| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773411 | Icarus | 2012 | 8 Pages |
Abstract
⺠Using Cassini-VIMS spectra, we map the water ice spatial abundance on Phoebe. ⺠The measured abundances are 0.1-4% with grain radii between 1 and 10 μm. ⺠We used dirty ice models to better fit Phoebe spectra. ⺠These models increase the measured spatial abundances by 1.6-12 times. ⺠We measured and mapped the strength of the CO2 band on Phoebe.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Gary B. Hansen, Emily C. Hollenbeck, Katrin Stephan, Sean K. Apple, Eun-Ju Z. Shin-White,