Heat transfer in volcano-ice interactions on Mars : synthesis of environments and implications for processes and landforms.

• Published in: Annals of Glaciology
• Main Authors: Head, James W., Wilson, Lionel
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: 2007
• Subjects: Moberg; Annals of Glaciology; Ice Sheet
• Online Access: https://eprints.lancs.ac.uk/id/eprint/31120/; https://doi.org/10.3189/172756407782282570

We review new advances in volcano-ice interactions on Mars and focus additional attention on (1) recent analyses of the mechanisms of penetration of the cryosphere by dikes and sills; (2) documentation of the glacial origin of huge fan-shaped deposits on the northwest margins of the Tharis Montes and evidence for abundant volcano-ice interactions during the later Amazonian period of volcanic edifice construction and (3) the circumpolar Hesperian-aged Dorsa Argentea Formation, interpreted as an ice sheet and displaying marginal features (channels, lakes and eskers) indicative of significant melting and interior features interpreted to be due to volcano-ice interactions (e.g. subglacial volcanic edifices, pits, basins, channels and eskers). In this context, we describe and analyse several stages and types of volcano-ice interactions: (1) magmatic interactions with ice-rich parts of the cryosphere; (2) subglacial volcanism represented by intrusion under and into the ice and formation of dikes and moberg-like ridges, intrusion of sills at the glacier-volcano substrate interface and their evolution into subglacial lava flows, formation of subglacial edifices, marginal melting and channels; (3) synglacial (ice contact) volcanism represented by flows banking up against glacier margins, chilling and forming remnant ridges and (4) post-glacial volcanism and interactions with ice deposits.