
New 3D Maps of Venus’s Coronae Point to a More Active Interior
Using decades-old Magellan data, researchers built new 3D models of Venus’s largest coronae and found evidence that multiple plume-driven processes may be shaping the planet’s surface.
- Researchers modeled Venus’s largest coronae using Magellan radar, gravity and topographic data.
- The team says coronae vary too much to come from one formation mechanism.





