Corona in planetary geology refers to a type of geological feature that can be found on the surface of some planets, including Venus and Mars. If you imagine a pancake, with its center pushed up to form a dome shape, that's kind of what a corona looks like.
Coronas are formed by a process called "uplift" – this is when tectonic activity (like the movement of the planet's crust) causes a section of the surface to push upwards. This uplift can create cracks and fissures, which in turn can cause magma to rise up from below the planet's surface.
When the magma reaches the upper layers of the planet's crust, it can create a bulge or dome shape that is characteristic of coronas. Over time, the magma will cool and solidify, creating a permanent geological feature.
Coronas can range in size from a couple of kilometers to hundreds of kilometers in diameter, and they often have concentric rings or ridges around their edges. They can also have distinctive patterns of valleys and ridges on their surfaces, which are thought to be caused by the movement and cooling of the magma.
Scientists study coronas to learn more about the geological processes that shape planets and how these processes work in different environments. By studying coronas on different planets, they can also learn more about the history and evolution of our solar system.