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dc.contributor.authorCraft, K.L.
dc.contributor.authorBarnouin, O.S.
dc.contributor.authorGaskell, R.
dc.contributor.authorPalmer, E.
dc.contributor.authorWeirich, J.
dc.contributor.authorPerry, M.
dc.contributor.authorBierhaus, B.
dc.contributor.authorNorman, C.
dc.contributor.authorHuish, D.
dc.contributor.authorOlds, R.
dc.contributor.authorDaly, M.G.
dc.contributor.authorLorenz, D.
dc.contributor.authorRizk, B.
dc.contributor.authorLauretta, D.S.
dc.date.accessioned2020-12-15T20:06:08Z
dc.date.available2020-12-15T20:06:08Z
dc.date.issued2020-11
dc.identifier.citationCraft, K. L., Barnouin, O. S., Gaskell, R., Palmer, E., Weirich, J., Perry, M., ... & Daly, M. G. (2020). Assessing stereophotoclinometry by modeling a physical wall representing asteroid Bennu. Planetary and Space Science, 193, 105077.en_US
dc.identifier.issn0032-0633
dc.identifier.doi10.1016/j.pss.2020.105077
dc.identifier.urihttp://hdl.handle.net/10150/649285
dc.description.abstractThe Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission is characterizing the surface and orbital environment of the primitive asteroid (101955) Bennu to enable the collection and return of pristine samples of carbonaceous material. The Altimetry Working Group (AltWG) generates digital terrain models (DTMs) that are essential for assessing the sampleability and science value of potential sample sites. The AltWG uses stereophotoclinometry (SPC) to generate these DTMs from images collected by the OSIRIS-REx Camera Suite. We built and evaluated an SPC-derived DTM by performing a flight-like test, using images (0.4-3 cm per pixel) of a physical test wall constructed to simulate a 3 m x 3m portion of Bennu's surface. We built the DTM using images acquired under similar lighting conditions to those planned for the OSIRIS-REx mission and processed them using flight-like SPC procedures. The results were compared to measurements of the wall obtained using a laser altimeter. We found maximum height differences between the SPC-derived model and the altimetric data of -2.6 and 3.4 cm (or 13-17% of the dynamic range of the heights across the wall), specifically around large surface rocks. For the majority of the SPC-derived model, differences are less than +/- 0.5 cm (<2.5% of the dynamic range of the heights across the wall) or similar to 1.5 x the images' best pixel scale of 0.4 cm. In the spatial frequency domain, spectral correlation and coherency assessments comparing the SPC-derived model and the altimetric data show that the SPC-generated DTMs are an excellent product from wavelengths of similar to 3 m down to shorter wavelengths of similar to 0.1 m. Cross-correlation assessment of images rendered from the SPC-derived model vs. images of the test wall further show that our models accurately reproduce the combined albedo and surface shape, with cross-correlation scores >0.65.en_US
dc.description.sponsorshipNational Aeronautics and Space Administrationen_US
dc.language.isoenen_US
dc.publisherPERGAMON-ELSEVIER SCIENCE LTDen_US
dc.rights© 2020 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.subjectOSIRIS-RExen_US
dc.subjectBennuen_US
dc.subjectStereophotoclinometryen_US
dc.subjectDigital terrain modelen_US
dc.titleAssessing stereophotoclinometry by modeling a physical wall representing asteroid Bennuen_US
dc.typeArticleen_US
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben_US
dc.identifier.journalPLANETARY AND SPACE SCIENCEen_US
dc.description.noteOpen access articleen_US
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
dc.eprint.versionFinal published versionen_US
dc.identifier.piiS0032063320302907
dc.source.journaltitlePlanetary and Space Science
dc.source.volume193
dc.source.beginpage105077
refterms.dateFOA2020-12-15T20:06:26Z


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© 2020 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
Except where otherwise noted, this item's license is described as © 2020 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).