The moon is the most visible object in the night sky, but it’s not the only one that orbits the Earth. There are also some small satellites called “quasi-satellites” that follow a similar path around our planet.
One of these quasi-satellites is a near-Earth asteroid named Kamo’oalewa. It was discovered in 2016 by a telescope in Hawaii. It has a shiny surface that reflects light like the moon does. But could it actually be part of the moon?
A new study suggests that Kamo’oalewa might have originated from the moon as a result of a collision with another object. The study, published in the journal Icarus, analyzed the orbit of Kamo’oalewa and compared it with other possible sources of lunar ejecta.
Kamo’oalewa is not a typical satellite. It is outside the Earth’s Hill Sphere, which is the region where the Earth’s gravity dominates over other forces. The moon is inside the Hill Sphere, and its orbit is relatively stable. But Kamo’oalewa is outside the sphere, and its orbit changes over time due to the influence of other planets.
Kamo’oalewa belongs to a group of asteroids called Apollo asteroids, which cross the Earth’s orbit. It is the smallest, closest, and most stable member of this group. It also belongs to a category of co-orbitals, which are objects that share an orbit with a larger body. There are three types of co-orbitals: Trojans, horseshoe, and retrograde/quasi-satellites.
Kamo’oalewa is a quasi-satellite, which means it orbits around the sun in the opposite direction as the Earth, but stays close to the Earth as if it were a satellite. It is one of only five known quasi-satellites of the Earth.
The researchers used computer simulations to test different scenarios for how Kamo’oalewa could have become a quasi-satellite. They found that the most likely scenario was that Kamo’oalewa was ejected from the moon by an impact with another object about 100 million years ago. The impact gave Kamo’oalewa enough speed and direction to escape the moon’s gravity and enter an orbit around the sun.
The researchers also found that Kamo’oalewa could remain a quasi-satellite for another 300 years before becoming a horseshoe co-orbital or leaving the Earth’s vicinity altogether.
The study provides new insights into the origin and evolution of quasi-satellites and other co-orbitals. It also shows that Kamo’oalewa might be a piece of lunar history that we can observe from Earth.
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