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1 nance linking Jupiter's moons Io, Europa and Ganymede.
2 that which links Jupiter with Io, Europa and Ganymede.
3 llisto, and detection of condensed oxygen on Ganymede.
4 also not predicted before being observed on Ganymede.
5 gen atmospheres recently found on Europa and Ganymede.
6 gas similar to the atmospheres of Europa and Ganymede.
7 of tenuous oxygen atmospheres at Europa and Ganymede and a tenuous carbon dioxide atmosphere at Call
9 ments of depths of impact craters on Europa, Ganymede and Callisto that reveal two anomalous transiti
10 uation applies to the galilean moons Europa, Ganymede and Callisto, which reside within Jupiter's rad
12 of the four galilean satellites--Io, Europa, Ganymede and Callisto-ranged from uniform mixtures of ro
18 -reflectance measurements of the jovian moon Ganymede, and a tenuous oxygen atmosphere has been obser
20 y bodies, such as Jupiter's moons Europa and Ganymede, and suggestive of a reservoir of radiolytic O(
21 elevation models of parts of the surface of Ganymede, derived from stereo pairs combining data from
22 of a strong intrinsic magnetic field within Ganymede, discovery of high-temperature silicate volcani
23 observed Jupiter's icy satellites Europa and Ganymede during its flyby in February and March 2007 at
24 ials of the Galilean satellites Callisto and Ganymede from analysis of reflectance spectra returned b
26 260 nanometers on the trailing hemisphere of Ganymede, identified as the Hartley band of Ozone (O3),
27 s that Io has a large metallic core and that Ganymede is strongly differentiated, most probably into
28 e present the discovery of mass anomalies on Ganymede, Jupiter's third and largest Galilean satellite
29 spacecraft during its second encounter with Ganymede on 6 September 1996 to model the mass anomalies
34 ture about 0.25 0.5 times the thicknesses of Ganymede's or Callisto's shells, depending on epoch.
35 riments suggest that the absorption bands in Ganymede's spectrum were not produced in the relatively
36 osphere inverted question mark is trapped in Ganymede's surface ice, an inference consistent with the
37 ce of trapped O3 is thus no longer unique to Ganymede, suggesting that special circumstances may not
38 trometer (NIMS) suggests that the surface of Ganymede, the largest satellite of Jupiter, contains hyd
39 bands in the visible reflectance spectrum of Ganymede, the reflectance of condensed films of pure oxy
40 eld which reveal that, in contrast to Io and Ganymede, this galilean satellite is most probably a hom
41 26 kelvin were similar to those reported for Ganymede, whereas those for the mixtures were slightly s
42 ted by its dynamical interaction with Io and Ganymede, which should cause the equilibrium spin rate o
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