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Hadriacus Mons : ウィキペディア英語版
Hadriacus Mons

Hadriacus Mons is an ancient, low-relief volcanic mountain on the planet Mars, located in the southern hemisphere just northeast of the impact basin Hellas and southwest of the similar volcano Tyrrhenus Mons. It has a diameter of . The name was approved in 2007.〔(【引用サイトリンク】url=http://planetarynames.wr.usgs.gov/Feature/14309 )〕〔(【引用サイトリンク】url=http://itouchmap.com/?r=marsfeatures&z=15946 )〕 The flanks of Hadriacus Mons have been eroded into gullies; its southern slopes are incised by the outflow channel Dao Vallis. The large extent of volcanic deposits and the caldera size leads some researchers to suggest that these features were the result of an explosive event caused by a contact between magma and groundwater.〔Calderón, L.; Robertson, K.; Tovar, D. 2015. (Geomorphologic Evolution of the Zone of Hadriaca Patera in Mars ). 46th Lunar and Planetary Science Conference, 2074.〕
''Hadriaca Patera'', a term formerly used for the entire edifice, is now only used for the central caldera, which is in diameter.〔(【引用サイトリンク】url=http://planetarynames.wr.usgs.gov/Feature/2310 )
== See also==

* List of mountains on Mars
* List of mountains on Mars by height

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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