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 from the host star. There are gaps at and, with bright rings at and.
In 1998, Rainer Wichmann et al. announced that the star, then known as RXJ1608.6-3922, is a variable star, based on visual band photometry over a nine day interval. They classified it as an eclipsing binary. Later observations showed that the brightness variations are due to starspots. It was given its variable star designation in the year 2000.
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 Currently, the presence of a substellar object has been retracted; again starspots have been invoked as the actual cause for observed radial velocity variations.