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Bradford J. Foley coauthored models coupling planetary cooling, melt production and the carbon cycle on stagnant-lid planets. The model balances volcanic carbon dioxide supply against weathering and tests conditions compatible with a temperate surface.^[ref]

The result makes plate tectonics a physical variable to test in a habitability model, rather than an automatic prerequisite. Initial heat and carbon inventories remain important assumptions.

Chemical weathering alters or dissolves exposed rock and minerals through reactions with water, gases and dissolved substances. The reaction rate depends on mineral composition, temperature, reactive surface area and the supply and removal of fluid. Fracturing can accelerate weathering by exposing fresh surfaces.

In silicate weathering, reactions involving carbon dioxide connect rock alteration with the long-term carbon cycle. The eventual climate effect also depends on transport, carbonate burial and recycling. A classic feedback model links warmer conditions with increased weathering and carbon-dioxide removal; its operation requires suitable rocks and water supply.^[ref]

Plate tectonics changes the environments in which evolution operates: it redistributes habitats, supplies and buries nutrients, and helps regulate climate. It does not prescribe the direction of evolution, and its presence neither guarantees life nor demonstrates that life could not persist under another tectonic regime.

Long-term environmental regulation. Seafloor spreading and subduction exchange material between the mantle, crust, ocean and atmosphere. Volcanism and metamorphism release carbon dioxide, while exposure of fresh silicate minerals by tectonic uplift and erosion can promote chemical weathering. Coupled silicate weathering and carbonate burial remove carbon dioxide from the surface system. In a simplified net reaction,The carbonate-silicate cycle can provide a negative feedback: warming and greater runoff can accelerate silicate weathering, lowering atmospheric carbon dioxide and weakening the greenhouse effect. This requires available fresh rock and liquid water; a supply-limited chemical weathering regime need not respond strongly to warming. Plate tectonics therefore helps sustain some long-lived habitable environments without acting as an infallible thermostat.^[ref]

Nutrients and oxygenation. Tectonic uplift, erosion and hydrothermal circulation supply nutrients such as phosphorus and iron to surface environments. Changes in continental configuration, continental shelf area and ocean circulation alter primary production, nutrient recycling and ocean anoxia. Burial of organic carbon and reduced sulfur can leave an oxidizing surface budget, whereas reduced volcanic gases and freshly exposed reduced rock consume oxidants. Thus plate tectonics can influence atmospheric oxygen and the ecological opportunities for aerobic respiration, but the sign depends on competing fluxes rather than simply on the amount of volcanism.

Geographical isolation and environmental diversity. Continental rifting separates populations, favoring allopatric speciation; continental collision and the emergence of land bridges can reconnect populations, enabling dispersal and competition. Opening or closing ocean gateways changes ocean circulation and heat transport. Mountain building creates elevational habitats and rain shadows; changing continental shelf area changes shallow-water habitat. These processes can promote diversification, eliminate habitats or both. A proposed biological response should be tested against independently dated paleogeography and the fossil record, accounting for unequal preservation.

Abrupt disturbances. Large episodes of volcanism, including a large igneous province, can rapidly perturb the carbon cycle, ocean acidification and ocean anoxia; sulfur dioxide aerosols can instead produce shorter cooling episodes. Such disturbances may cause mass extinction, followed by ecological release and diversification of survivors. A mantle plume need not originate at a plate boundary, so association with a tectonically active planet is not proof that horizontal plate motion directly caused every eruption. The relevant reasoning links a dated geological forcing to its environmental effects and then to biological selectivity, rather than attributing all biological crises to plate tectonics.

Over billions of years, plate tectonics can repeatedly create habitable environments and new selective pressures. Nevertheless, models allow carbon cycling and habitable climate on some stagnant-lid planets. This makes plate tectonics a plausible contributor to sustained environmental diversity, not a demonstrated universal requirement for evolution.^[ref]

The real carbon cycle has multiple reservoirs and adjustment times, rather than one universally exponential removal process. Air-sea exchange, ocean mixing and carbonate chemistry give a long-lived atmospheric tail; uptake also changes with temperature, circulation and carbon loading. For example, a warming ocean can absorb less additional carbon dioxide, so a fixed $b_0$ omits a potentially positive climate-carbon feedback. Terrestrial vegetation and soil responses provide further examples. One missing feature is the dependence of carbon uptake on the changing state of the ocean and climate.

Peter B. Kelemen and Craig E. Manning combined rock carbon inventories, fluid solubility and transport mechanisms to reassess the subduction carbon cycle.^[ref]

Their analysis emphasizes transfer and storage above the descending slab. A carbon atom leaving subducting rock can enter another solid reservoir before reaching the atmosphere; counting only incoming sediment and volcanic output would miss that part of the budget.