10182

10182 is a small main-belt asteroid discovered by the Palomar Observatory on March 3, 1981. It is classified as an S-type asteroid, indicating a stony composition. Its orbital period is approximately 3.4 years, and it has a semi-major axis of about 2.2 astronomical units. The asteroid's size is estimated to be around 3 to 7 kilometers in diameter. Its absolute magnitude is 14.7, which is a measure of its intrinsic brightness. Like other asteroids in the main belt, 10182 is thought to be a remnant from the early formation of the solar system, a rocky body that never coalesced into a planet. Its precise characteristics, such as albedo and rotation period, are still subjects of ongoing astronomical observation and analysis. Further study of asteroids like 10182 helps scientists understand the composition and evolution of the inner solar system.