Abstract

Meteorites contain organic matter that may have contributed to the origin of life on Earth. Carbonyl compounds such as aldehydes and carboxylic acids, which occur in meteorites, may be precursors of biologically necessary organic materials in the solar system. Therefore, such organic matter is of astrobiological importance and their detection and characterization can contribute to the understanding of the early solar system as well as the origin of life. Most organic matter is typically sub-micrometer in size, and organic nanoglobules are even smaller (50–300 nm). Novel analytical techniques with nanoscale spatial resolution are required to detect and characterize organic matter within extraterrestrial materials. Most techniques require powdered samples, consume the material, and lose petrographic context of organics. Here, we report the detection of nanoglobular aldehyde and carboxylic acids in a highly primitive carbonaceous chondrite (DOM 08006) with ~ 20 nm spatial resolution using nano-FTIR spectroscopy. Such organic matter is found within the matrix of DOM 08006 and is typically 50–300 nm in size. We also show petrographic context and nanoscale morphologic/topographic features of the organic matter. Our results indicate that prebiotic carbonyl nanoglobules can form in a less aqueous and relatively elevated temperature-environment (220–230 °C) in a carbonaceous parent body.

Highlights

  • Carbonaceous chondrites are the most primitive meteorite samples in the solar system, and they retain records of their formation and post-accretionary processes

  • Nano-Fourier transform infrared (FTIR) spectroscopy is based on scattering-type scanning near-field optical microscopy (s-SNOM)[26], where a metal coated conductive atomic force microscope (AFM) tip acts as an antenna for probing the molecular v­ ibrations[27]

  • We report the detection of C=O functional group organic compounds in situ in DOM 08006 with ~ 20 nm spatial resolution using nano-FTIR spectroscopy

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Summary

Introduction

Carbonaceous chondrites are the most primitive meteorite samples in the solar system, and they retain records of their formation and post-accretionary processes. They contain a wide range of extraterrestrial organic compounds that can provide information about the processes in the interstellar medium and early solar system. Like other well-established carbonaceous chondrite groups, the properties of members of the CO3 chondrites are attributed to the thermal metamorphic processes they have been subjected to In this context, the subtype CO3.0 chondrites can be considered to be the least altered and relatively more primitive. The mineralogies of a carbonaceous chondrite and a cometary dust grain have been investigated at ~ 20 nm spatial resolution using nano-FTIR, within a limited (1100–800 ­cm−1) spectral r­ ange[33]. There is no other prior study that investigated chondritic organic matter using nano-FTIR spectroscopy

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