S/2003 J9 is a member of the Carme group, a family of Jovian satellites which have similar orbits and appearance and are therefore thought to have a common origin. The group probably began as a D-type asteroid (possibly from the Hilda family or the Jupiter Trojans) that suffered a collision, which broke off a number of pieces, either before or after being captured by Jupiter's gravity. The largest remaining chunk (still retaining 99% of the group's mass) was named "Carme," and the smaller pieces became the other 16 moons in the Carme group.
All of the Carme moons are retrograde, which means that they orbit Jupiter in the opposite direction from the planet's rotation. Their orbits are also eccentric (elliptical rather than circular) and highly inclined with respect to Jupiter's equatorial plane. They all are very similar in color -- light red -- except for Kalyke, which is considerably redder than the others. All of these characteristics support the idea that the Carme satellites began as a captured asteroid, rather than forming as part of the original Jupiter system. None of the Carme members is massive enough to pull itself into a sphere, so they are probably all irregularly shaped.
S/2003 J9 has a mean radius of about 0.5 kilometer. At a mean distance of about 23.4 million km from Jupiter, the satellite takes about 733 Earth days to complete one orbit.
S/2003 J9 was discovered in February 2003 by Scott Sander Sheppard Sheppard at the Mauna Kea Observatory in Hawaii.
How S/2003 J9 Got its Name:
S/2003 J9 was so designated because it is a satellite (S) that was discovered in 2003, and was the 9th satellite of Jupiter (J) to be found that year.