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- W2170254383 abstract "Introduction: Recently released, high-resolution images from the Mars Orbiter Camera (MOC) and the Thermal Emission Imaging System (THEMIS) reveal a myriad of intriguing landforms banked along the northern edge of Terby Crater located on the northern rim of Hellas (approx.28degS, 287degW). Landforms within this crater include north-trending troughs and ridges, a remarkable 2.5 km-thick sequence of exposed layers, mantled ramps that extend across and between layered sequences, fan-like structures, sinuous channels, collapse pits, a massive landslide and viscous flow features. The suite of diverse landforms in Terby and its immediate surroundings attest to a diversity of rock types and geologic processes, making this locality ideal for studying landform-climate relationships on Mars. In order to decipher the complicated geologic history of Terby Crater and the nature of the layered deposits, a generalized geomorphic map was created and the slope of the layered deposits was examined." @default.
- W2170254383 created "2016-06-24" @default.
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- W2170254383 date "2005-01-01" @default.
- W2170254383 modified "2023-09-28" @default.
- W2170254383 title "Moonshine Versus Earthshine: Physics Makes a Difference" @default.
- W2170254383 hasPublicationYear "2005" @default.
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