description Serenitatis Basin Overview
The Serenitatis Basin is a substantial impact basin on the Moon’s nearside. Formed by an ancient collision, it's notable for its expansive size and geological features. The Apollo 17 mission conducted extensive studies of its southwestern region, specifically within the Taurus-Littrow valley. Scientists and researchers interested in lunar geology and impact crater formation find this area particularly relevant.
help Serenitatis Basin FAQ
Where on the Moon is the Serenitatis Basin located?
The Serenitatis Basin is a massive, ancient impact crater located in the northeastern region of the Moon's near side. It is easily visible from Earth as the dark, circular Mare Serenitatis (Sea of Serenity).
Did NASA ever send astronauts to the Serenitatis Basin?
Yes, the southwestern edge of the Serenitatis Basin hosted the Apollo 17 mission in December 1972. Astronauts Eugene Cernan and Harrison Schmitt explored the Taurus-Littrow valley in this region, collecting ancient highland rocks.
How big is the Serenitatis Basin?
The Serenitatis Basin is an enormous impact structure, with the visible mare covering a diameter of roughly 700 kilometers. It was formed over 3.8 billion years ago during the Late Heavy Bombardment period.
What did Apollo 17 discover at the Serenitatis Basin?
At the southwestern edge of the basin, Apollo 17 astronauts discovered orange soil near Shorty Crater, which was later identified as tiny beads of volcanic glass. This proved that explosive volcanic activity had once occurred on the Moon.
explore Explore More
Similar to Serenitatis Basin
See all arrow_forward
Reviews & Comments
Write a Review
Be the first to review
Share your thoughts with the community and help others make better decisions.
