I checked the wiki ref but did not really understand the difference between Type I & II migration:-
Type I migration
Terrestrial mass planets drive spiral density waves in the surrounding gas or planetesimal disk. .... This causes the planet to lose angular momentum and the planet then migrates inwards on timescales that are short relative to the million-year lifetime of the disk.
[edit] Type II migration
Planets of more than about 10 Earth masses clear a gap in the disk, ending Type I migration. However, material continues to enter the gap on the timescale of the larger accretion disk, moving the planet and gap inward on the accretion timescale of the disk.
What is this 'timescale of the larger accretion disc', how is material entering the 'gap' (doesn't the protosun/T Tauri clear this or is accretion still running under gravity from the centre? Surely for migration (Type II) to occur, gas density HAS to be high so inflow should be equally 'high'?
Can you explain, please?
roj