Heat Source of Enceladus
Saturn's moon Enceladus has a liquid water ocean beneath its icy outer crust. Because Enceladus is far from the Sun, it receives very little solar energy. Two scientists discuss the primary source of the thermal energy that keeps this subsurface ocean liquid.
Scientist 1
The subsurface ocean is kept warm primarily by tidal heating. As Enceladus orbits Saturn in an elliptical path, the gravitational pull of Saturn and the neighboring moon Dione varies, causing Enceladus to repeatedly stretch and compress. This continuous deformation generates friction within the moon's interior, converting orbital energy into heat. This tidal heating is sufficient to prevent the ocean from freezing.
Scientist 2
The subsurface ocean is kept warm primarily by radiogenic heating (decay of radioactive elements). Enceladus's rocky core contains radioactive isotopes such as uranium, thorium, and potassium. The decay of these isotopes releases a steady supply of heat that warms the core and the ocean above it. Tidal forces are far too weak to generate the amount of heat required to maintain a liquid ocean over billions of years.
Both Scientist 1 and Scientist 2 share which of the following underlying assumptions?
- ATidal forces are too weak to maintain a liquid ocean over billions of years.
- Enceladus must have an active internal source of heat to prevent its subsurface ocean from freezing.Answer
- CRadioactive isotopes are present in the core of all of Saturn's moons.
- DThe surface temperature of Enceladus is warm enough to keep water liquid without internal heating.