Jupiter's moon Amalthea
was probably captured
NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN
Posted: December 24, 2004
In addition to the Galilean moons, Jupiter has two other types of satellites: four small inner moons orbiting Jupiter within the orbit of Io, the inner most Galilean satellite, and at least fifty five small outer moons outside the orbit of Callisto, the outer most Galilean satellite. All the outer satellites have tell-tale orbits that reveal that they must have been captured by Jupiter during or after the formation of the planet and its larger moons.
The origin of the four small inner moons remain a mystery, however. They have orbits compatible with the hypothesis that they formed in orbit around Jupiter like the Galilean moons. On the other hand, their small irregular shapes and their comparatively low reflectivity and low densities resemble asteroids and suggest that they were captured by Jupiter's gravitational pull just like the outer moons.
The mystery persists because of the challenge inherent in observing Jupiter's small inner moons from Earth. The moons are small and therefore faint, and they are obscured by the bright glare from Jupiter. Although NASA's space probes Voyager and Galileo have captured detailed images of Jupiter's small inner moons, these data have been insufficient for resolving the question of their origin.
Naruhisa Takato from the National Astronomical Observatory of Japan and his collaborators have now had success in obtaining the first infrared spectrum of two of Jupiter's small inner moons, Amalthea and Thebe. To obtain a spectrum over a wide range of infrared wavelengths, the group combined the strengths of two instruments on two telescopes on the summit of Mauna Kea, Hawaii. For high resolution spectroscopy at wavelengths longer than 3 µm ,the group used the Infrared Camera and Spectrograph on the Subaru telescope. For shorter wavelengths, the group used SpeX on the NASA IRTF, which has broad wavelength coverage.
The new spectrum of Amalthea shows the characteristic signatures of water. The most likely location of this water is within water containing hydrous minerals. Such minerals typically form in low temperature environments, ruling out the possibility that Amalthea could have formed in the high temperature environment of Jupiter's immediate neighbourhood while the planet was forming and where Amalthea now is.
If Amalthea did not form near its present location, where did it come from? The surface of Amalthea resembles regions of Callisto that are not covered by ice. This suggests that Amalthea may have been one of the many small "micro-satellites" orbiting Jupiter that was sucked into an inner orbit when the Galilean moons formed. However, the spectrum of Amalthea has similarities with asteroids orbiting the Sun, suggesting that is was a "micro-planet" that was pulled into Jupiter's orbit when Jupiter itself was forming.
Takato says "although we think Jupiter's moons formed as an assembly of many smaller bodies, the same
way we think planets formed from 'planetesimals', until now we have not found any example of the
original building blocks of a planet's moon. However, our results strengthen the argument that Amalthea
is one of the few remaining pieces of the material that formed the Galilean moons. Amalthea may have
ended up in orbit close to Jupiter rather than get incorporated into a larger moon or Jupiter itself.
If this is the case, Amalthea would be the first known example of a 'satellitesimal.'"
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