4.5 Article

Geological analysis of Monad Regio, Triton: Possible evidence of endogenic and exogenic processes

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ICARUS
卷 392, 期 -, 页码 -

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ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2022.115368

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Triton; Neptune satellites; Ices; Geological processes; Satellites surfaces

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The surface of Triton is shaped by various endogenic processes like tectonism, volcanism, diapirism, and geyser-like eruptions. A geological analysis of the Monad Regio area was conducted to understand how these processes have influenced the surface. By analyzing Voyager images, a digital elevation model, and a roughness map, a geomorphological map was created to accurately identify known and new landforms. The study also revealed a sequence of endogenic and exogenic processes, including depositional and erosional events involving ice and liquid nitrogen flow.
The surface morphology of Triton is believed to be predominantly influenced by endogenic processes, such as tectonism, volcanism, diapirism and geyser-like eruptions. To understand how some of these processes have reshaped the surface of the satellite during its evolutionary history, we performed a geological analysis of an extended area located in Monad Regio, where several of these endogenic processes may have taken place. We produced a geomorphological map at 1:1,000,000 scale derived from the joint analysis of the Voyager images, a digital elevation model and a roughness map of the study area. Such approach allowed us to delimit with higher accuracy the geomorphological units already known in literature, as planitiae, cantaloupe and smooth terraced terrains, paterae, knobby, and smooth terraced terrains, but it also enabled us to identify new ones (hummocky terrain, inner planitia, inner patera). We reconstructed the relative ages between such terrains, and we found that after an endogenic phase, an exogenic phase could have followed, during which several geological events reshaped the area. These comprise depositional and erosional processes, including the movement of ice and the subglacial flowing of liquid nitrogen. Such observations imply that Monad Regio could be strongly influenced by exogenic processes, perhaps still active today.

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