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Science 10 October 1997: Vol. 278. no. 5336, pp. 271 - 275 DOI: 10.1126/science.278.5336.271
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Reports
Organics and Other Molecules in the Surfaces of Callisto and Ganymede
T. B. McCord,
*
R. W. Carlson,
W. D. Smythe,
G. B. Hansen,
R.
N. Clark,
C. A. Hibbitts,
F. P. Fanale,
J. C. Granahan,
M. Segura,
D. L. Matson,
T. V. Johnson,
P.
D. Martin
Five absorption features are reported at wavelengths of 3.4, 3.88, 4.05, 4.25, and 4.57 micrometers in the surface materials of the
Galilean satellites Callisto and Ganymede from analysis of reflectance
spectra returned by the Galileo mission near-infrared mapping
spectrometer. Candidate materials include CO2, organic materials (such as tholins containing C N and C-H),
SO2, and compounds containing an SH-functional group;
CO2, SO2, and perhaps cyanogen [(CN)2] may be present within the surface material itself
as collections of a few molecules each. The spectra indicate that the
primary surface constituents are water ice and hydrated minerals.
T. B. McCord, G. B. Hansen, C. A. Hibbitts, F. P. Fanale, P. D. Martin, Hawaii Institute of Geophysics and
Planetology, University of Hawaii, Honolulu, HI 96822, USA.
R. W. Carlson, W. D. Smythe, M. Segura, D. L. Matson, T. V. Johnson, Jet Propulsion Laboratory, Pasadena, CA
91109, USA.
R. N. Clark, U.S. Geological Survey, Denver, CO
80225-0046, USA.
J. C. Granahan, Science and Technology International,
Incorporated, Honolulu, HI 56813, USA.
*
To whom correspondence should be addressed. E-mail:
tom{at}kahana.pgd.hawaii.edu
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