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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 of the surfaces of icy moons like Europa and Ganymede.
7 gas similar to the atmospheres of Europa and Ganymede.
8 es, such as the Jovian moons Io, Europa, and Ganymede.
9  of tenuous oxygen atmospheres at Europa and Ganymede and a tenuous carbon dioxide atmosphere at Call
10                      The icy lithospheres of Ganymede and Callisto are equally ice-rich, but Europa's
11 ments of depths of impact craters on Europa, Ganymede and Callisto that reveal two anomalous transiti
12 uation applies to the galilean moons Europa, Ganymede and Callisto, which reside within Jupiter's rad
13  of the four galilean satellites-Io, Europa, Ganymede and Callisto-on each orbit.
14 of the four galilean satellites--Io, Europa, Ganymede and Callisto-ranged from uniform mixtures of ro
15  probably significantly younger than that of Ganymede and Callisto.
16                We infer from these data that Ganymede and Europa have persistent interactions with Ju
17 iolet emission from the jovian footprints of Ganymede and Europa.
18  an important part in the formation of O2 on Ganymede and Europa.
19 able internal magnetic field, in contrast to Ganymede and possibly Io.
20 te observations of the surface of Europa and Ganymede and previously available data on NaCl solids.
21 -reflectance measurements of the jovian moon Ganymede, and a tenuous oxygen atmosphere has been obser
22 understanding of Jupiter's moons Io, Europa, Ganymede, and Callisto over the past few years.
23 y bodies, such as Jupiter's moons Europa and Ganymede, and suggestive of a reservoir of radiolytic O(
24 ate on icy moon surfaces like Europa, Titan, Ganymede, Callisto, Enceladus, or Ceres.
25  elevation models of parts of the surface of Ganymede, derived from stereo pairs combining data from
26  of a strong intrinsic magnetic field within Ganymede, discovery of high-temperature silicate volcani
27 observed Jupiter's icy satellites Europa and Ganymede during its flyby in February and March 2007 at
28 ials of the Galilean satellites Callisto and Ganymede from analysis of reflectance spectra returned b
29             Large regions of the jovian moon Ganymede have been resurfaced, but the means has been un
30 260 nanometers on the trailing hemisphere of Ganymede, identified as the Hartley band of Ozone (O3),
31 s that Io has a large metallic core and that Ganymede is strongly differentiated, most probably into
32                                              Ganymede is the only satellite in the solar system known
33 e present the discovery of mass anomalies on Ganymede, Jupiter's third and largest Galilean satellite
34  spacecraft during its second encounter with Ganymede on 6 September 1996 to model the mass anomalies
35 rbital angular velocities of Io, Europa, and Ganymede, respectively.
36                      Spectra of Callisto and Ganymede reveal a feature at 4.25 micrometers, attribute
37 s, and is consistent with partial melting of Ganymede's interior.
38  filling large gaps in compositional maps of Ganymede's Jupiter-facing hemisphere.
39 nd JUICE could use our approach to determine Ganymede's k(2)/Q.
40 cles along partially open field lines within Ganymede's magnetosphere.
41 ture about 0.25 0.5 times the thicknesses of Ganymede's or Callisto's shells, depending on epoch.
42 on of this polar hydrogen peroxide, those of Ganymede's other radiolytic oxidants, and that of hydrog
43 face chemistry across the Jupiter system, to Ganymede's polar regions.
44 riments suggest that the absorption bands in Ganymede's spectrum were not produced in the relatively
45 osphere inverted question mark is trapped in Ganymede's surface ice, an inference consistent with the
46 ce of trapped O3 is thus no longer unique to Ganymede, suggesting that special circumstances may not
47 trometer (NIMS) suggests that the surface of Ganymede, the largest satellite of Jupiter, contains hyd
48 bands in the visible reflectance spectrum of Ganymede, the reflectance of condensed films of pure oxy
49 eld which reveal that, in contrast to Io and Ganymede, this galilean satellite is most probably a hom
50 26 kelvin were similar to those reported for Ganymede, whereas those for the mixtures were slightly s
51 ted by its dynamical interaction with Io and Ganymede, which should cause the equilibrium spin rate o
52 ctromagnetic interactions of Io, Europa, and Ganymede with the magnetospheric plasma flow.