Enhanced Groundwater Flow on and Below Vera Rubin Ridge, the Murray Formation, Gale Crater: Evidence from Thermochemical Modeling.

التفاصيل البيبلوغرافية
العنوان: Enhanced Groundwater Flow on and Below Vera Rubin Ridge, the Murray Formation, Gale Crater: Evidence from Thermochemical Modeling.
المؤلفون: Hicks, L. J., Rampe, E. B., McAdam, A., Kirnbauer, T., Bridges, J. C., Parnell, J., Reed, M. H., Mangold, N., Schwenzer, S. P., Fraeman, A. A., Turner, S. M. R., Bedford, C. C., Achilles, C. N.
المصدر: CASI
سنة النشر: 2020
المجموعة: NASA Technical Reports Server (NTRS)
مصطلحات موضوعية: Space Sciences (General)
جغرافية الموضوع: Unclassified, Unlimited, Publicly available
الوصف: NASAs Mars Science Laboratory Curiosity rover has been exploring Vera Rubin ridge (VRR), part of the Murray formation in Gale crater, Mars, between sol 1809 and 2302. Evidence for Fe-oxides and phyllosilicates in mineralogical and geochemical data for this region was returned by Curiosity [1-5]. We applied thermochemical modeling to con-strain the formation conditions of the phyllosilicate-hematite assemblage identified on and below VRR. Average alteration compositions for the Murray formation on and below VRR were derived using CheMin and APXS data. These compositions were reacted with Gale Portage Water (GPW) between 25100 C and for 10% and 50% Fe3+/Fetot of the host rock [6]. Here we summarize models run at 50 C and 10% Fe3+/Fetot for alteration compositions derived from Murray host rock compositions.
نوع الوثيقة: other/unknown material
وصف الملف: application/pdf
اللغة: unknown
العلاقة: Document ID: 20200001795; http://hdl.handle.net/2060/20200001795Test
الإتاحة: http://hdl.handle.net/2060/20200001795Test
حقوق: Copyright, Public use permitted
رقم الانضمام: edsbas.9FF74745
قاعدة البيانات: BASE