Ariel – a window to the origin of life on early earth?

0582169 - ÚFP 2024 RIV DE eng J - Článek v odborném periodiku
Ferus, M. - Adam, V. - Cassone, G. - Civiš, S. - Čuba, V. - Chatzitheodoridis, E. - Drtinová, B. - Lefloch, B. - Heays, A.N. - Jheeta, S. - Kereszturi, A. - Knížek, A. - Krůs, Miroslav - Kubelík, P. - Lammer, H. - Lenža, L. - Nejdl, L. - Pastorek, A. - Petera, L. - Rimmer, P. - Saladino, R. - Saija, F. - Sproß, L. - Šponer, J. - Šponer, J. - Todd, Z. - Vaculovičová, M. - Zemánková, K. - Chernov, V. V.
Ariel – a window to the origin of life on early earth?
Experimental Astronomy. Roč. 53, č. 2 (2022), s. 679-728. ISSN 0922-6435. E-ISSN 1572-9508
Grant CEP: GA ČR GA19-03314S; GA MŠMT EF16_019/0000778
Institucionální podpora: RVO:61389021
Klíčová slova: Exoplanet * Origin of life * Prebiotic chemistry * Prebiotic molecule detection
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 3, rok: 2022
Způsob publikování: Omezený přístup
https://link.springer.com/article/10.1007/s10686-020-09681-w

Is there life beyond Earth? An ideal research program would first ascertain how life on Earth began and then use this as a blueprint for its existence elsewhere. But the origin of life on Earth is still not understood, what then could be the way forward? Upcoming observations of terrestrial exoplanets provide a unique opportunity for answering this fundamental question through the study of other planetary systems. If we are able to see how physical and chemical environments similar to the early Earth evolve we open a window into our own Hadean eon, despite all information from this time being long lost from our planet’s geological record. A careful investigation of the chemistry expected on young exoplanets is therefore necessary, and the preparation of reference materials for spectroscopic observations is of paramount importance. In particular, the deduction of chemical markers identifying specific processes and features in exoplanetary environments, ideally “uniquely”. For instance, prebiotic feedstock molecules, in the form of aerosols and vapours, could be observed in transmission spectra in the near future whilst their surface deposits could be observed from reflectance spectra. The same detection methods also promise to identify particular intermediates of chemical and physical processes known to be prebiotically plausible. Is Ariel truly able to open a window to the past and answer questions concerning the origin of life on our planet and the universe? In this paper, we discuss aspects of prebiotic chemistry that will help in formulating future observational and data interpretation strategies for the Ariel mission. This paper is intended to open a discussion and motivate future detailed laboratory studies of prebiotic processes on young exoplanets and their chemical signatures.
Trvalý link: https://hdl.handle.net/11104/0350247