V1094 Scorpii

V1094 Scorpii is a young stellar object in the constellation of Scorpius, located in the young Lupus Star Forming Region. It is being orbited by a protoplanetary disk that extends out to a distance of $300 AU$ from the host star. There are gaps at $100 AU$ and $170 AU$, with bright rings at $130 AU$ and $220 AU$.

Periodic radial velocity variations in the young star V1094 Scorpii had at first been explained by the presence of a substellar object in a tight orbit. Currently, the presence of a substellar object has been retracted, invoking starspots as the actual cause for observed radial velocity variations.