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Morphology: An Ambiguous Indicator of Biogenicity

dc.contributor.authorGarcia Ruiz, Juan Manuel
dc.contributor.authorCarnerup, Anna
dc.contributor.authorChristy, Andrew
dc.contributor.authorWelham, N
dc.contributor.authorHyde, Stephen
dc.date.accessioned2015-12-13T22:18:04Z
dc.date.issued2002
dc.date.updated2015-12-11T07:41:21Z
dc.description.abstractAn integrated analysis of both airborne and field short-wave infrared hyperspectral measurements was used in conjunction with conventional field mapping techniques to map hydrothermal alteration in the central portion of the Mount Painter Inlier in the Flinders Ranges, South Australia. The airborne hyperspectral data show the spatial distribution of spectrally distinct minerals occurring as primary minerals and as weathering and alteration products. Field spectral measurements, taken with a portable infrared mineral analyzer spectrometer and supported by thin-section analyses, were used to verify the mineral maps and enhance the level of information obtainable from the airborne data. Hydrothermal alteration zones were identified and mapped separately from the background weathering signals. A main zone of alteration, coinciding with the Paralana Fault zone, was recognized, and found to contain kaolinite, muscovite, biotite, and K-feldspar. A small spectral variation associated with a ring-like feature around Mount Painter was tentatively determined to be halloysite and interpreted to represent a separate hydrothermal fluid and fluid source, and probably a separate system. The older parts of the alteration system are tentatively dated as Permo-Carboniferous. The remote sensing of alteration at Mount Painter confirms that hyperspectral imaging techniques can produce accurate mineralogical maps with significant details that can be used to identify and map hydrothermal activity. Application of hyperspectral surveys such as that conducted at Mount Painter would be likely to provide similar detail about putative hydrothermal deposits on Mars.
dc.identifier.issn1531-1074
dc.identifier.urihttp://hdl.handle.net/1885/71466
dc.publisherMary Ann Liebert Inc.
dc.sourceAstrobiology
dc.subjectKeywords: article; astronomy; geology; infrared spectrophotometry; Earth (Planet); Geology; Mars; Spectrophotometry, Infrared
dc.titleMorphology: An Ambiguous Indicator of Biogenicity
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage351
local.bibliographicCitation.startpage335
local.contributor.affiliationGarcia Ruiz, Juan Manuel, Universidad de Granada
local.contributor.affiliationCarnerup, Anna, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationChristy, Andrew, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWelham, N, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHyde, Stephen, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidCarnerup, Anna, u3931514
local.contributor.authoruidChristy, Andrew, u9406101
local.contributor.authoruidWelham, N, u4014940
local.contributor.authoruidHyde, Stephen, u8604415
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor040399 - Geology not elsewhere classified
local.identifier.ariespublicationMigratedxPub2728
local.identifier.citationvolume2
local.identifier.scopusID2-s2.0-0038007041
local.type.statusPublished Version

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