Skip to main content
. Author manuscript; available in PMC: 2018 May 30.
Published in final edited form as: J Geophys Res Planets. 2016 Sep 9;121(10):1865–1884. doi: 10.1002/2016JE005128

Figure 10.

Figure 10

Weathering trends on Ida exhibited with 6-band reflectance spectra obtained by the Galileo mission compared with ordinary chondrite (OC) spectra. Fresh (younger) features have deeper ferrous absorption bands. The weathered terrains have a steeper continuum (red sloped) and have weaker bands. After Chapman [1996].