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dc.contributor.authorJaumann, Ralf
dc.contributor.authorBell, James F.
dc.contributor.authorPolanskey, Carol A.
dc.contributor.authorRaymond, Carol A.
dc.contributor.authorAspaugh, Erik
dc.contributor.authorBercovici, David
dc.contributor.authorBills, Bruce R.
dc.contributor.authorBinzel, Richard
dc.contributor.authorBottke, William
dc.contributor.authorChristoph, John M.
dc.contributor.authorMarchi, Simone
dc.contributor.authorNeesemann, Alicia
dc.contributor.authorOtto, Katharina
dc.contributor.authorPark, Ryan S.
dc.contributor.authorPreusker, Frank
dc.contributor.authorRoatsch, Thomas
dc.date.accessioned2022-03-14T14:00:29Z
dc.date.available2022-03-14T14:00:29Z
dc.date.issued2022-03-08
dc.identifier.urihttps://hdl.handle.net/1721.1/141150
dc.description.abstractAbstract Detailed mapping of topography is crucial for the understanding of processes shaping the surfaces of planetary bodies. In particular, stereoscopic imagery makes a major contribution to topographic mapping and especially supports the geologic characterization of planetary surfaces. Image data provide the basis for extensive studies of the surface structure and morphology on local, regional and global scales using photogeologic information from images, the topographic information from stereo-derived digital terrain models and co-registered spectral terrain information from color images. The objective of the Psyche topography and geomorphology investigation is to derive the detailed shape of (16) Psyche to generate orthorectified image mosaics, which are needed to study the asteroids’ landforms, interior structure, and the processes that have modified the surface over geologic time. In this paper we describe our approaches for producing shape models, and our plans for acquiring requested image data to quantify the expected accuracy of the results. Multi-angle images obtained by Psyche’s camera will be used to create topographic models with about 15 m/pixel horizontal resolution and better than 10 m height accuracy on a global scale. This is slightly better as global imaging obtained during the Dawn mission, however, both missions yield resolutions of a few m/pixel locally. Two different techniques, stereophotogrammetry and stereophotoclinometry, are used to model the shape; these models will be merged with the gravity fields obtained by the Psyche spacecraft to produce geodetically controlled topographic models. The resulting digital topography models, together with the gravity data, will reveal the tectonic, volcanic, impact, and gradational history of Psyche, and enable co-registration of data sets to determine Psyche’s geologic history.en_US
dc.publisherSpringer Netherlandsen_US
dc.relation.isversionofhttps://doi.org/10.1007/s11214-022-00874-7en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer Netherlandsen_US
dc.titleThe Psyche Topography and Geomorphology Investigationen_US
dc.typeArticleen_US
dc.identifier.citationSpace Science Reviews. 2022 Mar 08;218(2):7en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.mitlicensePUBLISHER_CC
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-03-13T04:13:20Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.embargo.termsN
dspace.date.submission2022-03-13T04:13:20Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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