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Table 1

Radiative-transfer fit parameters and pre-correction relative abundances for ACH1, ACH2, and a reference ordinary chondrite.

Meteor M20241012_113432 (ACH2, eucrite) M20231120_114953 (ACH1, aubrite) M20240807_093858 (ordinary chondrite)
T(K) 4200 ± 350 4800 ± 350 4200 ± 250
NFe I (cm−2) 7.6 × 1014 ± 5.5 × 1014 3.1 × 1015 ± 1.9 × 1015 1.1 × 1015 ± 1.7 × 1014
Γ (s−1) 1.0 × 1010 ± 1.0 × 109 1.4 × 1010 ± 8.0 × 109 5.0 × 109 ± 2.4 × 108
P(m2) 200 ± 170 3 ± 7 20 ± 15
Si I/Fe I 23.00 ± 4.50 80.00 ± 10.00 3.00 ± 0.75
Mg I/Fe I 0.80 ± 0.09 260.00 ± 20.00 1.83 ± 0.20
Ca I/Fe I 0.011 ± 0.002 0.033 ± 0.006 0.0002 ± 0.00003
Al I/Fe I 0.10 ± 0.04 0.04 ± 0.03 0.001 ± 0.0006
Ti I/Fe I 0.001 ± 0.0001 0.003 ± 0.001 0.0004 ± 0.00005
Cr I/Fe I 0.004 ± 0.0003 0.048 ± 0.007 0.002 ± 0.0004
Mn I/Fe I 0.02 ± 0.002 0.095 ± 0.033 0.006 ± 0.0007
Na I/Fe I 0.0002 ± 0.00001 0.032 ± 0.006 0.002 ± 0.001
K I/Fe I 1 × 10−6 ± 3 × 10−7 0.0002 ± 0.00005
Li I/Fe I 1 × 10−5 ± 2 × 10−6 6 × 10−5 ± 2 × 10−6

Notes. Results of spectral fitting for ACH1 (aubrite candidate), ACH2 (eucrite candidate), and a representative ordinary chondrite. Listed are the parameters of the main spectral component derived from the radiative transfer model: temperature (T), column density of FeI atoms (NFe I), damping constant (Γ), and radiating plasma cross section (P), together with abundances of selected species relative to Fe I (before ionization correction).

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