Nutikus

Nutikus is a small celestial body classified as an asteroid, located within the asteroid belt between Mars and Jupiter. Discovered on December 12, 1985, by astronomer Dr. Laura Martinez at the Cerro Tololo Inter-American Observatory, Nutikus has since become an object of interest for astronomers studying minor planets.

The asteroid has an approximate diameter of 15 kilometers and exhibits a carbonaceous (C-type) composition, indicating a rich presence of carbon and other organic compounds. Its orbit has a semi-major axis of about 2.5 astronomical units (AU), with an orbital period of approximately 3.97 years. Nutikus's orbit is characterized by a moderate eccentricity and an inclination of around 10 degrees relative to the plane of the solar system.

Nutikus is not classified as a near-Earth object (NEO) and poses no imminent threat to Earth. Its relative brightness and orbit make it accessible for observation through mid-sized telescopes, and it has been included in several observational campaigns aimed at understanding the diversity and composition of main-belt asteroids.

As of current knowledge, Nutikus does not have any known satellites or accompanying debris. Its surface features are primarily characterized by dark, primitive material, consistent with its C-type classification. Ongoing studies focus on its composition, rotation period, and potential as a target for future exploration missions to better understand the early solar system's formation processes.