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dc.contributor.authorSparks, W.
dc.contributor.authorHough, J.H.
dc.contributor.authorGermer, T.A.
dc.contributor.authorRobb, F.
dc.contributor.authorKolokolova, L.
dc.date.accessioned2014-09-01T13:30:54Z
dc.date.available2014-09-01T13:30:54Z
dc.date.issued2012-11-01
dc.identifier.citationSparks , W , Hough , J H , Germer , T A , Robb , F & Kolokolova , L 2012 , ' Remote sensing of chiral signatures on Mars ' , Planetary and Space Science , vol. 72 , no. 1 , pp. 111-115 . https://doi.org/10.1016/j.pss.2012.08.010
dc.identifier.issn0032-0633
dc.identifier.otherBibtex: urn:3d5328b5e06ba62e77f0c88c1e3d60d5
dc.identifier.urihttp://hdl.handle.net/2299/14412
dc.description.abstractWe describe circular polarization as a remote sensing diagnostic of chiral signatures which may be applied to Mars. The remarkable phenomenon of homochirality provides a unique biosignature which can be amenable to remote sensing through circular polarization spectroscopy. The natural tendency of microbes to congregate in close knit communities would be beneficial for such a survey. Observations of selected areas of the Mars surface could reveal chiral signatures and hence explore the possibility of extant or preserved biological material. We describe a new instrumental technique that may enable observations of this formen
dc.format.extent5
dc.format.extent1855971
dc.language.isoeng
dc.relation.ispartofPlanetary and Space Science
dc.titleRemote sensing of chiral signatures on Marsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1016/j.pss.2012.08.010
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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