Thermal instability triggers cyclic MRI activity in protoplanetary disks, enabling dust self-accumulation and planetesimal formation near 1 au with enough mass for multiple super-Earths.
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3 Pith papers cite this work. Polarity classification is still indexing.
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A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
Proposes AMBITION, a cryogenic comet nucleus sample return mission, to address open questions in cometary science that require Earth laboratory techniques after the Rosetta mission.
citing papers explorer
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Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks
Thermal instability triggers cyclic MRI activity in protoplanetary disks, enabling dust self-accumulation and planetesimal formation near 1 au with enough mass for multiple super-Earths.
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A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks
A new Monte Carlo method for dust coagulation ensures global conservation of dust properties and improves small-grain resolution in protoplanetary disk simulations.
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AMBITION -- Comet Nucleus Cryogenic Sample Return (White paper for ESA's Voyage 2050 programme)
Proposes AMBITION, a cryogenic comet nucleus sample return mission, to address open questions in cometary science that require Earth laboratory techniques after the Rosetta mission.