Pasiphae group
The Pasiphae group is a group of retrograde irregular satellites of Jupiter that follow similar orbits to Pasiphae and are thought to have a common origin.
Their semi-major axes (distances from Jupiter) range between 22.8 and 24.1 million km (the same range as the Carme group), their inclinations between 144.5° and 158.3°, and their eccentricities between 0.25 and 0.43.
Core members of the group include (from the largest to the smallest):
Pasiphae
Sinope, two-thirds the size of Pasiphae
Callirrhoe
Megaclite
Autonoe
Eurydome
Sponde
The International Astronomical Union (IAU) reserves names ending in -e for all retrograde moons, including this group's members.
Origin
The Pasiphae group is believed to have been formed when Jupiter captured an asteroid which subsequently broke up after a collision. The original asteroid was not disturbed heavily: the original body is calculated to have been 60 km in diameter, about the same size as Pasiphae; Pasiphae retains 99% of the original body's mass. However, if Sinope belongs to the group, the ratio is much smaller, 87%.