Geology and Stratigraphic Correlation of the Murray and Carolyn Shoemaker Formations Across the Glen Torridon Region, Gale Crater, Mars

التفاصيل البيبلوغرافية
العنوان: Geology and Stratigraphic Correlation of the Murray and Carolyn Shoemaker Formations Across the Glen Torridon Region, Gale Crater, Mars
المؤلفون: C. M. Fedo, A. B. Bryk, L. A. Edgar, K. A. Bennett, V. K. Fox, W. E. Dietrich, S. G. Banham, S. Gupta, K. M. Stack, R. M. E. Williams, J. P. Grotzinger, N. T. Stein, D. M. Rubin, G. Caravaca, R. E. Arvidson, M. N. Hughes, A. A. Fraeman, A. R. Vasavada, J. Schieber, B. Sutter
المصدر: Journal of Geophysical Research: Planets. 127(9)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2022.
سنة النشر: 2022
مصطلحات موضوعية: Geosciences (General), Lunar and Planetary Science and Exploration
الوصف: The Glen Torridon (GT) region within Gale crater, Mars, occurs in contact with the southern side of Vera Rubin ridge (VRR), a well-defined geomorphic feature that is comparatively resistant to erosion. Prior to detailed ground-based investigation of GT, its geologic relationship with VRR was unknown. Distinct lithologic subunits within the Jura member (Murray formation), which forms the upper part of VRR, made it possible to be also identified within GT. This indicates that the strata pass across the geomorphic divide between regions. Furthermore, the cross-bedded lower part of the overlying Knockfarril Hill member (Carolyn Shoemaker formation) also occurs within both VRR and GT. Correlation of both units demonstrates that the strata form a continuous stratigraphic succession regardless of large-scale geomorphic expression. The lithologic change from mudstone (Jura member) to cross-bedded sandstone (Knockfarril Hill member) heralds a significant shift in paleoenvironment from lacustrine to fluvial. The upper part of the Knockfarril Hill member consists of interbedded mudstone and sandstone that transitions to the overlying finely laminated mudstone of the Glasgow member, and a return to lacustrine deposition. In GT, the Stimson formation unconformably overlies the Glasgow member, where it demarks the southern boundary of GT. Contacts for each stratigraphic unit were defined and transferred to a high-resolution image base to make a geologic map and cross sections perpendicular to the NE strike. Stratal dips cannot exceed 2° NW to retain the positions of stratigraphic units in the locations they are exposed throughout GT.
نوع الوثيقة: Report
اللغة: English
تدمد: 2169-9100
2169-9097
DOI: 10.1029/2022JE007408
URL الوصول: https://ntrs.nasa.gov/citations/20230001590
ملاحظات: NNH15ZDA001 N

CNES 180027

UKSA ST/W002280/1

UKSA ST/N000579/1

UKSA ST/S001492/1

UKSA ST/S001506/1

UKSA ST/T001755/1
رقم الأكسشن: edsnas.20230001590
قاعدة البيانات: NASA Technical Reports
الوصف
تدمد:21699100
21699097
DOI:10.1029/2022JE007408