Xanthe Terra
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- Brock Walmsley Jonathan 2019.Pdf (13.47Mb)
- Geologic Mapping and Spectral Analyses of the Source Region of Shalbatana Vallis, Mars
- Arxiv:1404.3858V1 [Astro-Ph.EP] 15 Apr 2014 Hesperian (Approximately 3.7–3.3 Ga) Outflow Channels (Nel- Where Water That Was Discharged Was Replaced by Recharge
- Evidences of Possible Hydrothermal Alteration in Xanthe Terra: Implications for Surface Water on Early Mars
- Mars Pathfinder Landing Site Workshop Ii: Characteristics of the Ares Vallis Region and Field Trips in the Channeled Scabland, Washington
- The Hypanis Valles Delta: the Last Highstand of a Sea on Early Mars? ∗ Peter Fawdon A, , Sanjeev Gupta B, Joel M