Long-Wavelength Topographic Change on Mercury: Evidence and Mechanisms

Details Long-Wavelength Topographic Change on Mercury: Evidence and Mechanisms Long-Wavelength Topographic Change on Mercury: Evidence and Mechanisms

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1578s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1578

Physics

Scientific paper

Orbital observations by the MESSENGER spacecraft show that Mercury
experienced marked changes in long-wavelength topography more recently
than the end of late heavy bombardment and the volcanic emplacement of
the largest expanses of smooth plains.

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