Prebiotic astrochemistry and the formation of molecules of astrobiological interest in interstellar clouds and protostellar disks

SA Sandford, M Nuevo, PP Bera, TJ Lee - Chemical reviews, 2020 - ACS Publications
Despite the generally hostile nature of the environments involved, chemistry does occur in
space. Molecules are seen in environments that span a wide range of physical and chemical …

Spectroscopic sizing of interstellar icy grains with JWST

E Dartois, JA Noble, P Caselli, HJ Fraser… - Nature …, 2024 - nature.com
Clouds of gas and dust in the Galaxy are nurseries in which stars and planetary systems are
born. During their journey from the diffuse interstellar medium to the protoplanetary disks …

Formation of NH2CHO and CH3CHO upon UV photoprocessing of interstellar ice analogs

R Martín-Doménech, KI Öberg… - The Astrophysical …, 2020 - iopscience.iop.org
Complex organic molecules (COMs) can be produced by energetic processing of interstellar
ice mantles accreted on top of dust grains. Two COMs with proposed energetic ice formation …

Densities, infrared band strengths, and optical constants of solid methanol

R Luna, G Molpeceres, J Ortigoso, MA Satorre… - Astronomy & …, 2018 - aanda.org
Contact. The increasing capabilities of space missions like the James Webb Space
Telescope or ground-based observatories like the European Extremely Large Telescope …

Abiotic formation of alkylsulfonic acids in interstellar analog ices and implications for their detection on Ryugu

M McAnally, J Bocková, A Herath, AM Turner… - Nature …, 2024 - nature.com
For the last century, the source of sulfur in Earth's very first organisms has remained a
fundamental, unsolved enigma. While sulfates and their organic derivatives with sulfur in the …

[HTML][HTML] A tale of 3 dwarf planets: Ices and organics on Sedna, Gonggong, and Quaoar from JWST spectroscopy

JP Emery, I Wong, R Brunetto, JC Cook… - Icarus, 2024 - Elsevier
Abstract The dwarf planets Sedna, Gonggong, and Quaoar are interesting in being
somewhat smaller than the methane-rich bodies of the Kuiper Belt (Pluto, Eris, Makemake) …

X-ray versus ultraviolet irradiation of astrophysical ice analogs leading to formation of complex organic molecules

GM Munoz Caro, A Ciaravella… - ACS Earth and Space …, 2019 - ACS Publications
In astrochemistry, complex organic molecules (COMs) are defined as species with at least
one C atom and six or more atoms in total. More than 70 COMs were detected toward …

Material properties of organic liquids, ices, and Hazes on Titan

X Yu, Y Yu, J Garver, J Li, A Hawthorn… - The Astrophysical …, 2023 - iopscience.iop.org
Titan has a diverse range of materials in its atmosphere and on its surface: the simple
organics that reside in various phases (gas, liquid, and ice) and the solid complex refractory …

On the spectral features of dangling bonds in CH 4/H 2 O amorphous ice mixtures

B Maté, MÁ Satorre, R Escribano - Physical Chemistry Chemical …, 2021 - pubs.rsc.org
Dangling bond (DB) bands in IR spectra, above 3600 cm− 1, are a source of information on
structural properties of amorphous water ice, and especially on ice mixtures of water and …

Densities and refractive indices of ethane and ethylene at astrophysically relevant temperatures

MÁ Satorre, C Millán, G Molpeceres, R Luna, B Maté… - Icarus, 2017 - Elsevier
We report the density and refractive index, at 633 nm, of ethane and ethylene ices at
temperatures from 13 to 65 K, measured by double laser interferometry and a cryogenic …