229098

229098 is a notable astronomical object, classified as a minor planet, located in the outer region of the asteroid belt. It was discovered on October 15, 1977, by astronomers at the Palomar Observatory in California, USA. The object is part of the Eos family of asteroids, which are named after the largest member of the group, 221 Eos. The Eos family is believed to have originated from a collisional event that occurred approximately 1.5 billion years ago.

229098 has an estimated diameter of about 12 kilometers, making it one of the larger asteroids in the Eos family. Its orbit around the Sun is relatively stable, with an average distance of about 3.1 astronomical units (AU). The asteroid completes one orbit around the Sun every 5.5 Earth years. The orbital eccentricity of 229098 is 0.12, indicating a slightly elliptical orbit.

The surface of 229098 is characterized by a low albedo, meaning it reflects only a small amount of sunlight. This suggests that the asteroid's surface is composed of dark, carbonaceous material. The spectral classification of 229098 is C-type, which is typical for many asteroids in the outer asteroid belt.

Due to its size and composition, 229098 is of interest to astronomers studying the formation and evolution of the solar system. The asteroid's membership in the Eos family provides valuable insights into the collisional history of the asteroid belt. Further observations and studies of 229098 will contribute to our understanding of the dynamic processes that shape the solar system.