The surface of Amalthea is the reddest in the
Solar System. This color may be due to
sulfur originating from
Io or some other non-ice material. Bright patches of less-red tint appear on the major slopes of Amalthea, but the nature of this color is currently unknown. The surface of Amalthea is slightly brighter than surfaces of other
inner satellites of Jupiter. There is also a substantial asymmetry between the leading and trailing
hemispheres: the leading hemisphere is 1.3 times brighter than the trailing one. The asymmetry is probably caused by the higher velocity and frequency of
impacts on the leading hemisphere, which excavates a bright material—presumably ice—from the interior of the moon. '' images showing Amalthea's irregular shape (1997) and
Lyctos Facula are on the left side (on the
terminator). Bright spot underside is associated with crater
Gaea. Photo by
Galileo (2000) Amalthea is irregularly shaped, with the best
ellipsoidal approximation being . From this, Amalthea's surface area is likely between 88,000 and 170,000 square kilometers, or somewhere near 130,000. Like all other inner
moons of Jupiter, it is
tidally locked with the planet, with the long axis pointing towards Jupiter at all times. Its surface is heavily scarred by
craters, some of which are extremely large relative to the size of the moon:
Pan, the largest crater, measures 100 km across and is at least 8 km deep. Another crater,
Gaea, measures 80 km across and is likely twice as deep as Pan. Amalthea has several prominent bright spots, two of which are named. They are
Lyctos Facula and
Ida Facula, with a width reaching up to 25 km. They are located on the edge of ridges. Amalthea's irregular shape and large size led in the past to a conclusion that it is a fairly strong, rigid body, where it was argued that a body composed of ices or other weak materials would have been pulled into a more
spherical shape by its own gravity. However, on 5 November 2002, the
Galileo orbiter made a targeted flyby that came within 160 km of Amalthea, and the deflection of its orbit was used to compute the moon's mass (its volume had been calculated previously—to within 10% or so—from a careful analysis of all extant images). In the end, Amalthea's density was found to be as low as , so it must be either a relatively icy body or very porous "
rubble pile" or, more likely, something in between. Recent measurements of infrared spectra from the
Subaru telescope suggest that the moon indeed contains
hydrous minerals, indicating that it cannot have formed in its current position, since the hot primordial Jupiter would have melted it. It is therefore likely to have formed farther from the planet or to be a captured
Solar System body. No images were taken during this flyby (
Galileos cameras had been deactivated due to radiation damage in January 2002), and the resolution of other available images is generally low. Amalthea radiates slightly more heat than it receives from the
Sun, which is probably due to the influence of Jovian heat flux ( There are four named geological features on Amalthea: two craters and two (bright spots). The faculae are located on the edge of a ridge on the anti-Jupiter side of Amalthea. Craters are named after characters in
Greek mythology associated with
Zeus and Amalthea, and faculae are named after locations associated with
Zeus. == Relationship with Jupiter's rings ==