104761

104761, also known as 2002 RX12, is a minor planet that orbits within the inner regions of the asteroid belt. Discovered on September 5, 2002, by astronomers at the LINEAR (Lincoln Near-Earth Asteroid Research) program, it is classified as a near-Earth object (NEO) due to its proximity to Earth's orbit. The minor planet has an estimated diameter of about 500 meters, making it a sizable body within the vast population of asteroids.

The orbit of 104761 places it between the larger planets Mars and Jupiter, with an average distance of approximately 2.5 astronomical units (AU) from the Sun. Its orbital period is around 3.5 years, completing one full orbit in this time frame. The minor planet’s orbit is characterized by moderate eccentricity and inclination, indicating a somewhat elliptical and moderately tilted path relative to the plane of the solar system.

The surface composition of 104761 is not well understood, but it is believed to be composed of common asteroid materials such as silicates and metals. Its rotation period, which describes the time it takes to complete one rotation on its axis, has not been precisely determined, but it is assumed to fall within typical ranges for NEOs.

As a near-Earth object, 104761 is of interest to astronomers and planetary scientists who study the potential impact threats it may pose. Given its size and orbit, it is regularly monitored to ensure no immediate threat to Earth exists. The tracking and study of such objects are crucial for understanding the dynamics of the asteroid belt and the broader solar system.