| Sample . | vol% Cb in protolith . | vol% Cb consumed . | wt% CO2 produced . | Reference . | ||
|---|---|---|---|---|---|---|
| . | . | (A) . | (B) . | (A) . | (B) . | . |
| Dolomite series | ||||||
| 17b-12 | 7 | 6 ± 0.7 | 7 | 2.9 ± 0.4 | 3.6 | This study |
| 17a-29 | 14 | 10 ± 1.7 | 11 | 5.2 ± 0.9 | 5.6 | This study |
| 15a-28a | 31 | 14 ± 2.9 | 10 | 6.9 ± 1.4 | 5.1 | This study |
| 18a-26* | 40 | 10 ± 2.0 | 1 | 5.3 ± 0.9 | 0.5 | This study |
| 17b-10b | 80 | 1 ± 0.04 | 0 | 0.6 ± 0.02 | 0 | This study |
| Magnesite series | ||||||
| 17a-36b | 7.5 | 7 ± 0.5 | 7.5 | 3.9 ± 0.3 | 4.2 | This study |
| 17a-35 | 17 | 15 ± 1.7 | 17 | 8.5 ± 1.0 | 9.7 | This study |
| 17b-7d§ | 84 | 1 ± 0.01 | 11 | 0.6 ± 0.01 | 6.2 | This study |
| Calcite series | ||||||
| ‘Synthetic’ Cal3 | 3 | 3 ± 0.4 | 3 | 1.2 ± 0.2 | 1.2 | Rapa et al. (2017) |
| ‘Synthetic’ Cal6 | 6 | 5 ± 0.8 | 6 | 2.3 ± 0.4 | 2.5 | Rapa et al. (2017) |
| ‘Synthetic’ Cal9 | 9 | 8 ± 1.7 | 9 | 3.4 ± 0.7 | 3.7 | Groppo et al. (2017) |
| ‘Synthetic’ Cal10 | 10 | 9 ± 1.9 | 7.5 | 3.7 ± 0.8 | 3.1 | Groppo et al. (2017) |
| 14-53c (Cal-poor) | 14 | 12 ± 2.8 | 14 | 5.0 ± 1.1 | 5.9 | Groppo et al. (2021) |
| 14-53c (Cal-rich) | 21 | 16 ± 4.2 | 20 | 6.5 ± 1.8 | 8.4 | Groppo et al. (2021) |
| ‘Synthetic’ Cal30 | 30 | 16 ± 4.6 | 12 | 6.8 ± 1.9 | 4.6 | Groppo et al. (2021) |
| 07–22 (Cpx-rich) | 34 | 15 ± 4.1 | 19 | 6.3 ± 1.7 | 8.0 | Groppo et al. (2022) |
| 07–22 (Cal-rich) | 43 | 10 ± 2.3 | 14 | 4.3 ± 0.9 | 5.9 | Groppo et al. (2022) |
| ‘Synthetic’ Cal50 | 50 | 7 ± 1.1 | 4 | 2.8 ± 0.4 | 1.6 | Groppo et al. (2022) |
| ‘Synthetic’ Cal70 | 70 | 2 ± 0.1 | 1.5 | 0.7 ± 0.1 | 0.6 | Groppo et al. (2022) |
| Sample . | vol% Cb in protolith . | vol% Cb consumed . | wt% CO2 produced . | Reference . | ||
|---|---|---|---|---|---|---|
| . | . | (A) . | (B) . | (A) . | (B) . | . |
| Dolomite series | ||||||
| 17b-12 | 7 | 6 ± 0.7 | 7 | 2.9 ± 0.4 | 3.6 | This study |
| 17a-29 | 14 | 10 ± 1.7 | 11 | 5.2 ± 0.9 | 5.6 | This study |
| 15a-28a | 31 | 14 ± 2.9 | 10 | 6.9 ± 1.4 | 5.1 | This study |
| 18a-26* | 40 | 10 ± 2.0 | 1 | 5.3 ± 0.9 | 0.5 | This study |
| 17b-10b | 80 | 1 ± 0.04 | 0 | 0.6 ± 0.02 | 0 | This study |
| Magnesite series | ||||||
| 17a-36b | 7.5 | 7 ± 0.5 | 7.5 | 3.9 ± 0.3 | 4.2 | This study |
| 17a-35 | 17 | 15 ± 1.7 | 17 | 8.5 ± 1.0 | 9.7 | This study |
| 17b-7d§ | 84 | 1 ± 0.01 | 11 | 0.6 ± 0.01 | 6.2 | This study |
| Calcite series | ||||||
| ‘Synthetic’ Cal3 | 3 | 3 ± 0.4 | 3 | 1.2 ± 0.2 | 1.2 | Rapa et al. (2017) |
| ‘Synthetic’ Cal6 | 6 | 5 ± 0.8 | 6 | 2.3 ± 0.4 | 2.5 | Rapa et al. (2017) |
| ‘Synthetic’ Cal9 | 9 | 8 ± 1.7 | 9 | 3.4 ± 0.7 | 3.7 | Groppo et al. (2017) |
| ‘Synthetic’ Cal10 | 10 | 9 ± 1.9 | 7.5 | 3.7 ± 0.8 | 3.1 | Groppo et al. (2017) |
| 14-53c (Cal-poor) | 14 | 12 ± 2.8 | 14 | 5.0 ± 1.1 | 5.9 | Groppo et al. (2021) |
| 14-53c (Cal-rich) | 21 | 16 ± 4.2 | 20 | 6.5 ± 1.8 | 8.4 | Groppo et al. (2021) |
| ‘Synthetic’ Cal30 | 30 | 16 ± 4.6 | 12 | 6.8 ± 1.9 | 4.6 | Groppo et al. (2021) |
| 07–22 (Cpx-rich) | 34 | 15 ± 4.1 | 19 | 6.3 ± 1.7 | 8.0 | Groppo et al. (2022) |
| 07–22 (Cal-rich) | 43 | 10 ± 2.3 | 14 | 4.3 ± 0.9 | 5.9 | Groppo et al. (2022) |
| ‘Synthetic’ Cal50 | 50 | 7 ± 1.1 | 4 | 2.8 ± 0.4 | 1.6 | Groppo et al. (2022) |
| ‘Synthetic’ Cal70 | 70 | 2 ± 0.1 | 1.5 | 0.7 ± 0.1 | 0.6 | Groppo et al. (2022) |
(A) Average values inferred from the non-linear fitting of punctual data. (B) Punctual data constrained from the phase diagram modelling.
*Note that sample 18a-26 derives from a protolith extremely enriched in quartz and very poor in clay minerals, which explains its deviation from the average behaviour of the dolomite series.
§Note that an externally buffered behaviour has been inferred for sample 17b-7d, which explains its deviation from the average behaviour of the magnesite series.
| Sample . | vol% Cb in protolith . | vol% Cb consumed . | wt% CO2 produced . | Reference . | ||
|---|---|---|---|---|---|---|
| . | . | (A) . | (B) . | (A) . | (B) . | . |
| Dolomite series | ||||||
| 17b-12 | 7 | 6 ± 0.7 | 7 | 2.9 ± 0.4 | 3.6 | This study |
| 17a-29 | 14 | 10 ± 1.7 | 11 | 5.2 ± 0.9 | 5.6 | This study |
| 15a-28a | 31 | 14 ± 2.9 | 10 | 6.9 ± 1.4 | 5.1 | This study |
| 18a-26* | 40 | 10 ± 2.0 | 1 | 5.3 ± 0.9 | 0.5 | This study |
| 17b-10b | 80 | 1 ± 0.04 | 0 | 0.6 ± 0.02 | 0 | This study |
| Magnesite series | ||||||
| 17a-36b | 7.5 | 7 ± 0.5 | 7.5 | 3.9 ± 0.3 | 4.2 | This study |
| 17a-35 | 17 | 15 ± 1.7 | 17 | 8.5 ± 1.0 | 9.7 | This study |
| 17b-7d§ | 84 | 1 ± 0.01 | 11 | 0.6 ± 0.01 | 6.2 | This study |
| Calcite series | ||||||
| ‘Synthetic’ Cal3 | 3 | 3 ± 0.4 | 3 | 1.2 ± 0.2 | 1.2 | Rapa et al. (2017) |
| ‘Synthetic’ Cal6 | 6 | 5 ± 0.8 | 6 | 2.3 ± 0.4 | 2.5 | Rapa et al. (2017) |
| ‘Synthetic’ Cal9 | 9 | 8 ± 1.7 | 9 | 3.4 ± 0.7 | 3.7 | Groppo et al. (2017) |
| ‘Synthetic’ Cal10 | 10 | 9 ± 1.9 | 7.5 | 3.7 ± 0.8 | 3.1 | Groppo et al. (2017) |
| 14-53c (Cal-poor) | 14 | 12 ± 2.8 | 14 | 5.0 ± 1.1 | 5.9 | Groppo et al. (2021) |
| 14-53c (Cal-rich) | 21 | 16 ± 4.2 | 20 | 6.5 ± 1.8 | 8.4 | Groppo et al. (2021) |
| ‘Synthetic’ Cal30 | 30 | 16 ± 4.6 | 12 | 6.8 ± 1.9 | 4.6 | Groppo et al. (2021) |
| 07–22 (Cpx-rich) | 34 | 15 ± 4.1 | 19 | 6.3 ± 1.7 | 8.0 | Groppo et al. (2022) |
| 07–22 (Cal-rich) | 43 | 10 ± 2.3 | 14 | 4.3 ± 0.9 | 5.9 | Groppo et al. (2022) |
| ‘Synthetic’ Cal50 | 50 | 7 ± 1.1 | 4 | 2.8 ± 0.4 | 1.6 | Groppo et al. (2022) |
| ‘Synthetic’ Cal70 | 70 | 2 ± 0.1 | 1.5 | 0.7 ± 0.1 | 0.6 | Groppo et al. (2022) |
| Sample . | vol% Cb in protolith . | vol% Cb consumed . | wt% CO2 produced . | Reference . | ||
|---|---|---|---|---|---|---|
| . | . | (A) . | (B) . | (A) . | (B) . | . |
| Dolomite series | ||||||
| 17b-12 | 7 | 6 ± 0.7 | 7 | 2.9 ± 0.4 | 3.6 | This study |
| 17a-29 | 14 | 10 ± 1.7 | 11 | 5.2 ± 0.9 | 5.6 | This study |
| 15a-28a | 31 | 14 ± 2.9 | 10 | 6.9 ± 1.4 | 5.1 | This study |
| 18a-26* | 40 | 10 ± 2.0 | 1 | 5.3 ± 0.9 | 0.5 | This study |
| 17b-10b | 80 | 1 ± 0.04 | 0 | 0.6 ± 0.02 | 0 | This study |
| Magnesite series | ||||||
| 17a-36b | 7.5 | 7 ± 0.5 | 7.5 | 3.9 ± 0.3 | 4.2 | This study |
| 17a-35 | 17 | 15 ± 1.7 | 17 | 8.5 ± 1.0 | 9.7 | This study |
| 17b-7d§ | 84 | 1 ± 0.01 | 11 | 0.6 ± 0.01 | 6.2 | This study |
| Calcite series | ||||||
| ‘Synthetic’ Cal3 | 3 | 3 ± 0.4 | 3 | 1.2 ± 0.2 | 1.2 | Rapa et al. (2017) |
| ‘Synthetic’ Cal6 | 6 | 5 ± 0.8 | 6 | 2.3 ± 0.4 | 2.5 | Rapa et al. (2017) |
| ‘Synthetic’ Cal9 | 9 | 8 ± 1.7 | 9 | 3.4 ± 0.7 | 3.7 | Groppo et al. (2017) |
| ‘Synthetic’ Cal10 | 10 | 9 ± 1.9 | 7.5 | 3.7 ± 0.8 | 3.1 | Groppo et al. (2017) |
| 14-53c (Cal-poor) | 14 | 12 ± 2.8 | 14 | 5.0 ± 1.1 | 5.9 | Groppo et al. (2021) |
| 14-53c (Cal-rich) | 21 | 16 ± 4.2 | 20 | 6.5 ± 1.8 | 8.4 | Groppo et al. (2021) |
| ‘Synthetic’ Cal30 | 30 | 16 ± 4.6 | 12 | 6.8 ± 1.9 | 4.6 | Groppo et al. (2021) |
| 07–22 (Cpx-rich) | 34 | 15 ± 4.1 | 19 | 6.3 ± 1.7 | 8.0 | Groppo et al. (2022) |
| 07–22 (Cal-rich) | 43 | 10 ± 2.3 | 14 | 4.3 ± 0.9 | 5.9 | Groppo et al. (2022) |
| ‘Synthetic’ Cal50 | 50 | 7 ± 1.1 | 4 | 2.8 ± 0.4 | 1.6 | Groppo et al. (2022) |
| ‘Synthetic’ Cal70 | 70 | 2 ± 0.1 | 1.5 | 0.7 ± 0.1 | 0.6 | Groppo et al. (2022) |
(A) Average values inferred from the non-linear fitting of punctual data. (B) Punctual data constrained from the phase diagram modelling.
*Note that sample 18a-26 derives from a protolith extremely enriched in quartz and very poor in clay minerals, which explains its deviation from the average behaviour of the dolomite series.
§Note that an externally buffered behaviour has been inferred for sample 17b-7d, which explains its deviation from the average behaviour of the magnesite series.
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