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Table 3

Error estimates computed from predicted values at the given interval.

Value 0–10 10–20 20–30 30–40 40–50 50–60 60–70 70–80 80–90 90–100
OL (vol%) 3.1 (54) 18.0(1) N/A (0) 11.2 (2) 5.7 (4) 4.1 (5) 9.3 (6) 8.1 (4) 20.3 (3) 8.3 (23)
OPX (vol%) 17.5 (45) 11.4 (4) 7.3 (6) 8.7 (4) 4.4 (7) 9.2 (4) 33.6 (4) 51.6 (2) 63.4 (2) 4.9 (24)
CPX (vol%) 11.6 (65) 30.1 (9) 5.7 (2) 65.3 (1) 10.5 (3) 5.4 (2) N/A (0) N/A (0) N/A (0) 24.8 (20)

Fa 3.0(13) 3.5 (16) 5.3 (11) 6.8 (4) 10.0 (3) 8.3 (1) 19.5 (1) N/A (0) N/A (0) 0.0(1)
Fo 0.0 (1) N/A (0) N/A (0) 19.5 (1) 8.3 (1) 10.0 (3) 6.8 (4) 5.3 (11) 3.5 (16) 3.0 (13)

Fs (OPX) 10.0 (5) 2.7 (27) 2.3 (16) 16.8 (3) 3.4 (2) N/A (0) 5.7 (4) 0.8 (1) 14.3 (1) 3.3 (2)
En (OPX) 3.3 (2) 14.3 (1) 0.8 (1) 5.7 (4) N/A (0) 3.4 (2) 16.8 (3) 2.3 (16) 2.7 (27) 10.0 (5)

Fs (CPX) 5.6 (19) 6.0 (16) 10.9 (6) 20.7 (3) 8.6 (3) N/A (0) 9.2 (1) N/A (0) N/A (0) N/A (0)
En (CPX) 8.3 (1) N/A (0) 16.8 (3) 10.8 (3) 8.6 (28) 16.4 (12) 3.1 (1) N/A (0) N/A (0) N/A (0)
Wo (CPX) 3.0 (1) 25.5 (3) 9.6 (6) 6.9 (18) 11.5 (19) N/A (0) 25.4 (1) N/A (0) N/A (0) N/A (0)

Notes. The values are the RMSE in percentage points. In brackets we quote the number of points from which the error was estimated. Typical values for ordinary chondrites (S- and Q-type asteroids) are highlighted.

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