Speaker
Description
Near-Earth Objects (NEOs), encompassing both asteroids and comets, are celestial bodies whose trajectories bring them into proximity with Earth, presenting both scientific opportunities and potential collision risks. A comprehensive investigation of their physical characteristics, dynamical behaviors, and orbital evolutions is paramount for planetary defense strategies and advancing astrophysical knowledge. This study leverages the 1.88m telescope at the National Research Institute of Astronomy and Geophysics (NRIAG) in Egypt to conduct targeted observational campaigns of NEOs.
Employing cutting-edge ground-based optical observation techniques, we achieved high-precision detection, tracking, and characterization of multiple NEOs. Advanced astrometric and photometric data reduction pipelines enabled the determination of orbital elements, size estimations, and compositional analyses. These methodologies underscore the strategic potential of regional facilities in contributing to the global network of NEO monitoring and research.
This work not only reinforces the critical role of localized observatories in the global observational infrastructure but also provides vital insights into the distribution, behavior, and resource potential of NEO populations. The findings significantly enhance the collective understanding of NEO dynamics, informing planetary defense initiatives and future resource exploitation endeavors.