73982

73982 is an asteroid that has been studied as part of the Surveying and Ages of Solar System Objects (SASSO) program. It is a minor planet that orbits the Sun and is classified as a primitive Ph2-type asteroid within the outer regions of the asteroid belt.

Astronomical observations of 73982 have been conducted to gain insight into the asteroid's composition, size, and orbital characteristics. Studies show that 73982 is approximately 4 kilometers in diameter, suggesting that it may have retained a significant amount of primordial material from the early formation of the solar system.

The asteroid's orbit has been well-documented, with observations spanning multiple revolutions around the Sun. Astrometric measurements reveal that 73982 has an elongated orbital path, with its closest approach to the Sun occurring at a distance of 3.05 astronomical units (AU). It reaches its most distant point from the Sun at a distance of 4.42 AU.

Minor planets such as 73982 serve as valuable tools for understanding the formation and evolution of the asteroid belt. Continued monitoring and study of this and other primitive asteroids provide a unique window into the early structure and composition of the solar system.

Interdisciplinary research involving astrodynamics, planetary science, and materials analysis are all closely related to the study of objects like 73982. Such endeavors aim to improve our understanding of the underlying processes that shaped the inner solar system. While 73982 has received individual attention within scientific communities, broader implications for general scientific knowledge continue to unfold.