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21 - Spectral Analyses of Saturn’s Moons Using the Cassini Visual Infrared Mapping Spectrometer

from Part IV - Applications to Planetary Surfaces

Published online by Cambridge University Press:  15 November 2019

Janice L. Bishop
Affiliation:
SETI Institute, California
James F. Bell III
Affiliation:
Arizona State University
Jeffrey E. Moersch
Affiliation:
University of Tennessee, Knoxville
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Summary

The Cassini Visual Infrared Mapping Spectrometer (VIMS) spans a wavelength range of 0.34 to 5.2 µm. Executing numerous close targeted flybys of the major moons of Saturn, as well as serendipitous flybys of the smaller moons, VIMS gathered millions of spectra of these bodies during its 13-year mission, some at spatial resolutions of a few hundred meters. The surfaces of the inner moons are dominated by water ice, while Iapetus, Hyperion, and Titan have substantial amounts of dark materials, including hydrocarbons, on their surfaces. Phoebe is grayer in color in the visible than Saturn’s other low-albedo moons. The surfaces of the inner small moons are also dominated by water ice, and they share compositional similarities to the main rings. The optical properties of the main moons are affected by particles from Saturn’s rings: the inner moons are coated by the E-ring, which originates from cryoactivity on Enceladus, while Iapetus and Hyperion are coated by particles from the Phoebe ring. Cassini VIMS detected previously unknown volatiles and organics on these moons, including CO2, H2, organic molecules as complex as aromatic hydrocarbons, nano-iron, and nano-iron oxides.

Type
Chapter
Information
Remote Compositional Analysis
Techniques for Understanding Spectroscopy, Mineralogy, and Geochemistry of Planetary Surfaces
, pp. 428 - 441
Publisher: Cambridge University Press
Print publication year: 2019

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References

Barnes, J.W., Brown, R.H., Soderblom, L., et al. (2008) Spectroscopy, morphometry, and photoclinometry of Titan’s dunefields from Cassini/VIMS. Icarus, 195, 400414.CrossRefGoogle Scholar
Barnes, J.W., Bow, J., Schwartz, J., et al. (2011) Organic sedimentary deposits in Titan’s dry lakebeds: Probable evaporite. Icarus, 216, 136140.CrossRefGoogle Scholar
Brown, R.H., Baines, K.H., Bellucci, G., et al. (2004) The Cassini visual and infrared mapping spectrometer (VIMS) investigation. Space Science Reviews, 115, 111168.Google Scholar
Brown, R.H., Clark, R.N., Buratti, B.J., et al. (2006) Composition and physical properties of Enceladus’ surface. Science, 311, 14251428.CrossRefGoogle ScholarPubMed
Brown, R.H., Soderblom, L.A., Soderblom, J.M., et al. (2008) The identification of liquid ethane in Titan’s Ontario Lacus. Nature, 454, 607610.CrossRefGoogle ScholarPubMed
Brown, R.H., Lauretta, D.S., Schmidt, B., & Moores, J. (2012) Experimental and theoretical simulations of ice sublimation with implications for the chemical, isotopic, and physical evolution of icy objects. Planetary and Space Science, 60, 166180.CrossRefGoogle Scholar
Buratti, B.J., Mosher, J.A., & Johnson, T.V. (1990) Albedo and color maps of the saturnian satellites. Icarus, 87, 339357.CrossRefGoogle Scholar
Buratti, B.J., Cruikshank, D.P., Brown, R.H., et al. (2005) Cassini visual and infrared mapping spectrometer observations of Iapetus: Detection of CO2. The Astrophysical Journal Letters, 622, L149L152.Google Scholar
Buratti, B.J., Sotin, C., Brown, R.H., et al. (2006) Titan: Preliminary results on surface properties and photometry from VIMS observations of the early flybys. Planetary and Space Science, 54, 14981509.CrossRefGoogle Scholar
Buratti, B.J., Bauer, J.M., Hicks, M.D., et al. (2010) Cassini spectra and photometry 0.25–5.1 μm of the small inner satellites of Saturn. Icarus, 206, 524536.CrossRefGoogle Scholar
Clark, R.N., Brown, R.H., Jaumann, R., et al. (2005) Compositional maps of Saturn’s moon Phoebe from imaging spectroscopy. Nature, 435, 6669.CrossRefGoogle ScholarPubMed
Clark, R.N., Curchin, J.M., Jaumann, R., et al. (2008) Compositional mapping of Saturn’s satellite Dione with Cassini VIMS and implications of dark material in the Saturn system. Icarus, 193, 372386.CrossRefGoogle Scholar
Clark, R.N., Curchin, J.M., Barnes, J.W., et al. (2010) Detection and mapping of hydrocarbon deposits on Titan. Journal of Geophysical Research, 115, E10005, DOI:10.1029/2009JE003369.CrossRefGoogle Scholar
Clark, R.N., Cruikshank, D.P., Jaumann, R., et al. (2012) The surface composition of Iapetus: Mapping results from Cassini VIMS. Icarus, 218, 831860.Google Scholar
Clark, R.N., Brown, R.H., & Lytle, D.M. (2016) The VIMS wavelength and radiometric calibration. NASA Planetary Data System, The Planetary Atmospheres Node, https://atmos.nmsu.edu/data_and_services/atmospheres_data/Cassini/vims_2.html.Google Scholar
Cruikshank, D.P., Owen, T.C., Dalle Ore, C., et al. (2005) A spectroscopic study of the surfaces of Saturn’s large satellites: H2O ice, tholins, and minor constituents. Icarus, 175, 268283.CrossRefGoogle Scholar
Cruikshank, D.P., Dalton, J.B., Dalle Ore, C.M., et al. (2007) Surface composition of Hyperion. Nature, 448, 5456.CrossRefGoogle ScholarPubMed
Cruikshank, D.P., Wegryn, E., Dalle Ore, C., et al. (2008) Hydrocarbons on Saturn’s satellites Iapetus and Phoebe. Icarus, 193, 334343.CrossRefGoogle Scholar
Cruikshank, D.P., Meyer, A.W., Brown, R.H., et al. (2010) Carbon dioxide on the satellites of Saturn: Results from the Cassini VIMS investigation and revisions to the VIMS wavelength scale. Icarus, 206, 561572.CrossRefGoogle Scholar
Cruikshank, D.P., Dalle Ore, C.M., Clark, R.N., & Pendleton, Y.J. (2014) Aromatic and aliphatic organic materials on Iapetus: Analysis of Cassini VIMS data. Icarus, 233, 306315.Google Scholar
Dalton, J.B. III, Cruikshank, D.P., & Clark, R.N. (2012) Compositional analysis of Hyperion with the Cassini Visual and Infrared Mapping Spectrometer. Icarus, 220, 752776.CrossRefGoogle Scholar
Denk, T., Neukum, G., Roatsch, T., et al. (2010) Iapetus: Unique surface properties and a global color dichotomy from Cassini imaging. Science, 327, 435439.Google Scholar
Emery, J.P., Burr, D.M., Cruikshank, D.P., Brown, R.H., & Dalton, J.B. (2005) Near-infrared (0.8–4.0 µm) spectroscopy of Mimas, Enceladus, Tethys, and Rhea. Astronomy and Astrophysics, 435, 353362.Google Scholar
Filacchione, G., Capaccioni, F., Clark, R., et al. (2010) Saturn’s icy satellites investigated by Cassini–VIMS: II. Results at the end of nominal mission. Icarus, 206, 507523.Google Scholar
Filacchione, G., Capaccioni, F., Ciarniello, M., et al. (2012) Saturn’s icy satellites and rings investigated by Cassini–VIMS: III–Radial compositional variability. Icarus, 220, 10641096.Google Scholar
Filacchione, G., Capaccioni, F., Clark, R.N., et al. (2013) The radial distribution of water ice and chromophores across Saturn’s system. The Astrophysical Journal, 766, 76.Google Scholar
Gladman, B., Kavelaars, J., Holman, M., et al. (2001) Discovery of 12 satellites of Saturn exhibiting orbital clustering. Nature, 412, 163166.Google Scholar
Goguen, J.D., Buratti, B.J., Brown, R.H., et al. (2013) The temperature and width of an active fissure on Enceladus measured with Cassini VIMS during the 14 April 2012 South Pole flyover. Icarus, 226, 11281137.CrossRefGoogle Scholar
Grav, T. & Bauer, J. (2007) A deeper look at the colors of the saturnian irregular satellites. Icarus, 191, 267285.CrossRefGoogle Scholar
Griffith, C.A., Owen, T., Geballe, T.R., Rayner, J., & Rannou, P. (2003) Evidence for the exposure of water ice on Titan’s surface. Science, 300, 628630.Google Scholar
Hayne, P.O., McCord, T.B., & Sotin, C. (2014) Titan’s surface composition and atmospheric transmission with solar occultation measurements by Cassini VIMS. Icarus, 243, 158172.CrossRefGoogle Scholar
Howett, C.J.A., Spencer, J.R., Schenk, P., et al. (2011) A high-amplitude thermal inertia anomaly of probable magnetospheric origin on Saturn’s moon Mimas. Icarus, 216, 221226.CrossRefGoogle Scholar
Howett, C.J.A., Spencer, J.R., Hurford, T., Verbiscer, A., & Segura, M. (2012) PacMan returns: An electron-generated thermal anomaly on Tethys. Icarus, 221, 10841088.CrossRefGoogle Scholar
Howett, C.J.A., Spencer, J.R., Hurford, T., Verbiscer, A., & Segura, M. (2014) Thermophysical property variations across Dione and Rhea. Icarus, 241, 239247.Google Scholar
Jewitt, D. & Haghighipour, N. (2007) Irregular satellites of the planets: Products of capture in the early Solar System. Annual Review of Astronomy and Astrophysics, 45, 261295.Google Scholar
Johnson, T.V. & Lunine, J.I. (2005) Saturn’s moon Phoebe as a captured body from the outer Solar System. Nature, 435, 6971.Google Scholar
Kokaly, R.F., Clark, R.N., Swayze, G.A., et al. (2017) USGS spectral library version 7, https://dx.doi.org/10.5066/F7RR1WDJ. https://speclab.cr.usgs.gov/spectral-lib.html. US Geological Survey.Google Scholar
McBride, N., Hillier, J., Green, S., et al. (2007) Cassini cosmic dust analyser: Composition of dust at Saturn. Workshop on Dust in Planetary Systems, 107–110.Google Scholar
McCord, T.B., Hansen, G.B., Buratti, B.J., et al. (2006) Composition of Titan’s surface from Cassini VIMS. Planetary and Space Science, 54, 15241539.Google Scholar
McCord, T.B., Hayne, P., Combe, J.-P., et al. (2008) Titan’s surface: Search for spectral diversity and composition using the Cassini VIMS investigation. Icarus, 194, 212242.Google Scholar
Paranicas, C., Roussos, E., Krupp, N., et al. (2012) Energetic charged particle weathering of Saturn’s inner satellites. Planetary and Space Science, 61, 6065.CrossRefGoogle Scholar
Porco, C.C., Helfenstein, P., Thomas, P.C., et al. (2006) Cassini observes the active south pole of Enceladus. Science, 311, 13931401.Google Scholar
Postberg, F., Schmidt, J., Hillier, J., Kempf, S., & Srama, R. (2011) A salt-water reservoir as the source of a compositionally stratified plume on Enceladus. Nature, 474, 620622.Google Scholar
Schenk, P., Hamilton, D.P., Johnson, R.E., et al. (2011) Plasma, plumes and rings: Saturn system dynamics as recorded in global color patterns on its midsize icy satellites. Icarus, 211, 740757.Google Scholar
Schenk, P.M., Buratti, B., Byrne, P., McKinnon, W.B., Nimmo, F., & Scipioni, F. (2015) Blood stains on Tethys: Evidence of recent activity. American Geophysical Union, Fall Meeting 2015, Abstract #P21B-02.Google Scholar
Spencer, J.R., Pearl, J.C., Segura, M., et al. (2006) Cassini encounters Enceladus: Background and the discovery of a south polar hot spot. Science, 311, 14011405.CrossRefGoogle ScholarPubMed
Squyres, S.W., Buratti, B., Veverka, J., & Sagan, C. (1984) Voyager photometry of Iapetus. Icarus, 59, 426435.Google Scholar
Tamayo, D., Burns, J.A., Hamilton, D.P., & Hedman, M.M. (2011) Finding the trigger to Iapetus’ odd global albedo pattern: Dynamics of dust from Saturn’s irregular satellites. Icarus, 215, 260278.CrossRefGoogle Scholar
Thomas, P.C., Burns, J.A., Hedman, M., et al. (2013) The inner small satellites of Saturn: A variety of worlds. Icarus, 226, 9991019.Google Scholar
Verbiscer, A.J., Peterson, D.E., Skrutskie, M.F., et al. (2006) Near-infrared spectra of the leading and trailing hemispheres of Enceladus. Icarus, 182, 211223.Google Scholar
Verbiscer, A.J., French, R., Showalter, M., & Helfenstein, P. (2007) Enceladus: Cosmic graffiti artist caught in the act. Science, 315, 815817.CrossRefGoogle Scholar
Verbiscer, A.J., Skrutskie, M.F., & Hamilton, D.P. (2009) Saturn’s largest ring. Nature, 461, 10981100.Google Scholar

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