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It is the first object that turned out to be a quasi-satellite of Pluto.
It was the first quasi-satellite to be discovered around a major planet in the Solar System.
In fact, Cruithne was discovered in 1986 and is actually a quasi-satellite.
As quasi-satellite, this minor body is trapped in a 1:1 mean motion resonance with Venus.
It is a quasi-satellite of Earth.
When viewed from the perspective of the planet, the quasi-satellite will appear to travel in an oblong retrograde loop around the planet.
The station is a quasi-satellite of WWGE in Loretto.
This dynamical behavior is recurrent, the object becomes a quasi-satellite of Pluto every 2 Myr and remains in that configuration for nearly 350,000 years.
A quasi-satellite's orbit around the Sun takes exactly the same time as the planet's, but has a different eccentricity (usually greater), as shown in the diagram on the right.
From a co-rotating perspective the quasi-satellite appears to orbit the primary like a retrograde satellite, although at distances so large that it is not gravitionally bound to it.
A quasi-satellite is an object in a specific type of co-orbital configuration (1:1 orbital resonance) with a planet where the object stays close to that planet over many orbital periods.
M. Connors, P. Chodas, S. Mikkola, P. Wiegert, C. Veillet, K. Innanen: Discovery of an asteroid and quasi-satellite in an Earth-like horseshoe orbit.
Other planets Based on simulations it is believed that Uranus and Neptune could potentially hold quasi-satellites for the age of the Solar System (about 4.5 billion years), but a quasi-satellite's orbit would remain stable for only 10 million years near Jupiter and 100,000 years near Saturn.
Wörterbuch für Astronomie