The planet candidates, on the other hand, reside
at orbital radii around 15 au, where disk observations have been unreliable until recently.
Not exact matches
They eliminated those with
orbital radii less than one tenth that of Earth's, because
at that distance moon systems might not remain in stable orbits around their planets on billion - year timescales.
A simulation (Wolf & D'Angelo 2005) of ALMA observations
at 950 GHz of a disc shows an embedded protoplanet of 1 Jupiter Mass around a 0.5 Solar Mass star (
orbital radius: 5AU).
We find that 16.5 + / - 3.6 % of main - sequence FGK stars have
at least one planet between 0.8 and 1.25 Earth
radii with
orbital periods up to 85 days.