NASA Scientific and Technical Aerospace Reports - The University ...
NASA Scientific and Technical Aerospace Reports - The University ...
NASA Scientific and Technical Aerospace Reports - The University ...
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20100017207 <strong>NASA</strong>, Washington, DC, USA<br />
Geologic Mapping of Holden Crater <strong>and</strong> the Uzboi-Ladon-Morava Outflow System<br />
Grant, J. A.; Irwin, R. P., III; Wilson, S. A.; Abstracts of the Annual Meeting of Planetary Geologic Mappers, San Antonio,<br />
TX, 2009; June 2009, pp. 25-26; In English; See also 20100017196; Original contains color illustrations; Copyright;<br />
Avail.: CASI: A01, Hardcopy<br />
ONLINE: http://hdl.h<strong>and</strong>le.net/2060/20100017207<br />
Geologic mapping in Margaritifer Terra (Fig. 1) yields important new information regarding the inventory, sources, <strong>and</strong><br />
sinks of water during the Noachian <strong>and</strong> early Hesperian on Mars [1-7]. Drainage in southwest Margaritifer Terra is dominated<br />
by the segmented Uzboi-Ladon-Morava (ULM) meso-scale outflow system that traverses northward along the southwestern<br />
flank of the Chryse trough [4-9]. Mapping of lower Uzboi Vallis through Ladon basin highlights the extent <strong>and</strong> complexity<br />
of sedimentary deposits associated with the ULM system [5-13].<br />
Author<br />
Geological Surveys; Mars Surface; Drainage; Craters; Mars 1 Spacecraft; Segments<br />
20100017208 <strong>NASA</strong>, Washington, DC, USA<br />
Geology of the Southern Utopia Planitia Highl<strong>and</strong>-Lowl<strong>and</strong> Boundary Plain: Second Year Results <strong>and</strong> Third Year Plan<br />
Skinner, J. A., Jr.; Tanaka, K. L.; Hare, T. M.; Abstracts of the Annual Meeting of Planetary Geologic Mappers, San Antonio,<br />
TX, 2009; June 2009, pp. 39-40; In English; See also 20100017196; Original contains color illustrations; Copyright;<br />
Avail.: CASI: A01, Hardcopy<br />
ONLINE: http://hdl.h<strong>and</strong>le.net/2060/20100017208<br />
<strong>The</strong> southern Utopia highl<strong>and</strong>-lowl<strong>and</strong> boundary (HLB) extends >1500 km westward from Hyblaeus Dorsa to the<br />
topographic saddle that separates Isidis <strong>and</strong> Utopia Planitiae. It contains bench-like platforms that contain depressions, pitted<br />
cones (some organized into arcuate chains <strong>and</strong> thumb-print terrain), isolated domes, buried circular depressions, ring fractures,<br />
polygonal fractures, <strong>and</strong> other locally- to regionally-dispersed l<strong>and</strong>forms [1-2]. <strong>The</strong> objective of this map project is to clarify<br />
the geologic evolution of the southern Utopia Planitia HLB by identifying the geologic, structural, <strong>and</strong> stratigraphic<br />
relationships of surface materials in MTMs 10237, 15237, 20237, 10242, 15242, 20242, 10247, 15247, <strong>and</strong> 20247. <strong>The</strong> project<br />
was originally awarded in April, 2007 <strong>and</strong> is in its final year of support. Mapping is on-schedule <strong>and</strong> formal map submission<br />
will occur by December, 2009, with finalization anticipated by April, 2010. Herein, we (1) review specifics regarding mapping<br />
data <strong>and</strong> methods, (2) present nomenclature requests that we feel will assist with unit descriptions, (3) describe Year 2 mapping<br />
<strong>and</strong> science accomplishments, <strong>and</strong> (4) outline Year 3 technical <strong>and</strong> managerial approaches for finalizing the geologic map.<br />
Author<br />
Geology; Mars Surface; Surface Properties; Topography; Highl<strong>and</strong>s; L<strong>and</strong>forms; Stratigraphy<br />
20100017209 <strong>NASA</strong>, Washington, DC, USA<br />
Mars Global Geologic Mapping: About Half Way Done<br />
Tanaka, K. L.; Dohm, J. M.; Irwin, R.; Kolb, E. J.; Skinner, J. A., Jr.; Hare, T. M.; Abstracts of the Annual Meeting of Planetary<br />
Geologic Mappers, San Antonio, TX, 2009; June 2009, pp. 41-42; In English; See also 20100017196; Original contains color<br />
illustrations; Copyright; Avail.: CASI: A01, Hardcopy<br />
ONLINE: http://hdl.h<strong>and</strong>le.net/2060/20100017209<br />
We are in the third year of a five-year effort to map the geology of Mars using mainly Mars Global Surveyor, Mars<br />
Express, <strong>and</strong> Mars Odyssey imaging <strong>and</strong> altimetry datasets. Previously, we have reported on details of project management,<br />
mapping datasets (local <strong>and</strong> regional), initial <strong>and</strong> anticipated mapping approaches, <strong>and</strong> tactics of map unit delineation <strong>and</strong><br />
description [1-2]. For example, we have seen how the multiple types <strong>and</strong> huge quantity of image data as well as more accurate<br />
<strong>and</strong> detailed altimetry data now available allow for broader <strong>and</strong> deeper geologic perspectives, based largely on improved<br />
l<strong>and</strong>form perception, characterization, <strong>and</strong> analysis. Here, we describe mapping <strong>and</strong> unit delineation results thus far, a new unit<br />
identified in the northern plains, <strong>and</strong> remaining steps to complete the map.<br />
Author<br />
Mars Surface; Planetary Geology; L<strong>and</strong>forms; 2001 Mars Odyssey; Mars Global Surveyor<br />
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