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ASTEROIDS OBSERVED FROM CS3: 2017 JANUARY - MARCH.

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 two Hungaria asteroids, offering insights into their physical characteristics. These observations contribute to our understanding of near-Earth asteroid populations.

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Area of Science:

  • Astronomy and astrophysics
  • Solar system exploration

Background:

  • The Hungaria asteroid group is a population of near-Earth asteroids with high inclinations.
  • Understanding their physical properties is crucial for asteroid research and hazard assessment.

Purpose of the Study:

  • To conduct CCD photometric observations of two specific Hungaria asteroids.
  • To gather data for analyzing the physical properties of these asteroids.

Main Methods:

  • Utilized CCD photometric techniques for data acquisition.
  • Observations were carried out from January to March 2017.
  • Data was obtained from the Center for Solar System Studies.

Main Results:

  • Acquired photometric data for two Hungaria asteroids.
  • The data provides a basis for further analysis of asteroid light curves and rotational periods.

Conclusions:

  • The collected photometric data will aid in characterizing the two Hungaria asteroids.
  • This research contributes to the broader study of small Solar System bodies.