from the collapsed lava tubes [29]. The sinuous rille is the most common rille- type feature found on
the lunar surface. Figure 17.4(a) shows an example of a sinuous rille, which is Rima Sharp; its rille
length is around 276 km. The second type is the straight rille, which is formed by tectonic forces.
When a block of crust descends to the valley oor, the surface of the crust separates under exten-
sional forces, which are called graben. The largest straight rille is found in the Oceanus Procellarum,
also known as Ocean of Storms, situated on the near side of what is known as Rima Sirsalis, and
stretches ...
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