TW Hydrae (TW Hya) is the nearest T-Tauri star to the Sun,
and is the star for which TW Hydrae association is named.
It has a face-on protoplanetary disk that includes a gap.
Such a gap suggests a likely extra-solar planet, which would be TW Hydrae b,
with a mass of up to about 1.5 Neptune masses, i.e.,
roughly 25 Earth masses. (A discounted study had
theorized a more massive planet based on other arguments.)
Characteristics: