We present new spectra of the leading and trailing hemispheres of Iapetus from 2.4 to 3.8 Β΅m. We have combined the leading hemisphere spectra with previous observations by others to construct a composite spectrum of the dark side (leading) hemisphere from 0.3 to 3.8 Β΅m. We review attempts to deduce
The roughness of the dark side of Iapetus from the 2004 to 2005 flyby
β Scribed by Janice S. Lee; Bonnie J. Buratti; Michael Hicks; Joel Mosher
- Book ID
- 103830618
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 930 KB
- Volume
- 206
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
β¦ Synopsis
The roughness of a planetary surface offers clues to its past geologic history. We apply a surface roughness model developed by
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