- #1
Hornbein
- 2,700
- 2,248
A quasi-moon of Earth is a rock to that orbits both the Earth and Sun with the same solar orbital period as Earth.
A quasi-moon is a natural satellite that is in a temporary orbit around a planet but does not have a stable, long-term orbit. These objects often originate from the asteroid belt or other regions and can be captured by a planet's gravitational field for a limited time before either escaping back into space or colliding with the planet.
Quasi-moons typically form when an object, such as an asteroid, passes close to a planet and is captured by its gravitational pull. The conditions for capture depend on the object's velocity, trajectory, and the gravitational influence of the planet. If the conditions are right, the object can enter a temporary orbit around the planet.
The duration of a quasi-moon's orbit can vary widely, ranging from a few weeks to several years. The lifespan of a quasi-moon is influenced by factors such as gravitational interactions with the planet and other nearby celestial bodies, as well as the object's size and composition, which can affect its stability in orbit.
Yes, there are several known quasi-moons in our solar system. One of the most notable examples is 2020 CD3, a small asteroid that was temporarily captured by Earth's gravity in early 2020. Such objects are often detected through telescopic observations and are classified as temporary satellites or quasi-satellites.
In general, quasi-moons do not become permanent moons due to their unstable orbits and the conditions required for capture. However, in rare cases, if a quasi-moon can lose enough energy through interactions with other bodies or through atmospheric drag, it may settle into a more stable orbit and become a permanent moon, although this is quite uncommon.