The crater Gassendi is 110 km in diameter and located on the northern edge of Mare Humorum at 17.5?S, 39.9?W. Gassendi features an array of intersecting fractures on its floor, collectively known as the Rimae Gassendi. Some of the largest fractures are thousands of meters wide. The origin of these fractures in the floor of Gassendi is not known for certain. After the impact the floor of Gassendi was molten and as it cooled, a crust of solid material formed at the surface. As the entire crater floor continued to cool and settle into its final shape, fractures could have formed due to the forces caused by these changes. This model is rendered with a 3x vertical exaggeration.
Author/Origin: Northeast Planetary Data Center, NASA RPIF System, Seth S Horowitz & Peter H. Schultz
You like Cults and you want to help us continue the adventure independently? Please note that we are a small team of 3 people, therefore it is very simple to support us to maintain the activity and create future developments. Here are 4 solutions accessible to all:
ADVERTISING: Disable your AdBlock banner blocker and click on our banner ads.
DONATE: If you want, you can make a donation via PayPal here.
WORD OF MOUTH: Invite your friends to come, discover the platform and the magnificent 3D files shared by the community!