While a large impact on Uranus when it was still surrounded by a protoplanetary disk would have eventually produced moons in
retrograde orbit around the planet, two or more smaller collisions had a much higher probability of generating the moons with the orbital direction observed today (Europlanet press release; and Phil Plait, Bad Astronomy Blog, Discover, October 7, 2011).
Not exact matches
Then we started finding some that were misaligned —
planets with tilted
orbits or
planets going
around their star in the opposite direction from its spin, in what we call a
retrograde orbit.
Then, each star's gravity caught the errant
planet and whipped it
around in a highly irregular, tight, and
retrograde orbit.