### Heat Source of Enceladus
Scientists debate the primary heat source maintaining the subsurface liquid water ocean on Saturn's moon, Enceladus.
Hypothesis 1
The liquid ocean is maintained primarily by tidal heating. Gravitational interactions with Saturn and other moons deform Enceladus, generating frictional heat within its silicate core and ice shell. Frictional heating in the core is highly localized and can produce temperatures exceeding .
Hypothesis 2
The liquid ocean is maintained primarily by radiogenic heating. The decay of radioactive isotopes (such as Uranium-235 and Potassium-40) in the moon's rocky core releases steady, uniform thermal energy. This decay is estimated to produce maximum core-mantle boundary temperatures of approximately .
New Evidence
Analysis of the water plumes erupting from Enceladus's south polar region reveals the presence of silica nanoparticles (). Laboratory experiments show that these nanoparticles can only form when alkaline water containing dissolved silica is heated to at least at the seafloor.
Which of the following statements best describes how this new evidence affects Hypotheses 1 and 2?
- It weakens Hypothesis 2 because radiogenic heating cannot generate the minimum temperature required to form the silica nanoparticles, and it supports Hypothesis 1 because tidal heating can produce these temperatures.Answer
- BIt supports Hypothesis 2 because radiogenic decay generates the steady, uniform temperatures required to synthesize silica nanoparticles, and it weakens Hypothesis 1.
- CIt weakens both Hypothesis 1 and Hypothesis 2 because the presence of silica nanoparticles implies the ocean is composed of liquid methane rather than water.
- DIt has no effect on either Hypothesis 1 or Hypothesis 2 because silica nanoparticles can only form at temperatures below , which both hypotheses can easily produce.