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The Kuiper Belt object (KBO) Arrokoth, the farthest object in the Solar System ever visited by a spacecraft, possesses a distinctive reddish surface and is characterized by pronounced spectroscopic features associated with methanol. However, the fundamental processes by which methanol ices are converted into reddish, complex organic molecules on Arrokoth's surface have remained elusive. Here, we combine laboratory simulation experiments with a spectroscopic characterization of methanol ices exposed to proxies of galactic cosmic rays (GCRs). Our findings reveal that the surface exposure of methanol ices at 40 K can replicate the color slopes of Arrokoth. Sugars and their derivatives (acids, alcohols) with up to six carbon atoms, including glucose and ribose-fundamental building block of RNA-were ubiquitously identified. In addition, polycyclic aromatic hydrocarbons (PAHs) with up to six ring units (CH) were also observed. These sugars and their derivatives along with PAHs connected by unsaturated linkers represent key molecules rationalizing the reddish appearance of Arrokoth. The formation of abundant sugar-related molecules dubs Arrokoth as a sugar world and provides a plausible abiotic preparation route for a key class of biorelevant molecules on the surface of KBOs prior to their delivery to prebiotic Earth.
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http://dx.doi.org/10.1073/pnas.2320215121 | DOI Listing |
J Am Chem Soc
August 2025
Combustion Research Facility, Sandia National Laboratories, Livermore, California 94551, United States.
Sugars are produced by living organisms, and are required building blocks for life as we know it, which raises the foundational question of how sugars formed in a prebiotic environment. The abiotic formose reaction produces sugars from formaldehyde, but our understanding of its initiation step remains murky, with chemists invoking the concept of an "activated aldehyde" to seed this reaction. Singlet hydroxycarbenes, high-energy isomers of aldehydes, were recently reported to facilitate sugar formation under cold, nonaqueous conditions relevant to interstellar environments.
View Article and Find Full Text PDFJ Chem Phys
July 2025
Università degli Studi di Torino, Dipartimento di Chimica, via P. Giuria 7, 10125 Torino, Italy.
Temperature programmed desorption (TPD) is a well-known technique to study gas-surface processes, and it is characterized by two main quantities: the adsorbate binding energy and the pre-exponential factor. While the former has been well addressed in recent years by both experimental and computational methods, the latter remains somewhat ill-defined, and different schemes have been proposed in the literature for its evaluation. In the astrochemistry context, binding energies and pre-exponential factors are key parameters that enter microkinetic models for studying the evolution over time of the chemical species in the universe.
View Article and Find Full Text PDFJ Mol Model
February 2025
Departamento de Físico-Química, Facultad de Ciencias Químicas, Universidad de Concepción, Concepción, Chile.
Context: Methyl formate (MF) has been detected in several interstellar environments, but whether or not the formation of this molecule takes place in the gas phase or on the ices of interstellar grains is still unclear. In this study, we explore the synthesis of methyl formate through the nucleophilic acyl substitution (S Acyl) reaction between methanol (CH OH) and formic acid (HCOOH) on amorphous solid water, which is the main component of interstellar ice mantles.
Methods: Using density functional theory (DFT), we model MF formation by sampling HCOOH in different catalytic sites on the water clusters with CH OH, and vice versa, for initial reactant configurations.
J Chem Phys
September 2024
Department of Chemistry, University of Missouri, Columbia, Missouri 65203, USA.
This second paper in a series of two describes the chirped-pulse ice apparatus that permits the detection of buffer gas cooled molecules desorbed from an energetically processed ice using broadband mm-wave rotational spectroscopy. Here, we detail the lower ice stage developed to generate ices at 4 K, which can then undergo energetic processing via UV/VUV photons or high-energy electrons and which ultimately enter the gas phase via temperature-programmed desorption (TPD). Over the course of TPD, the lower ice stage is interfaced with a buffer gas cooling cell that allows for sensitive detection via chirped-pulse rotational spectroscopy in the 60-90 GHz regime.
View Article and Find Full Text PDFProc Natl Acad Sci U S A
June 2024
Department of Chemistry, University of Hawaii at Mānoa, Honolulu, HI 96822.
The Kuiper Belt object (KBO) Arrokoth, the farthest object in the Solar System ever visited by a spacecraft, possesses a distinctive reddish surface and is characterized by pronounced spectroscopic features associated with methanol. However, the fundamental processes by which methanol ices are converted into reddish, complex organic molecules on Arrokoth's surface have remained elusive. Here, we combine laboratory simulation experiments with a spectroscopic characterization of methanol ices exposed to proxies of galactic cosmic rays (GCRs).
View Article and Find Full Text PDF