodies of carbonaceous chondrites and asteroid Ryugu. [PDF]
Li Y +12 more
europepmc +1 more source
I/Pu reveals Earth mainly accreted from volatile-poor differentiated planetesimals. [PDF]
Liu W +5 more
europepmc +1 more source

