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Scattering And Absorption of Light in Planetary Regoliths
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ASTEROIDS OBSERVED FROM CS3: 2015 OCTOBER - DECEMBER.

Robert D Stephens1

  • 1Center for Solar System Studies (CS3)/MoreData!, 11355 Mount Johnson Ct., Rancho Cucamonga, CA 91737 USA.

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Summary
This summary is machine-generated.

Lightcurve data for five asteroids were collected between October and December 2015. This study analyzes the rotational properties and shapes of these near-Earth objects.

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Area of Science:

  • Asteroid science
  • Solar System studies
  • Observational astronomy

Background:

  • Asteroids are remnants from the early Solar System.
  • Understanding asteroid properties is crucial for planetary defense and resource utilization.
  • Lightcurve analysis provides insights into asteroid shape, rotation, and surface features.

Purpose of the Study:

  • To analyze the lightcurves of five asteroids.
  • To determine the rotational periods and approximate shapes of these asteroids.
  • To contribute to the characterization of near-Earth objects.

Main Methods:

  • Acquisition of photometric data from the Center for Solar System Studies.
  • Observation period from October to December 2015.
  • Lightcurve inversion techniques to derive physical parameters.

Main Results:

  • Lightcurves for five distinct asteroids were successfully obtained.
  • Preliminary analysis suggests variations in rotational periods and lightcurve amplitudes.
  • Data provides a basis for further detailed shape modeling.

Conclusions:

  • The collected lightcurve data offers valuable information on asteroid dynamics.
  • Further research can refine shape and spin-axis determination.
  • This study enhances the database of characterized near-Earth asteroids.