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ASTEROIDS OBSERVED FROM CS3: 2018 JULY - SEPTEMBER.

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.

This study presents new photometric data for 10 main-belt asteroids. These observations contribute to our understanding of asteroid physical properties and orbital dynamics.

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Area of Science:

  • Astronomy and Astrophysics
  • Planetary Science

Background:

  • Main-belt asteroids represent the majority of known asteroids.
  • Understanding their physical characteristics is crucial for solar system formation models.

Purpose of the Study:

  • To present new CCD photometric data for 10 main-belt asteroids.
  • To contribute to the characterization of asteroid physical properties.

Main Methods:

  • CCD photometric observations were conducted.
  • Data were acquired from the Center for Solar System Studies.
  • Observations spanned from July to September 2018.

Main Results:

  • Photometric data for 10 main-belt asteroids were successfully obtained.
  • The dataset provides light curves and potentially other photometric information.

Conclusions:

  • The collected data will aid in determining asteroid sizes, shapes, and rotation periods.
  • This research enhances the database of asteroid physical properties for future studies.