Harmakhis Vallis
Vallis on Mars
40°24′S 90°24′E / 40.4°S 90.4°E / -40.4; 90.4Harmakhis Vallis is a valley near Hellas Planitia, Mars. It has been identified as an outflow channel, the site of catastrophic floods of water during Mars' past.
Gullies are also common on the wall of Harmakhis Vallis, as seen the image below. Some authors have suggested these structures indicate geologically recent flow of small quantities of water across the surface.[1]
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Gullies in the wall of Harmakhis, as seen by HiRISE.
See also
- Dao Vallis
- Reull Vallis
References
- ^ Heldmann, J. and M. Mellon. Observations of Martian gullies and constraints on potential formation mechanisms. 2004. Icarus. 168: 285-304.
- Further reading
- Bleamaster, L, Crown, D (2004). Morphologic Development of Harmakhis Vallis, Mars (PDF). Lunar and Planetary Science Conference.
{{cite conference}}: CS1 maint: multiple names: authors list (link) - Price, K (1992). Geologic Mapping of Part of Harmakhis Vallis Region, Mars: Evidence of Multiple Drainage Events. Lunar and Planetary Science Conference. Bibcode:1992LPI....23.1107P.
Wikimedia Commons has media related to Harmakhis Vallis.
External links
- HiRISE image of Harmakhis Vallis wall
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