The orbital distance at which close-in exoplanets maintain their initial mass is estimated
by modelling the maximum expected nonthermal mass loss rates over several
Gyr. Our results indicate that nonthermal mass loss induced by Coronal Mass Ejections
of a host star can significantly erode weakly magnetized short periodic gas giants.
The observed exoplanets Gliese 876d at 0.0208 AU with a mass of about 0.033
Jupiter masses and 55 Cnc e at 0.045 AU with a mass of about 0.038 Jupiter masses
could be strongly eroded gas giants, while HD69830b, at 0.078 AU, HD160691d at
0.09 AU and HD69830c at 0.18 AU belonged most likely since their origin to the
Neptune-mass domain. The consequences for the planetary population expected to
be discovered with the CoRoTs are: (1) for orbital distances less than about 0.05 AU
weakly magnetized or highly irradiated gas giants may lose a large fraction of their initial
mass and even completely lose their gas envelopes. (2) Observed planetary masses
which resemble theoretically calculated planetary mass spectra at these orbital periods
would indicate a major effect of magnetic field protection. (3) At distances larger than
0.05 AU the impact of loss processes for Hot Jupiters is minor and the observed mass
spectra should be close to the theoretical ones.