Institut für Mineralogie, Westfälische Wilhelms-Universität, Corrensstr. 24, 48149, Münster, Germany.
Particle Chemistry Department, Max Planck Institute for Chemistry, Hahn-Meitner-Weg 1, 55128, Mainz, Germany.
Sci Rep. 2020 Nov 20;10(1):20251. doi: 10.1038/s41598-020-77190-z.
We report on the detection of primordial organic matter within the carbonaceous chondrite Maribo that is distinct from the majority of organics found in extraterrestrial samples. We have applied high-spatial resolution techniques to obtain C-N isotopic compositions, chemical, and structural information of this material. The organic matter is depleted in N relative to the terrestrial value at around δN ~ -200‰, close to compositions in the local interstellar medium. Morphological investigations by electron microscopy revealed that the material consists of µm- to sub-µm-sized diffuse particles dispersed within the meteorite matrix. Electron energy loss and synchrotron X-ray absorption near-edge structure spectroscopies show that the carbon functional chemistry is dominated by aromatic and C=O bonding environments similar to primordial organics from other carbonaceous chondrites. The nitrogen functional chemistry is characterized by C-N double and triple bonding environments distinct from what is usually found in N-enriched organics from aqueously altered carbonaceous chondrites. Our investigations demonstrate that Maribo represents one of the least altered CM chondrite breccias found to date and contains primordial organic matter, probably originating in the interstellar medium.
我们报告了在碳质球粒陨石马里博中检测到的原始有机物,其与大多数在天体样本中发现的有机物明显不同。我们应用了高空间分辨率技术来获取该物质的 C-N 同位素组成、化学和结构信息。该有机物相对于地球值,氮含量较低,约为 δN~-200‰,与局部星际介质中的组成相近。通过电子显微镜进行的形态学研究表明,该物质由微米到亚微米大小的弥散颗粒组成,分散在陨石基质中。电子能量损失和同步加速器 X 射线吸收近边结构光谱表明,碳的官能团化学主要由芳香族和 C=O 键合环境主导,类似于其他碳质球粒陨石中的原始有机物。氮的官能团化学的特点是 C-N 双键和三键环境,与水蚀变碳质球粒陨石中通常发现的富氮有机物明显不同。我们的研究表明,马里博代表了迄今为止发现的最不易受改变的 CM 球粒陨石碎片之一,其中含有原始有机物,可能源自星际介质。