Mars open-atmosphere terraforming requires exaton-class volatile inventories and sustained multi-100 TW to PW power over centuries, whereas regional paraterraforming is plausible with near-term industry.
Schorghofer, Mars: Quantitative Evaluation of Crocus Melting behind Boulders, ApJ890, 49 (2020)
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Terraforming Mars: Mass, Forcing, and Industrial Throughput Constraints
Mars open-atmosphere terraforming requires exaton-class volatile inventories and sustained multi-100 TW to PW power over centuries, whereas regional paraterraforming is plausible with near-term industry.