When the solar system condensed into being 4.6 billion years ago, the nascent Sun radiated at merely three-quarters of its present luminosity. Nevertheless, the sedimentary strata of early Mars —preserved in the planet's ancient cratered highlands—betray no unambiguous signature of planet-wide cryogenic conditions until roughly 3.5 billion years ago. Kasting and Toon proposed in the 1980s that a dense carbon dioxide atmosphere, sustained by pervasive volcanism, trapped sufficient heat to maintain liquid water at the surface. However, subsequent geochemical modeling demonstrated that \(\mathrm{CO}_2\), even at the high partial pressures required, would condense into reflective clouds under the weak early Sun, drastically diminishing its greenhouse efficacy. A growing contingent of planetary scientists now posits that tidal flexure-gravitational kneading of Mars's interior by a then-much-closer moon or passing planetesimals-generated internal frictional heat that kept the subsurface and possibly the surface clement. This tidal-heating hypothesis offers a parsimonious explanation for the abrupt onset of Martian glaciation: around 3.5 billion years ago, orbital perturbations caused the perturbing body to migrate outward, where upon tidal stresses decayed exponentially and the geothermal supplement that had propped up the climate collapsed.
Which of the following best describes the function of the highlighted sentence?
A. It refutes the possibility of a causal connection between two phenomena that earlier theories had treated as interdependent.
B. It indicates how a particular hypothesis can account for the timing of an event mentioned earlier in the passage.
C. It presents evidence that undermines a claim advanced in the opening sentence of the passage.
D. It elucidates a distinction between two competing hypotheses that had previously been conflated.
E. It introduces data that challenge the prevailing explanation for a specific phenomenon.
Which of the following can be inferred from the passage about the tidal heating mechanism on early Mars?
A. The tidal heating mechanism must have ceased to operate entirely after 3.5 billion years ago.
B. The tidal heating mechanism must have produced effects that varied considerably across different latitudes of the Martian surface.
C. The warming generated by tidal flexure would have been more susceptible to diminution by cloud-albedo feedbacks than would warming from a dense \(\mathrm{CO}_2\) atmosphere.
D. The tidal heating mechanism could not have sustained clement surface conditions on early Mars without a contemporaneous \(\mathrm{CO}_2\) greenhouse effect.
E. The tidal heating mechanism would have been less consequential for early Martian climate if the perturbing body had migrated outward significantly earlier than 3.5 billion years ago.