An independent Bayesian analysis from proper motion measurements results in a 87 % probability that this free - floating
planet is a member of the 50 - 120
Myr old AB Doradus moving group, which strengthens the spectroscopic youth diagnosis.
We observed and spatially resolved the disk around the ~ 10
Myr old protoplanetary disk HD 100453 in polarized scattered light with SPHERE / VLT at optical and near - infrared wavelengths, reaching an angular resolution of ~ 0.02», and an inner working angle... ▽ More Understanding the diversity of
planets requires to study the morphology and the physical conditions in the protoplanetary disks in which they form.