EARTH SURFACE PROCESSES AND LANDFORMS Earth Surf. Process. Landforms (2011) Copyright © 2011 John Wiley & Sons, Ltd. Published online in Wiley Online Library (wileyonlinelibrary.com) DOI: 10.1002/esp.2266 Spectral and petrologic analyses of basaltic sands in Ka’u Desert (Hawaii) – implications for the dark dunes on Mars Daniela Tirsch,1* Robert Anthony Craddock,2 Thomas Platz,3 Alessandro Maturilli,1 Jörn Helbert1 and Ralf Jaumann13 1 Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany 2 Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA 3 Department of Geological Sciences, Freie Universität, Berlin, Germany Received 30 May 2011; Revised 2 November 2011; Accepted 3 November 2011 *Correspondence to: Daniela Tirsch, Institute of Planetary Research, German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany. E-mail:
[email protected] ABSTRACT: Dark aeolian deposits on Mars are thought to consist of volcanic materials due to their mineral assemblages, which are common to basalts. However, the sediment source is still debated. Basaltic dunes on Earth are promising analogs for providing further insights into the assumed basaltic sand dunes on Mars. In our study we characterize basaltic dunes from the Ka’u Desert in Hawaii using optical microscopes, electron microprobe, and spectral analyses. We compare the spectra of terrestrial and Martian dune sands to determine possible origins of the Martian dark sediments. Our results show that the terrestrial sands consist primarily of medium to coarse sand-sized volcanic glass and rock fragments as well as olivine, pyroxene, and plagioclase minerals. Grain shapes range from angular to subrounded.