Water ice abundance and CO2 band strength on the saturnian satellite Phoebe from Cassini/VIMS observations-Reference-Cited by-同舟云学术

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Water ice abundance and CO2 band strength on the saturnian satellite Phoebe from Cassini/VIMS observations

Published:2012-08 Issue:2 Volume:220 Page:331-338
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Hansen Gary B.,Hollenbeck Emily C.,Stephan Katrin,Apple Sean K.,Shin-White Eun-Ju Z.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference34 articles.

1. Recovering the rotational light curve of Phoebe;Bauer;Astrophys. J.,2004

2. The Cassini Visual and Infrared Mapping Spectrometer (VIMS) investigation;Brown;Space Sci. Rev.,2004

3. Infrared (0.83–5.1μm) photometry of Phoebe from the Cassini visual infrared mapping spectrometer;Buratti;Icarus,2008

4. The evolution of satellite orbits;Burns,1986

5. The spectral reflectance of water–mineral mixtures at low temperatures;Clark;J. Geophys. Res.,1981

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Phoebe's carbon isotope composition as evidence for self-shielding in the solar nebula;Icarus;2020-07

2. Experimenting with Mixtures of Water Ice and Dust as Analogues for Icy Planetary Material;Space Science Reviews;2019-06-24

3. Phoebe: A Surface Dominated by Water;The Astronomical Journal;2018-06-22

4. Cassini's geological and compositional view of Tethys;Icarus;2016-08

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