45827

45827 is a minor planet located in the outer region of the asteroid belt between Mars and Jupiter. It was discovered on November 16, 1994, by astronomers working at the Spacewatch program at Kitt Peak National Observatory in Arizona, United States. The object was officially designated as 1994 WJ2 upon its discovery before receiving its permanent numbering.

The asteroid belongs to the outer main-belt population, orbiting the Sun at an average distance of approximately 3.1 astronomical units (AU). Its orbital period is roughly 5.5 years, and its orbit has a moderate inclination of about 10 degrees relative to the ecliptic plane. The asteroid’s name has not yet been officially assigned, as the naming process typically requires further study of its physical properties or historical significance.

45827 is classified as a carbonaceous (C-type) asteroid, which means its surface is composed primarily of carbon-rich materials, including silicates and possibly organic compounds. These types of asteroids are among the most common in the outer asteroid belt and are believed to contain primitive material from the early solar system. Observations suggest that 45827 has a relatively dark surface, reflecting only a small fraction of incoming sunlight.

Due to its size—estimated to be around 5 kilometers (3.1 miles) in diameter—45827 is not large enough to be classified as a dwarf planet. It remains an object of interest for astronomers studying the composition and dynamics of the asteroid belt. No known moons or unusual features have been documented for this asteroid, and it does not pose any significant threat of Earth impact. Further observations, particularly from space-based telescopes or future missions, could provide additional insights into its physical characteristics.