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Geologic Mapping Methods for a Mission-Driven Mapping Scenario: The Dawn at Vesta Example

Yingst, R.A. and Mest, S.C. and Williams, D.A. and Garry, W.B. and Berman, D.C. and Pieters, C. and Jaumann, R. (2013) Geologic Mapping Methods for a Mission-Driven Mapping Scenario: The Dawn at Vesta Example. GSA, Anniversary Annual Meeting & Exposition, 2013-10-27 - 2013-10-30, Denver, USA.

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Abstract

We report on methods used to create a global geologic map of Vesta based on data from the Dawn spacecraft’s High-Altitude Mapping Orbit (HAMO) data. Each of Dawn’s several orbital phases at Vesta provided increasingly higher spatial resolution data that fed into three main iterations of the global map. The first iteration was created during the approach phase and was based on clear filter data from the Framing Camera (FC), which at this stage covered the surface at 3-9 km/pixel resolution. The second iteration used FC clear filter data at ~200 m/pixel resolution and a Digital Terrain Model derived from image data acquired during Survey orbit. The third iteration was based on data from the High-Altitude Mapping Orbit (HAMO; spatial resolution ~61 m/pixel). We mapped three broad terrain types: heavily-cratered, ridge-and-trough (equatorial and northern fossae), and terrain associated with the Rheasilvia and Veneneia impact structures. Local features include bright and dark material and ejecta, lobate deposits, and mass-wasting materials. Stratigraphy of Vesta’s geologic units suggests a history in which primary crust formation was followed by first the Veneneia and then the Rheasilvia impact events, along with associated structural deformation that shaped the Saturnalia and Divalia Fossae Formations respectively. Subsequent impacts and mass wasting events subdued impact craters and parts of ridge-and-trough sets, and formed slumps and landslides. Discontinuous low-albedo deposits also formed or were emplaced; these lie stratigraphically above the equatorial fossae. The youngest features are bright-rayed craters and other surface mantling deposits. Lessons learned in this mapping effort include: (1) iterative mapping provides teams with a robust way to organize knowns and unknowns, feeding forward into subsequent science decisions; (2) the process must include enough people working concurrently as well as collaboratively and individually, to be efficient enough to serve tactical needs; and (3) generic descriptors of features should be retained for as long as possible — during the iterative mapping process, ideally until features can be observed with the highest resolution. This lessens bias and potentially reduces confusion (among the team and the community) as feature interpretations evolve.

Item URL in elib:https://elib.dlr.de/86776/
Document Type:Conference or Workshop Item (Speech)
Title:Geologic Mapping Methods for a Mission-Driven Mapping Scenario: The Dawn at Vesta Example
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Yingst, R.A.Planetary Science Institute, 1700 E. Ft. Lowell, Suite 106, Tucson, AZ, 85719, USAUNSPECIFIEDUNSPECIFIED
Mest, S.C.Planetary Science Institute,Tucson, AZUNSPECIFIEDUNSPECIFIED
Williams, D.A.Arizona State UniversityUNSPECIFIEDUNSPECIFIED
Garry, W.B.Planetary Science Institute, Tucson, AZ, USAUNSPECIFIEDUNSPECIFIED
Berman, D.C.Planetary Science Institute, 1700 E. Ft. Lowell, Suite 106, Tucson, AZ, 85719, USAUNSPECIFIEDUNSPECIFIED
Pieters, C.Brown University, Providence, RI, USAUNSPECIFIEDUNSPECIFIED
Jaumann, R.ralf.jaumann (at) dlr.deUNSPECIFIEDUNSPECIFIED
Date:28 October 2013
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:DAWN, Vesta
Event Title:GSA, Anniversary Annual Meeting & Exposition
Event Location:Denver, USA
Event Type:international Conference
Event Start Date:27 October 2013
Event End Date:30 October 2013
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - Project DAWN (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Geology
Deposited By: Voigt, Joana
Deposited On:17 Dec 2013 07:01
Last Modified:24 Apr 2024 19:53

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