Metis was once considered to be a member of an
asteroid family known as the Metis family, but more recent searches for prominent families did not recognize any such group, nor is a clump evident in the vicinity of Metis by visual inspection of
proper orbital element diagrams. However, a spectroscopic analysis found strong spectral similarities between Metis and
113 Amalthea, and it is suggested that these asteroids may be remnants of a very old (at least ~1
Ga) dynamical family whose smaller members have been pulverised by collisions or perturbed away from the vicinity. The putative parent body is estimated to have been 300 to 600 km in diameter (
Vesta-sized) and
differentiated. Metis would be the relatively intact core remnant (though smaller than
16 Psyche), and Amalthea a fragment of the mantle, with 90% of the original body unaccounted for. Coincidentally, both Metis and Amalthea have namesakes among
Jupiter's inner moons. ==Occultations==