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PRELIMINARY POLE AND SHAPE MODELS FOR THREE NEAR-EARTH ASTEROIDS.

Brian D Warner1, Petr Pravec2, Peter Kusnirak2

  • 1Center for Solar System Studies / MoreData!, 446 Sycamore Ave., Eaton, CO 80615 USA.

The Minor Planet Bulletin
|April 8, 2020
PubMed
Summary

Researchers developed preliminary pole and shape models for three near-Earth asteroids (NEAs) using observational data collected from 1993 to 2016. This study provides new insights into the physical characteristics of these celestial bodies.

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Area of Science:

  • Astronomy and astrophysics
  • Planetary science

Background:

  • Near-Earth asteroids (NEAs) pose potential impact risks and are crucial for understanding solar system evolution.
  • Characterizing NEAs' physical properties, such as shape and rotation, is essential for hazard assessment and mission planning.

Purpose of the Study:

  • To determine preliminary pole and shape models for three specific near-Earth asteroids: 1863 Antinous, (5836) 1993 MF, and (154244) 2002 KL6.
  • To contribute to the growing database of physical properties for potentially hazardous asteroids.

Main Methods:

  • Photometric observations of the selected NEAs were conducted over a period spanning from 1993 to 2016.
  • Collected observational data were processed to derive rotational parameters and reconstruct three-dimensional shape models.

Main Results:

  • Preliminary pole and shape models were successfully generated for 1863 Antinous, (5836) 1993 MF, and (154244) 2002 KL6.
  • The derived models offer initial insights into the physical configurations and rotational states of these NEAs.

Conclusions:

  • The study successfully established initial physical models for three NEAs, enhancing our understanding of their morphology and dynamics.
  • These findings serve as a foundation for more detailed future investigations and refined risk assessments of near-Earth objects.