Extended Data Fig. 3: Baseline crustal production rate adopted in this study. | Nature Geoscience

Extended Data Fig. 3: Baseline crustal production rate adopted in this study.

From: A nitrogen-rich atmosphere on ancient Mars consistent with isotopic evolution models

Extended Data Fig. 3

(a) Crustal production rates derived from the photogeologic analysis of volcanic provinces57 from 3.8 Ga. To convert the photogeological analysis (expressed as the total volcanic emplacement in each geologic period from middle Noachian to late Amazonian) to the crustal production rate, we compare the rates derived using the age boundaries from the crater density65 and the chronology model of Ivanov (2001)66 and Hartmann (2005)67, as well as interpolation methods using either step functions or mid-point averages. The labels show the total volcanic activity and the integrated volcanic activity in the last 2 billion years (in parentheses). The midpoint approach would introduce substantially more total volcanism, and so we use the step-function approach. Also in comparison is a volcanic history derived from earlier photogeologic analyses and used in the recent argon isotope study15. The step-function approach on the Hartmann (2015) chronology leads to a baseline model that is very similar to the one used in the argon isotope study15 in terms of the total and the recent volcanic rates. (b) Baseline crustal production rate adopted in this work, based on the global thermal evolution model56 and the step-function interpolation of the photogeologic analysis of volcanic provinces57, whichever is greater. We adopt the model using the Hartmann (2015) chronology as our baseline model, and consider the one using the Ivanov (2001) chronology as the variant. The two models have appreciable difference in the last 2 billion years.

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