... mass as Saturn instead of some Jupiter masses.” Despite these positive results, challenges still remain. Simulations of disk instability still do not cover a long enough timescale and it is possible that after the protoplanet has collapsed to the...
...’t see any of these features. We saw a well-defined, almost symmetric disk made of concentric rings,” says Hales. If disc instability is not the cause of the cavities in HL Tau, then perhaps the gaps are the result of a self-induced...