The SKA as a Prebiotic Molecule Detector

[EN] One of the theories for the origin of life proposes that a significant fraction of prebiotic material could have arrived to Earth from outer space between 4.1 and 3.8 billion years ago. This suggests that those prebiotic compounds could have originated in interstellar space, to be later on inco...

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Detalles Bibliográficos
Autores: Jiménez Serra, Izaskun, Martín Pintado, Jesús, Insausti Beiro, Aran, Alonso Alonso, Elena Rita, Cocinero Pérez, Emilio José, Bourke, Tyler L.
Tipo de recurso: artículo
Fecha de publicación:2022
País:España
Institución:Universidad del País Vasco
Repositorio:Addi. Archivo Digital para la Docencia y la Investigación
OAI Identifier:oai:addi.ehu.eus:10810/56607
Acceso en línea:http://hdl.handle.net/10810/56607
Access Level:acceso abierto
Palabra clave:square kilometre array
complex organic molecules
prebiotic chemistry
interstellar medium
astrochemistry
Descripción
Sumario:[EN] One of the theories for the origin of life proposes that a significant fraction of prebiotic material could have arrived to Earth from outer space between 4.1 and 3.8 billion years ago. This suggests that those prebiotic compounds could have originated in interstellar space, to be later on incorporated to small Solar-system bodies and planetesimals. The recent discovery of prebiotic molecules such as hydroxylamine and ethanolamine in the interstellar medium, strongly supports this hypothesis. However, some species such as sugars, key for the synthesis of ribonucleotides and for metabolic processes, remain to be discovered in space. The unmatched sensitivity of the Square Kilometre Array (SKA) at centimeter wavelengths will be able to detect even more complex and heavier prebiotic molecules than existing instrumentation. In this contribution, we illustrate the potential of the SKA to detect simple sugars with three and four carbon atoms, using a moderate investment of observing time.