4495

**4495** is a minor planet, or asteroid, in the outer regions of the asteroid belt between Mars and Jupiter. It was discovered on October 28, 1981, by astronomer Schelte J. Bus at the Siding Spring Observatory in New South Wales, Australia. The asteroid was officially numbered as asteroid 4495 and received its temporary designation of 1981 UH. Its orbit is relatively distant, with a semi-major axis of approximately 2.9 astronomical units (AU) from the Sun, placing it in the outer main belt.

4495 is classified as a carbonaceous asteroid, belonging to the C-type group, which are known for their dark surfaces and high carbon content. These asteroids are thought to be remnants from the early solar system, preserving materials from its formation. Observations have suggested that 4495 has a composition similar to other C-type asteroids, though precise spectral analysis remains limited due to its distance and faint brightness.

The asteroid has a rotational period of about 10.3 hours, which is typical for many main-belt objects. Its diameter is estimated to be around 13 kilometers, though these measurements can vary based on different observational techniques. There are no known moons or significant rotational irregularities associated with 4495.

No close approaches to Earth have been recorded for 4495, and its orbit does not pose any immediate or long-term risk. It is monitored as part of ongoing efforts to track near-Earth objects and understand the characteristics of distant asteroids. The asteroid’s study contributes to broader research on the composition, formation, and evolution of the solar system’s minor bodies.