In carbonaceous chondrite meteorites such as the Murchison meteorite, several non-proteinogenic alpha-amino acids exhibit slight left-handed (L-enantiomer) excesses, ranging from 2% to 18%. Because terrestrial biological contamination exclusively yields standard proteinogenic amino acids, the presence of L-excesses in non-terrestrial, non-proteinogenic amino acids indicates that abiotic chiral asymmetry originated prior to the emergence of terrestrial biochemistry. The leading astrophysical model posits that this enantiomeric bias was induced by asymmetric photolysis driven by ultraviolet circularly polarized light (UV-CPL) in the protoplanetary nebula. Laboratory irradiations of racemic amino acid ices with synchrotron UV-CPL have successfully reproduced small enantiomeric excesses; however, the magnitude of the photo-induced excess is strictly constrained by the total degree of photochemical destruction, with high enantiomeric excesses requiring over 99% molecular degradation. Consequently, researchers propose that secondary aqueous alteration within the meteorite's parent asteroid must have subsequently amplified these initial modest asymmetries via solid-solution phase equilibria without requiring catastrophic photolytic depletion.
Based on the passage, which of the following statements are logically supported by the text? (Select all that apply.)
- The chiral bias observed in non-proteinogenic amino acids from carbonaceous chondrites cannot be attributed to contamination from living terrestrial organisms.Cevap
- BSecondary aqueous alteration inside parent asteroids generated the initial chiral asymmetry without any prior exposure to ultraviolet circularly polarized light.
- CSynchrotron radiation is emitted naturally by protoplanetary nebulae and serves as the primary environmental driver of chiral selection in deep space.
- Producing a substantial enantiomeric excess through UV-CPL photolysis alone would necessitate the destruction of almost all of the precursor amino acid molecules.Cevap
- EEvery amino acid extracted from the Murchison meteorite displays an L-enantiomer excess greater than 18%.