Skip to main content
Kent Academic Repository

New Signatures of Bio-Molecular Complexity in the Hypervelocity Impact Ejecta of Icy Moon Analogues

Singh, Suvrendra V., Dilip, Haritha, Meka, Jaya K., Thiruvenkatam, Vija, Jayarum, Vishakantaiah, Muruganantham, Mariyappan, Sivaprahasam, Vijayan, Rajasekhar, Balabhadrapatruni N., Bhardwaj, Anil, Mason, Nigel J., and others. (2022) New Signatures of Bio-Molecular Complexity in the Hypervelocity Impact Ejecta of Icy Moon Analogues. Life, 12 (4). Article Number 508. E-ISSN 2075-1729. (doi:10.3390/life1204050) (KAR id:95465)

Abstract

Impact delivery of prebiotic compounds to the early Earth from an impacting comet is considered to be one of the possible ways by which prebiotic molecules arrived on the Earth. Given the ubiquity of impact features observed on all planetary bodies, bolide impacts may be a common source of organics on other planetary bodies both in our own and other solar systems. Biomolecules such as amino acids have been detected on comets and are known to be synthesized due to impact-induced shock processing. Here we report the results of a set of hypervelocity impact experiments where we shocked icy mixtures of amino acids mimicking the icy surface of planetary bodies with high-speed projectiles using a two-stage light gas gun and analyzed the ejecta material after impact. Electron microscopic observations of the ejecta have shown the presence of macroscale structures with long polypeptide chains revealed from LCMS analysis. These results suggest a pathway in which impact on cometary ices containing building blocks of life can lead to the synthesis of material architectures that could have played a role in the emergence of life on the Earth and which may be applied to other planetary bodies as well. View Full-Text

Item Type: Article
DOI/Identification number: 10.3390/life1204050
Uncontrolled keywords: amino acids; polypeptides; impact ejecta; icy moons; astrobiology
Subjects: Q Science > QB Astronomy > QB651 Planets, Minor
Divisions: Divisions > Division of Natural Sciences > Physics and Astronomy
Funders: Royal Society (https://ror.org/03wnrjx87)
Depositing User: Mark Burchell
Date Deposited: 16 Jun 2022 09:11 UTC
Last Modified: 17 Jun 2022 08:46 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/95465 (The current URI for this page, for reference purposes)

University of Kent Author Information

  • Depositors only (login required):

Total unique views for this document in KAR since July 2020. For more details click on the image.