195199

195199 is a minor planet in the asteroid belt, located between the orbits of Mars and Jupiter. It was discovered on October 26, 1971, by the Soviet astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, Ukraine. The asteroid is classified as a main-belt asteroid, which means it orbits the Sun within the asteroid belt's inner region.

The asteroid has an estimated diameter of about 10 kilometers (6.2 miles) based on its absolute magnitude. Its orbit is relatively stable, with an eccentricity of 0.12 and an inclination of 1.5 degrees relative to the ecliptic plane. The semi-major axis of its orbit is approximately 2.7 astronomical units (AU), which is the average distance from the Sun to Earth.

195199 has not been visited by any spacecraft, and little is known about its physical properties. Its spectral classification is not well-determined, but it is likely a stony asteroid based on its location in the asteroid belt. The asteroid's rotation period is not known, but it is likely to be several hours, similar to other main-belt asteroids.

The asteroid's name is a combination of the year of its discovery and the order of its discovery within that year. It is not named after a person, place, or mythological figure, unlike many other asteroids. The International Astronomical Union's Minor Planet Center assigns a provisional designation to newly discovered asteroids, which is replaced by a permanent number and name once the asteroid's orbit is well-determined and its identity is confirmed.

In summary, 195199 is a minor planet in the asteroid belt, discovered in 1971. It is a stony asteroid with an estimated diameter of about 10 kilometers and a stable orbit. Little is known about its physical properties, and it has not been visited by any spacecraft. Its name is a combination of the year of its discovery and the order of its discovery within that year.