E-mail a Wiley Online Library Link

Teemu Öhman and David A. Kring Photogeologic analysis of impact melt-rich lithologies in Kepler crater that could be sampled by future missions Journal of Geophysical Research: Planets (1991–2012) 117

Version of Record online: 15 FEB 2012 | DOI: 10.1029/2011JE003918

Key Points

  • Impact melt-rich lithologies are observed asymmetrically in and around Kepler
  • Impact melt flows imply a yield strength of ~1-10 kPa
  • Fractures and pits (possible caves) are abundant in melt-rich crater floor

Complete the form below and we will send an e-mail message containing a link to the selected article on your behalf

Required = Required Field