  Solar system materials are variably depleted in moderately volatile elements
(MVEs) relative to the proto-solar composition. To address the origin of this
MVE depletion, we conducted a systematic study of high-precision K isotopic
composition on 16 carbonaceous chondrites (CCs) of types CM1-2, CO3, CV3, CR2,
CK4-5 and CH3 and 28 ordinary chondrites (OCs) covering petrological types 3 to
6 and chemical groups H, L, and LL. We observed significant overall K isotope
(delta41K) variations (-1.54 to 0.70 permil). The K isotope compositions of CCs
are largely higher than the Bulk Silicate Earth (BSE) value, whereas OCs show
typically lower values than BSE. Neither CCs nor OCs show resolvable
correlations between K isotopes and chemical groups, petrological types, shock
levels, exposure ages, fall or find occurrence, or terrestrial weathering. The
lack of a clear trend between K isotopes and K content indicates that the K
isotope fractionations were decoupled from the relative elemental K depletions.
The range of K isotope variations in the CCs is consistent with a
four-component (chondrule, refractory inclusion, matrix and water) mixing model
that is able to explain the bulk elemental and isotopic compositions of the
main CC groups, but requires a fractionation in K isotopic compositions in
chondrules. We propose that the major control of the isotopic compositions of
group averages is condensation or vaporization in nebular environments that is
preserved in the compositional variation of chondrules. Parent-body processes
(aqueous alteration, thermal metamorphism, and metasomatism) can mobilize K and
affect the K isotopes in individual samples. In the case of the OCs, the full
range of K isotopic variations can only be explained by the combined effects of
the size and relative abundances of chondrules, parent-body aqueous and thermal
alteration.
