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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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.