An article published in “The Astrophysical Journal” reports the results of observations of the protoplanetary disk surrounding the very young star TW Hydrae. A team of researchers used observations conducted with the Hubble Space Telescope to examine the ongoing processes and evolution of planetary formation in the system. A protoplanet was identified in 2016 and that had increased the interest in that protoplanetary disk. In 2017, a shadow was identified that indicated the presence of an internal disk inclined relative to the external disk. Now a second shadow appears to come from another disk on the system’s inner side. This means that there may also be another planet in the making.