Potential for Lava Erosion on Mercury: Modeling the Formation of Both Small and Large Lava Channels

Details Potential for Lava Erosion on Mercury: Modeling the Formation of Both Small and Large Lava Channels Potential for Lava Erosion on Mercury: Modeling the Formation of Both Small and Large Lava Channels

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1055h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1055

Physics

Scientific paper

Features consistent with channelized lava flow and erosion have been
identified in images collected by MESSENGER. Analytical models are used
to estimate potential erosion rates and eruption durations required to
form these observed channels.

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