The Monahans chondrite and halite: 39Ar-40Ar age, solar gases, cosmic-ray exposure ages, and parent body regolith neutron flux and thickness

Details The Monahans chondrite and halite: 39Ar-40Ar age, solar gases, cosmic-ray exposure ages, and parent body regolith neutron flux and thickness The Monahans chondrite and halite: 39Ar-40Ar age, solar gases, cosmic-ray exposure ages, and parent body regolith neutron flux and thickness

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001m%26ps...36..107b&link_type=abstract

Meteoritics & Planetary Science, vol. 36, no. 1, p. 107-122 (2001).

Computer Science

8

Scientific paper

The Monahans H-chondrite is a regolith breccia containing light and dark phases and the first reported presence of small grains of halite. We made detailed noble gas analyses of each of these phases. The 39Ar-40Ar age of Monahans light is 4.533 (0.006 Myr. Monahans dark and halite samples show greater amounts of diffusive loss of 40Ar and the maximum ages are 4.50 Gyr and 4.33 Gyr, respectively. Monahans dark phase contains significant concentrations of He, Ne and Ar implanted by the solar wind when this material was extant in a parent body regolith. Monahans light contains no solar gases. From the cosmogenic 3He, 21Ne, and 38Ar in Monahans light we calculate a probable cosmic-ray, space exposure age of 6.0 (0.5 Myr. Monahans dark contains twice as much cosmogenic 21Ne and 38Ar as does the light and indicates early near-surface exposure of 13-18 Myr in a H-chondrite regolith. The existence of fragile halite grains in H-chondrites suggests that this regolith irradiation occurred very early. Large concentrations of 36Ar in the halite were produced during regolith exposure by neutron capture on 35Cl, followed by decay to 36Ar. The thermal neutron fluence seen by the halite was 2-4 x1014 n/cm2. The thermal neutron flux during regolith exposure was ~0.4-0.7 n/cm2/s. The Monahans neutron fluence is more than an order of magnitude less than that acquired during space exposure of several large meteorites and of lunar soils, but the neutron flux is lower by a factor of (5. Comparison of the 36Arn/21Necos ratio in Monahans halite and silicate with the theoretically calculated ratio as a function of shielding depth in an H-chondrite regolith suggests that irradiation of Monahans dark occurred under low shielding in a regolith that may have been relatively shallow. Late addition of halite to the regolith can be ruled out. However, irradiation of halite and silicate for different times at different depths in an extensive regolith cannot be excluded.

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