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Hrad Vallis information


Hrad Vallis
Hrad Vallis may have been formed when the large Elysium Mons volcanic complex melted ground ice, as seen by THEMIS.
Coordinates38°42′N 224°42′W / 38.7°N 224.7°W / 38.7; -224.7

Hrad Vallis is an ancient outflow channel in the Cebrenia quadrangle of Mars, located at 38.7° north latitude and 224.7° west longitude. It is 825 km in length and was named for the word for "Mars" in Armenian.[1]

  1. ^ "Hrad Vallis". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Retrieved 2014-07-11. {{cite web}}: External link in |work= (help)

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Hrad Vallis

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Hrad Vallis is an ancient outflow channel in the Cebrenia quadrangle of Mars, located at 38.7° north latitude and 224.7° west longitude. It is 825 km...

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Utopia Planitia

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along Hrad Vallis, as seen by CTX. Photo labeled with layers, streamlined forms, and arrow indicating direction water flowed. Layers exposed along Hrad Vallis...

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Volcanism on Mars

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debris flows (lahars). Some channels in Martian volcanic areas, such as Hrad Vallis near Elysium Mons, may have been similarly carved or modified by lahars...

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Cebrenia quadrangle

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Hrad Vallis in the Cebrenia quadrangle is close to Elysium Mons, a large volcano, which may have supplied water to create the channel. Hrad Vallis is...

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List of valles on Mars

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languages, while small ones are named for rivers. "Planetary Names: Vallis, valles: Neretva Vallis on Mars". planetarynames.wr.usgs.gov. Gazetteer of Planetary...

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Outflow channels

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Ares Vallis (Aram Chaos; Iani Chaos) Kasei Vallis (Echus Chasma) Maja Valles (Juventae Chasma) Mawrth Vallis (no obvious source) Ravi Vallis (Aromatum...

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Epenthesis

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Polish gród, Old Church Slavonic градъ gradŭ, Serbo-Croatian grad and Czech hrad. Another environment can be observed in the history of Modern Persian, in...

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