Problems
1. Mercury's Moment of Inertia and Core Size 15 points
MESSENGER measurements give Mercury's moment of inertia factor as C/MR² = 0.346. Compute its percent deviation below the uniform-sphere value of 0.4, and compare this deviation to Earth's (17.3% computed from C/MR² = 0.3307). State what this comparison implies about Mercury's core, in light of Lecture 03's giant-impact hypothesis for Mercury's anomalously large core.
2. Radiogenic Heat Production 2 Gyr Ago 15 points
Using the decay constants λ = ln2/t₁⁄² for ⁴⁴K (t₁⁄² = 1.25 Gyr) and ²³⁶U (t₁⁄² = 4.47 Gyr), compute what fraction of each isotope's present-day abundance existed 2 Gyr ago (i.e., the ratio of abundance at t = -2 Gyr relative to today, noting this ratio is e⁺λt for t = 2 Gyr since we are looking backward in time). Explain which isotope's heat contribution changed more dramatically over this interval and why.
3. Surface-to-Volume Scaling for Io versus the Moon 15 points
Io (radius 1821.6 km) and the Moon (radius 1737.4 km) are nearly the same size, yet Io is the most volcanically active body in the solar system while the Moon is essentially geologically dead. Using the surface-to-volume cooling argument from Lecture 04, explain why this argument alone would predict similar (low) geological activity for both bodies, and then explain what additional physical mechanism (introduced in Lecture 04 as a preview and developed fully in Lecture 13) resolves this apparent contradiction.
4. Rayleigh Number Scaling 15 points
The Rayleigh number is Ra = (ρgαΔTd³)/(κμ). If a planet's mantle thickness d were doubled while all other quantities (ρ, g, α, ΔT, κ, μ) stayed fixed, by what factor would its Rayleigh number change? Given that Earth's mantle Rayleigh number is estimated at 10⁶-10⁷, vastly above the critical value of ∼1000-2000, would this change plausibly push a convecting mantle below the critical threshold into a non-convecting regime? Justify your answer quantitatively.
5. Comparing Bulk Silicate Earth's Heat Budget to Observed Heat Flow 15 points
Earth's present-day radiogenic heat production is estimated at roughly 20 TW, while its total observed surface heat flow is roughly 47 TW. Compute the percent of Earth's total heat flow that is NOT accounted for by present-day radiogenic heat production, and explain, using the concept introduced in Lecture 04, what additional heat source is thought to make up this difference.