245499

245499 is a minor planet located in the outer region of the asteroid belt, between the orbits of Mars and Jupiter. It was discovered on February 22, 2007, by the Catalina Sky Survey, an astronomical survey project that searches for near-Earth objects and comets. The discovery was made using a 0.68-meter Schmidt telescope located at the Mount Lemmon Observatory in Arizona, USA.

245499 has an estimated diameter of about 1.5 kilometers, based on its absolute magnitude and an assumed albedo. Its orbital period around the Sun is approximately 4.4 years, and it has an eccentric orbit with an inclination of about 12 degrees relative to the ecliptic plane. The asteroid's semi-major axis is roughly 2.6 astronomical units (AU), placing it in the outer part of the main asteroid belt.

The asteroid's rotation period is not well-determined, but it is estimated to be around 5 to 10 hours. The spectral classification of 245499 is not yet known, but it is likely to be a common S-type asteroid, which are composed mainly of silicate materials and nickel-iron.

245499 has not been observed to come close to Earth, and its orbit does not intersect with Earth's path around the Sun. Therefore, there is no immediate threat of a collision with our planet. However, as with all near-Earth objects, it is important to continue monitoring its orbit and any potential future close approaches to ensure public safety.

In summary, 245499 is a minor planet located in the outer asteroid belt, discovered in 2007. It has an eccentric orbit and an estimated diameter of about 1.5 kilometers. The asteroid's spectral classification and rotation period are not yet well-determined, but it is likely to be a common S-type asteroid. There is no immediate threat of a collision with Earth, and continued monitoring of its orbit is recommended.