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Chaotic Terrain (Venus)

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Encyclopedia of Planetary Landforms
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Definition

Chaotically collapsed terrain occurring at the source region of Venusian outflow channels (Kargel et al. 1994).

Formation

Its origin is likely similar to chaotic terrain formation on Mars. Lava suddenly withdrew from a subsurface reservoir while the overlying rock collapsed, and rapid subsequent drainage eroded the channel (Baker et al. 1992; Ford et al. 1993; Komatsu 1993; Kargel et al. 1994).

Prominent Examples

The source region of Kallistos Vallis consists of graben-forming coalesced fractures that are flooded by lava and widened by slumping, collapse, and sapping. Its floor near the edges contains “a chaotic jumble of rocks,” 0.6–2 km across. The chaos area is few 10’s km in diameter (Kargel et al. 1994) (Fig. 1).

Chaotic Terrain (Venus), Fig. 1
figure 377 figure 377

Chaotic source of an outflow valley on Venus, on the southwest flank of Ammavaru volcano (Ford et al. 1993). Scale bar 10 km. Magellan left-looking radar mosaic (NASA/JPL/USGS) (Cf. Fig. 14 from Baker et al. (1992), Fig. 7b from...

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References

  • 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 97:13421–13445

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  • Ford JP, Plaut JJ, Parker TJ (1993) Volcanic features. Chapter 9. In: Ford JP et al (eds) Guide to Magellan image interpretation. NASA, JPL-Caltech, Pasadena

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  • Kargel JS, Kirk RL, Fegly B Jr, Treiman AH (1994) Carbonate–sulfate volcanism on Venus? Icarus 112:219–252

    Article  Google Scholar 

  • Komatsu G (1993) Channels and valleys on Venus. PhD dissertation, University of Arizona

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Correspondence to Henrik Hargitai .

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Hargitai, H. (2015). Chaotic Terrain (Venus). In: Hargitai, H., Kereszturi, Á. (eds) Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-3134-3_47

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