ライフサイエンスコーパス: Callisto

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1 tosphere) in the vicinity of both Europa and Callisto.

2 nificantly younger than that of Ganymede and Callisto.

3 similar to that of the non-ice components of Callisto and can be attributed to hydrous minerals.

4 evidence for internal liquid water oceans in Callisto and Europa, detection of a strong intrinsic mag

5 surface materials of the Galilean satellites Callisto and Ganymede from analysis of reflectance spect

6 Spectra of Callisto and Ganymede reveal a feature at 4.25 micromete

7 e and a tenuous carbon dioxide atmosphere at Callisto, and detection of condensed oxygen on Ganymede.

8 rock are mixed all the way to the center of Callisto are also consistent with the data.

9 The icy lithospheres of Ganymede and Callisto are equally ice-rich, but Europa's icy shell ha

10 ect information on the interior structure of Callisto determined from previous spacecraft fly-bys was

11 meter have indicated that neither Europa nor Callisto have an appreciable internal magnetic field, in

12 (C10) indicate that the rock and ice within Callisto have partially, but not completely, separated.

13 Callisto may be differentiated into a rock-metal core le

14 galilean satellites-Io, Europa, Ganymede and Callisto-on each orbit.

15 of Jupiter's moons Io, Europa, Ganymede, and Callisto over the past few years.

16 alilean satellites--Io, Europa, Ganymede and Callisto-ranged from uniform mixtures of rock and ice (t

17 Here we report measurements of Callisto's gravitational field which reveal that, in con

18 to a rock-metal core less than 25 percent of Callisto's radius, an outer layer of clean ice less than

19 5 0.5 times the thicknesses of Ganymede's or Callisto's shells, depending on epoch.

20 Callisto's undifferentiated state is consistent with the

21 hs of impact craters on Europa, Ganymede and Callisto that reveal two anomalous transitions in crater

22 ncounter (C3) of the Galileo spacecraft with Callisto, the outermost Galilean moon of Jupiter, indica

23 An off-limb scan of Callisto was conducted by the Galileo near-infrared mapp

24 ost Galilean moon of Jupiter, indicated that Callisto was probably undifferentiated.

25 s to the galilean moons Europa, Ganymede and Callisto, which reside within Jupiter's radiation belts.

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