关于碳质陨石中 L-异戊烯对映体过量与水蚀程度之间的关系

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Frontiers in Astronomy and Space Sciences Pub Date : 2024-07-26 DOI:10.3389/fspas.2024.1427260
David Avnir
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引用次数: 0

摘要

研究发现,L-异戊烯(L-iVal)的对映体过量(ee)与碳质陨石的水蚀变程度(AqA)之间存在正相关。从两个角度来看,这一显著现象的起源一直是个谜:首先,这种相关性是在看似不相关的观测数据之间产生的--AqA 并不具有手性特征;其次,根据公认的假设,即圆偏振光(CPL)是观测到的陨石 L-氨基酸(AAs)ee 的起源,但仍然不清楚为什么在这种相关性中观测到的一些 L-iVal ee 水平明显高于在实验室模拟中观测到的水平或通过圆二色性(CD)g 因子计算得到的水平。目前对这一情况的解释是,陨石母体的晚期 AqA 条件为早期最初由 CPL 产生的低水平 L-ee 的放大提供了依据。出于以下原因,我们重新审视了这种解释,它把 CPL 事件和 AqA 过程看作是发生在时间相隔很远的时代。对观测到的相关性和高ee值提供了另一种解释。它侧重于前太阳系早期湿恒星形成区中的亲水性尘埃-聚集云,CPL事件和导致后来母体AqA过程的原因都发生在那里。这种机制消除了初始ee形成与母体AqA之间的时间差,取而代之的是平行过程,为观测到高ee而没有完全摧毁提供了一种设想,也为明显的AqA/L-ee相关性提供了一种设想。虽然 iVal 是本报告的重点,但发展替代机制的步骤和由此得出的结论与陨石 AA 的 L-ee 的一般观测结果相关并适用。
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On the correlation between the enantiomeric excess of L-isovaline and the level of aqueous alteration in carbonaceous meteorites
A positive correlation was observed between the enantiomeric excess (ee) of L-isovaline (L-iVal) and the degree of aqueous alteration (AqA) of carbonaceous meteorites. The origin of this remarkable phenomenon has remained enigmatic from two points of view: First, the correlation is between seemingly unrelated observables–nothing about AqA is of chiral characteristics; and second, following the accepted assumption that circularly polarized light (CPL) was the origin of the observed meteoritic ee of L-amino acids (AAs), it remined unclear why some of the observed levels of the ee of L-iVal in that correlation are significantly higher than those observed in laboratory simulations or those obtained from circular dichroism (CD) g-factor calculations. The current proposition accounting for this picture attributes late AqA conditions of the meteoritic parent bodies as providing the grounds for amplification of early initially CPL-generated low levels of L-ee. For reasons summarized below, this interpretation, which treats the CPL event and the AqA process as occurring in wide-time separated eras, is re-visited. An alternative interpretation of the observed correlation and of the high ee-values, is provided. It focuses on hydrophilic dust-aggregates clouds in wet star-forming regions in early pre-solar times, where both the CPL event and the grounds leading to the later AqA processes of the parent bodies, occurred. This mechanism removes the time separation between the initial ee formation and the AqA of the parent body, and replaces it with parallel processes, providing a scenario to the observation of high ee’s without total destruction, and to the apparent AqA/L-ee correlation. Although iVal is at the focus of this report, the steps of the development of the alternative mechanism and the conclusions that arise from it, are relevant and applicable to the general observations of L-ee’s of meteoritic AA’s.
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
期刊最新文献
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