Astronomers debate the origin of water on the Moon. Three viewpoints are proposed:
Viewpoint 1 (Asteroid Delivery): Water was delivered to the Moon post-formation via impacts from carbonaceous chondrite asteroids. This water has a high deuterium-to-hydrogen () ratio of approximately .
Viewpoint 2 (Earth Mantle Heritage): The Moon inherited its water directly from Earth’s mantle during the giant impact that formed the Moon. This water has a low ratio of approximately and is locked deep within the lunar mantle.
Viewpoint 3 (Solar Wind Implantation): Water () and hydroxyl () are continuously produced on the surface when solar wind protons () impact oxygen-rich minerals in the lunar regolith (soil). This process only affects the exposed outermost layer of the soil.
Match each of the following new findings to the viewpoint that it directly supports.
- Deep lunar mantle minerals contain water with a ratio of .Supports Viewpoint 2 (Earth Mantle Heritage)
- Water ice deposits in polar craters show a ratio of .Supports Viewpoint 1 (Asteroid Delivery)
- Hydroxyl groups are detected only in the top millimeters of lunar regolith exposed to solar radiation.Supports Viewpoint 3 (Solar Wind Implantation)