94129

The designation **94129** is primarily associated with the **International Astronomical Union’s (IAU) Minor Planet Center**, where it is cataloged as an asteroid in the main belt. Discovered on **October 19, 1996**, by astronomers at the **Lincoln Near-Earth Asteroid Research (LINEAR)** program in New Mexico, the object was later classified as a member of the **Florence asteroid family**, a group of space rocks sharing similar orbital characteristics.

94129 is classified as a **main-belt asteroid**, meaning it orbits the Sun between Mars and Jupiter. Its approximate diameter is estimated to be around **4.7 kilometers (2.9 miles)**, and it follows a relatively stable orbit with a period of roughly **3.6 years**. Due to its size and distance from Earth, it is not considered a near-Earth object (NEO) and poses no known threat of collision with our planet.

The asteroid has been studied for its orbital dynamics and composition, contributing to broader research on the formation and evolution of the solar system. Its designation follows the IAU’s naming conventions for minor planets, where numbers are assigned sequentially based on discovery date rather than any specific significance.

While 94129 lacks a formal name, it remains an object of interest in asteroid tracking and astronomical surveys. Observations continue to refine its orbital parameters and help scientists better understand the distribution and behavior of main-belt asteroids.