The team poured over two sets of Magellan radar data obtained in 1990 and 1992 to look for evidence of volcanic activity. In the images, team members found surface changes in two areas, the western flank of Sif Mons, a volcano on Venus, and in western Niobe Planitia, a large volcanic lowland province on the planet. Scientists have previously found volcanic-related features on both of those areas, but the team behind the new study discovered variations in the radar backscatter between different images taken by Magellan over a period of two years. The variations are likely indicative of new lava flows on the surface of Venus, according to the study published in Nature Astronomy.