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Ariel a window to the origin of life on early earth?
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SYSNO ASEP 0536992 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Ariel a window to the origin of life on early earth? Author(s) Ferus, Martin (UFCH-W) ORCID, RID
Adam, V. (CZ)
Cassone, G. (IT)
Civiš, Svatopluk (UFCH-W) RID, ORCID, SAI
Čuba, V. (CZ)
Chatzitheodoridis, E. (GR)
Drtinová, B. (CZ)
Le Floch, P. (FR)
Heays, Alan (UFCH-W) ORCID, RID, SAI
Jheeta, S. (GB)
Kereszturi, A. (HU)
Knížek, Antonín (UFCH-W) ORCID, RID, SAI
Krůs, M. (CZ)
Kubelík, Petr (UFCH-W) RID, ORCID
Lammer, H. (AT)
Lenža, Libor (UFCH-W) ORCID, RID, SAI
Nejdl, L. (CZ)
Pastorek, Adam (UFCH-W) ORCID
Petera, Lukáš (UFCH-W) ORCID
Rimmer, P. (GB)
Saladino, R. (IT)
Saija, F. (IT)
Spross, L. (AT)
Šponer, Jiří (BFU-R) RID, ORCID
Šponer, Judit E. (BFU-R) RID, ORCID
Todd, Z. (US)
Vaculovičová, M. (CZ)
Zemánková, K. (CZ)
Chernov, V. E. (RU)Source Title Experimental Astronomy. - : Springer - ISSN 0922-6435
Roč. 53, č. 2 (2022), s. 679-728Number of pages 50 s. Publication form Online - E Language eng - English Country NL - Netherlands Keywords high-power laser ; induced dielectric-breakdown ; late heavy bombardment ; high-energy chemistry ; amino-acids ; prebiotic chemistry ; hydrogen-peroxide ; emission-spectroscopy ; terrestrial planets ; radiation-chemistry ; Prebiotic chemistry ; Origin of life ; Prebiotic molecule detection ; Exoplanet Subject RIV CF - Physical ; Theoretical Chemistry OECD category Physical chemistry Subject RIV - cooperation Institute of Biophysics - Physical ; Theoretical Chemistry R&D Projects GA19-03314S GA ČR - Czech Science Foundation (CSF) EF16_019/0000778 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) Method of publishing Limited access Institutional support UFCH-W - RVO:61388955 ; BFU-R - RVO:68081707 UT WOS 000592518400001 EID SCOPUS 85096518696 DOI 10.1007/s10686-020-09681-w Annotation 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. Workplace J. Heyrovsky Institute of Physical Chemistry Contact Michaela Knapová, michaela.knapova@jh-inst.cas.cz, Tel.: 266 053 196 Year of Publishing 2023 Electronic address https://link.springer.com/article/10.1007%2Fs10686-020-09681-w
Number of the records: 1