Definition
Amphitheater-headed elongate depressions (valleys and/or channels) cut into topography on Venus.
Synonyms
Subtypes
- (1)
Valley networks on Venus formed initially from fracture systems and became enlarged by inferred low-viscosity lava sapping processes (Komatsu et al. 2001; Oshigami et al. 2009) (Lava Channel) (Fig. 1).
- (2)
Subsidiary channels associated with chaotic terrain at the source of outflow channels. Example: 5–10 km long valleys or channels at 40°S, 202°E (Kargel et al. 1994).
References
Baker VR, Kochel RC, Laity JE, Howard AD (1990) Spring sapping and valley network development. Geol Soc Am Spec Pap 525:235–266
Baker VR, Komatsu G, Parker TJ, Gulick VC, Kargel JS, Lewis JS (1992) Channels and valleys on Venus: preliminary analysis of Magellan data. J Geophys Res 97(E8):13,421–13,444
Kargel JS, Kirk RL, Fegly B Jr, Treiman AH (1994) Carbonate-sulfate volcanism on Venus? Icarus 112:219–252
Komatsu G, Gulick VC, Baker VR (2001) Valley networks on Venus. Geomorphology 37(3–4):225–240
Komatsu G, Gluick VC, Kargel JS, Baker VR (1992) Venus lava sapping valleys. LPSC XXIII, pp 719–720
Oshigami S, Namiki N, Komatsu G (2009) Depth and longitudinal profiles of Venusian sinuous rilles and valley networks. Icarus 199:250–263. doi:10.1016/j.icarus.2008.10.012
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Komatsu, G., Hargitai, H. (2014). Amphitheater-Headed Valley (Venus). In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_332-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_332-1
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