336091

336091 is a minor planet in the outer region of the asteroid belt, orbiting the Sun at a distance of approximately 3.1 astronomical units (AU). It was discovered on October 10, 2005, by the Catalina Sky Survey, an astronomical survey project that aims to discover and track near-Earth objects and potentially hazardous asteroids. The minor planet is classified as a main-belt asteroid, which are asteroids that orbit the Sun between the orbits of Mars and Jupiter.

The orbital period of 336091 is approximately 5.6 Earth years, and its orbit has an eccentricity of 0.11, indicating a relatively circular orbit. The asteroid has an estimated diameter of about 2 kilometers, based on its absolute magnitude and assumed albedo. The rotation period of 336091 is not yet determined, but it is expected to be in the range of a few hours to a few days, similar to other main-belt asteroids.

The spectral classification of 336091 is not yet determined, but it is likely to be a C-type asteroid, which are carbonaceous asteroids that are among the most common types of asteroids in the asteroid belt. The composition of 336091 is not yet known, but it is expected to be similar to other C-type asteroids, which are thought to be composed of primitive, carbon-rich materials that have not been significantly altered since the formation of the Solar System.

The discovery and study of 336091 contribute to our understanding of the formation and evolution of the Solar System, as well as the composition and dynamics of the asteroid belt. Further observations and analysis of 336091 and other minor planets will help to refine our understanding of these fascinating objects and their role in the history of the Solar System.